[{"article_type":"original","page":"443-447","publication":"Proceedings of the Edinburgh Mathematical Society","citation":{"ama":"Lenz D, Weinmann T, Wirth M. Self-adjoint extensions of bipartite Hamiltonians. Proceedings of the Edinburgh Mathematical Society. 2021;64(3):443-447. doi:10.1017/S0013091521000080","ista":"Lenz D, Weinmann T, Wirth M. 2021. Self-adjoint extensions of bipartite Hamiltonians. Proceedings of the Edinburgh Mathematical Society. 64(3), 443–447.","apa":"Lenz, D., Weinmann, T., & Wirth, M. (2021). Self-adjoint extensions of bipartite Hamiltonians. Proceedings of the Edinburgh Mathematical Society. Cambridge University Press. https://doi.org/10.1017/S0013091521000080","ieee":"D. Lenz, T. Weinmann, and M. Wirth, “Self-adjoint extensions of bipartite Hamiltonians,” Proceedings of the Edinburgh Mathematical Society, vol. 64, no. 3. Cambridge University Press, pp. 443–447, 2021.","mla":"Lenz, Daniel, et al. “Self-Adjoint Extensions of Bipartite Hamiltonians.” Proceedings of the Edinburgh Mathematical Society, vol. 64, no. 3, Cambridge University Press, 2021, pp. 443–47, doi:10.1017/S0013091521000080.","short":"D. Lenz, T. Weinmann, M. Wirth, Proceedings of the Edinburgh Mathematical Society 64 (2021) 443–447.","chicago":"Lenz, Daniel, Timon Weinmann, and Melchior Wirth. “Self-Adjoint Extensions of Bipartite Hamiltonians.” Proceedings of the Edinburgh Mathematical Society. Cambridge University Press, 2021. https://doi.org/10.1017/S0013091521000080."},"date_published":"2021-08-01T00:00:00Z","scopus_import":"1","day":"01","article_processing_charge":"No","title":"Self-adjoint extensions of bipartite Hamiltonians","status":"public","intvolume":" 64","user_id":"4359f0d1-fa6c-11eb-b949-802e58b17ae8","_id":"9627","oa_version":"Published Version","type":"journal_article","abstract":[{"lang":"eng","text":"We compute the deficiency spaces of operators of the form 𝐻𝐴⊗̂ 𝐼+𝐼⊗̂ 𝐻𝐵, for symmetric 𝐻𝐴 and self-adjoint 𝐻𝐵. This enables us to construct self-adjoint extensions (if they exist) by means of von Neumann's theory. The structure of the deficiency spaces for this case was asserted already in Ibort et al. [Boundary dynamics driven entanglement, J. Phys. A: Math. Theor. 47(38) (2014) 385301], but only proven under the restriction of 𝐻𝐵 having discrete, non-degenerate spectrum."}],"issue":"3","isi":1,"quality_controlled":"1","main_file_link":[{"url":"https://doi.org/10.1017/S0013091521000080","open_access":"1"}],"oa":1,"external_id":{"arxiv":["1912.03670"],"isi":["000721363700003"]},"language":[{"iso":"eng"}],"doi":"10.1017/S0013091521000080","month":"08","publication_identifier":{"issn":["0013-0915"],"eissn":["1464-3839"]},"publication_status":"published","department":[{"_id":"JaMa"}],"publisher":"Cambridge University Press","year":"2021","acknowledgement":"M. W. gratefully acknowledges financial support by the German Academic Scholarship Foundation (Studienstiftung des deutschen Volkes). T.W. thanks PAO Gazprom Neft, the Euler International Mathematical Institute in Saint Petersburg and ORISA GmbH for their financial support in the form of scholarships during his Master's and Bachelor's studies respectively. The authors want to thank Mark Malamud for pointing out the reference [1] to them. This work was supported by the Ministry of Science and Higher Education of the Russian Federation, agreement No 075-15-2019-1619.","date_created":"2021-07-04T22:01:24Z","date_updated":"2023-08-17T07:12:05Z","volume":64,"author":[{"full_name":"Lenz, Daniel","first_name":"Daniel","last_name":"Lenz"},{"last_name":"Weinmann","first_name":"Timon","full_name":"Weinmann, Timon"},{"last_name":"Wirth","first_name":"Melchior","orcid":"0000-0002-0519-4241","id":"88644358-0A0E-11EA-8FA5-49A33DDC885E","full_name":"Wirth, Melchior"}]},{"doi":"10.1007/s00222-021-01041-5","language":[{"iso":"eng"}],"tmp":{"name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)","image":"/images/cc_by.png"},"oa":1,"external_id":{"arxiv":["2005.08933"],"isi":["000646573600001"]},"quality_controlled":"1","isi":1,"project":[{"name":"IST Austria Open Access Fund","_id":"B67AFEDC-15C9-11EA-A837-991A96BB2854"},{"_id":"25C6DC12-B435-11E9-9278-68D0E5697425","grant_number":"694227","name":"Analysis of quantum many-body systems","call_identifier":"H2020"}],"month":"05","publication_identifier":{"eissn":["1432-1297"],"issn":["0020-9910"]},"author":[{"full_name":"Benedikter, Niels P","first_name":"Niels P","last_name":"Benedikter","id":"3DE6C32A-F248-11E8-B48F-1D18A9856A87","orcid":"0000-0002-1071-6091"},{"full_name":"Nam, Phan Thành","last_name":"Nam","first_name":"Phan Thành"},{"full_name":"Porta, Marcello","last_name":"Porta","first_name":"Marcello"},{"last_name":"Schlein","first_name":"Benjamin","full_name":"Schlein, Benjamin"},{"full_name":"Seiringer, Robert","first_name":"Robert","last_name":"Seiringer","id":"4AFD0470-F248-11E8-B48F-1D18A9856A87","orcid":"0000-0002-6781-0521"}],"date_updated":"2023-08-21T06:30:30Z","date_created":"2020-05-28T16:48:20Z","volume":225,"acknowledgement":"We thank Christian Hainzl for helpful discussions and a referee for very careful reading of the paper and many helpful suggestions. NB and RS were supported by the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (grant agreement No. 694227). Part of the research of NB was conducted on the RZD18 Nice–Milan–Vienna–Moscow. NB thanks Elliott H. Lieb and Peter Otte for explanations about the Luttinger model. PTN has received funding from the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) under Germany’s Excellence Strategy (EXC-2111-390814868). MP acknowledges financial support from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (ERC StG MaMBoQ, grant agreement No. 802901). BS gratefully acknowledges financial support from the NCCR SwissMAP, from the Swiss National Science Foundation through the Grant “Dynamical and energetic properties of Bose-Einstein condensates” and from the European Research Council through the ERC-AdG CLaQS (grant agreement No. 834782). All authors acknowledge support for workshop participation from Mathematisches Forschungsinstitut Oberwolfach (Leibniz Association). NB, PTN, BS, and RS acknowledge support for workshop participation from Fondation des Treilles.","year":"2021","publication_status":"published","publisher":"Springer","department":[{"_id":"RoSe"}],"file_date_updated":"2022-05-16T12:23:40Z","ec_funded":1,"license":"https://creativecommons.org/licenses/by/4.0/","date_published":"2021-05-03T00:00:00Z","publication":"Inventiones Mathematicae","citation":{"ama":"Benedikter NP, Nam PT, Porta M, Schlein B, Seiringer R. Correlation energy of a weakly interacting Fermi gas. Inventiones Mathematicae. 2021;225:885-979. doi:10.1007/s00222-021-01041-5","ista":"Benedikter NP, Nam PT, Porta M, Schlein B, Seiringer R. 2021. Correlation energy of a weakly interacting Fermi gas. Inventiones Mathematicae. 225, 885–979.","apa":"Benedikter, N. P., Nam, P. T., Porta, M., Schlein, B., & Seiringer, R. (2021). Correlation energy of a weakly interacting Fermi gas. Inventiones Mathematicae. Springer. https://doi.org/10.1007/s00222-021-01041-5","ieee":"N. P. Benedikter, P. T. Nam, M. Porta, B. Schlein, and R. Seiringer, “Correlation energy of a weakly interacting Fermi gas,” Inventiones Mathematicae, vol. 225. Springer, pp. 885–979, 2021.","mla":"Benedikter, Niels P., et al. “Correlation Energy of a Weakly Interacting Fermi Gas.” Inventiones Mathematicae, vol. 225, Springer, 2021, pp. 885–979, doi:10.1007/s00222-021-01041-5.","short":"N.P. Benedikter, P.T. Nam, M. Porta, B. Schlein, R. Seiringer, Inventiones Mathematicae 225 (2021) 885–979.","chicago":"Benedikter, Niels P, Phan Thành Nam, Marcello Porta, Benjamin Schlein, and Robert Seiringer. “Correlation Energy of a Weakly Interacting Fermi Gas.” Inventiones Mathematicae. Springer, 2021. https://doi.org/10.1007/s00222-021-01041-5."},"article_type":"original","page":"885-979","day":"03","article_processing_charge":"Yes (via OA deal)","has_accepted_license":"1","scopus_import":"1","oa_version":"Published Version","file":[{"file_id":"11386","relation":"main_file","date_created":"2022-05-16T12:23:40Z","date_updated":"2022-05-16T12:23:40Z","success":1,"checksum":"f38c79dfd828cdc7f49a34b37b83d376","file_name":"2021_InventMath_Benedikter.pdf","access_level":"open_access","creator":"dernst","file_size":1089319,"content_type":"application/pdf"}],"_id":"7901","user_id":"4359f0d1-fa6c-11eb-b949-802e58b17ae8","status":"public","ddc":["510"],"title":"Correlation energy of a weakly interacting Fermi gas","intvolume":" 225","abstract":[{"lang":"eng","text":"We derive rigorously the leading order of the correlation energy of a Fermi gas in a scaling regime of high density and weak interaction. The result verifies the prediction of the random-phase approximation. Our proof refines the method of collective bosonization in three dimensions. We approximately diagonalize an effective Hamiltonian describing approximately bosonic collective excitations around the Hartree–Fock state, while showing that gapless and non-collective excitations have only a negligible effect on the ground state energy."}],"type":"journal_article"},{"keyword":["Space and Planetary Science","Astronomy and Astrophysics"],"scopus_import":"1","day":"27","article_processing_charge":"No","article_type":"original","publication":"The Astrophysical Journal","citation":{"short":"E. Berzin, A. Secunda, R. Cen, A. Menegas, Y.L.L. Götberg, The Astrophysical Journal 918 (2021).","mla":"Berzin, Elizabeth, et al. “Spectral Signatures of Population III and Envelope-Stripped Stars in Galaxies at the Epoch of Reionization.” The Astrophysical Journal, vol. 918, no. 1, 5, American Astronomical Society, 2021, doi:10.3847/1538-4357/ac0af6.","chicago":"Berzin, Elizabeth, Amy Secunda, Renyue Cen, Alexander Menegas, and Ylva Louise Linsdotter Götberg. “Spectral Signatures of Population III and Envelope-Stripped Stars in Galaxies at the Epoch of Reionization.” The Astrophysical Journal. American Astronomical Society, 2021. https://doi.org/10.3847/1538-4357/ac0af6.","ama":"Berzin E, Secunda A, Cen R, Menegas A, Götberg YLL. Spectral signatures of population III and envelope-stripped stars in galaxies at the epoch of reionization. The Astrophysical Journal. 2021;918(1). doi:10.3847/1538-4357/ac0af6","apa":"Berzin, E., Secunda, A., Cen, R., Menegas, A., & Götberg, Y. L. L. (2021). Spectral signatures of population III and envelope-stripped stars in galaxies at the epoch of reionization. The Astrophysical Journal. American Astronomical Society. https://doi.org/10.3847/1538-4357/ac0af6","ieee":"E. Berzin, A. Secunda, R. Cen, A. Menegas, and Y. L. L. Götberg, “Spectral signatures of population III and envelope-stripped stars in galaxies at the epoch of reionization,” The Astrophysical Journal, vol. 918, no. 1. American Astronomical Society, 2021.","ista":"Berzin E, Secunda A, Cen R, Menegas A, Götberg YLL. 2021. Spectral signatures of population III and envelope-stripped stars in galaxies at the epoch of reionization. The Astrophysical Journal. 918(1), 5."},"date_published":"2021-08-27T00:00:00Z","type":"journal_article","abstract":[{"lang":"eng","text":"While most simulations of the epoch of reionization have focused on single-stellar populations in star-forming dwarf galaxies, products of binary evolution are expected to significantly contribute to emissions of hydrogen-ionizing photons. Among these products are stripped stars (or helium stars), which have their envelopes stripped from interactions with binary companions, leaving an exposed helium core. Previous work has suggested these stripped stars can dominate the Lyman Continuum (LyC) photon output of high-redshift, low-luminosity galaxies post-starburst. Other sources of hard radiation in the early universe include zero-metallicity Population iii stars, which may have similar spectral energy distribution (SED) properties to galaxies with radiation dominated by stripped-star emissions. Here, we use four metrics (the power-law exponent over wavelength intervals 240–500 Å, 600–900 Å, and 1200–2000 Å, and the ratio of total luminosity in FUV wavelengths to LyC wavelengths) to compare the SEDs of simulated galaxies with only single-stellar evolution, galaxies containing stripped stars, and galaxies containing Population iii stars, with four different initial mass functions (IMFs). We find that stripped stars significantly alter SEDs in the LyC range of galaxies at the epoch of reionization. SEDs in galaxies with stripped stars have lower power-law indices in the LyC range and lower FUV to LyC luminosity ratios. These differences in SEDs are present at all considered luminosities (${M}_{\\mathrm{UV}}\\gt -15$, AB system), and are most pronounced for lower-luminosity galaxies. Intrinsic SEDs as well as those with interstellar medium absorption of galaxies with stripped stars and Population iii stars are found to be distinct for all tested Population iii IMFs."}],"issue":"1","title":"Spectral signatures of population III and envelope-stripped stars in galaxies at the epoch of reionization","status":"public","intvolume":" 918","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","_id":"13456","oa_version":"Published Version","month":"08","publication_identifier":{"issn":["0004-637X"],"eissn":["1538-4357"]},"quality_controlled":"1","oa":1,"external_id":{"arxiv":["2102.08408"]},"main_file_link":[{"open_access":"1","url":"https://doi.org/10.3847/1538-4357/ac0af6"}],"language":[{"iso":"eng"}],"doi":"10.3847/1538-4357/ac0af6","article_number":"5","extern":"1","publication_status":"published","publisher":"American Astronomical Society","year":"2021","date_created":"2023-08-03T10:11:24Z","date_updated":"2023-08-21T11:44:50Z","volume":918,"author":[{"first_name":"Elizabeth","last_name":"Berzin","full_name":"Berzin, Elizabeth"},{"first_name":"Amy","last_name":"Secunda","full_name":"Secunda, Amy"},{"full_name":"Cen, Renyue","last_name":"Cen","first_name":"Renyue"},{"first_name":"Alexander","last_name":"Menegas","full_name":"Menegas, Alexander"},{"full_name":"Götberg, Ylva Louise Linsdotter","id":"d0648d0c-0f64-11ee-a2e0-dd0faa2e4f7d","orcid":"0000-0002-6960-6911","first_name":"Ylva Louise Linsdotter","last_name":"Götberg"}]},{"language":[{"iso":"eng"}],"doi":"10.3847/2041-8213/ac0b42","quality_controlled":"1","external_id":{"arxiv":["2104.03317"]},"main_file_link":[{"url":"https://arxiv.org/abs/2104.03317","open_access":"1"}],"oa":1,"publication_identifier":{"eissn":["2041-8213"],"issn":["2041-8205"]},"month":"07","volume":916,"date_updated":"2023-08-21T11:37:48Z","date_created":"2023-08-03T10:11:45Z","author":[{"full_name":"Vartanyan, David","first_name":"David","last_name":"Vartanyan"},{"full_name":"Laplace, Eva","first_name":"Eva","last_name":"Laplace"},{"full_name":"Renzo, Mathieu","first_name":"Mathieu","last_name":"Renzo"},{"full_name":"Götberg, Ylva Louise Linsdotter","last_name":"Götberg","first_name":"Ylva Louise Linsdotter","orcid":"0000-0002-6960-6911","id":"d0648d0c-0f64-11ee-a2e0-dd0faa2e4f7d"},{"full_name":"Burrows, Adam","last_name":"Burrows","first_name":"Adam"},{"last_name":"de Mink","first_name":"Selma E.","full_name":"de Mink, Selma E."}],"publisher":"American Astronomical Society","publication_status":"published","year":"2021","extern":"1","article_number":"L5","date_published":"2021-07-23T00:00:00Z","article_type":"original","citation":{"chicago":"Vartanyan, David, Eva Laplace, Mathieu Renzo, Ylva Louise Linsdotter Götberg, Adam Burrows, and Selma E. de Mink. “Binary-Stripped Stars as Core-Collapse Supernovae Progenitors.” The Astrophysical Journal Letters. American Astronomical Society, 2021. https://doi.org/10.3847/2041-8213/ac0b42.","short":"D. Vartanyan, E. Laplace, M. Renzo, Y.L.L. Götberg, A. Burrows, S.E. de Mink, The Astrophysical Journal Letters 916 (2021).","mla":"Vartanyan, David, et al. “Binary-Stripped Stars as Core-Collapse Supernovae Progenitors.” The Astrophysical Journal Letters, vol. 916, no. 1, L5, American Astronomical Society, 2021, doi:10.3847/2041-8213/ac0b42.","ieee":"D. Vartanyan, E. Laplace, M. Renzo, Y. L. L. Götberg, A. Burrows, and S. E. de Mink, “Binary-stripped stars as core-collapse supernovae progenitors,” The Astrophysical Journal Letters, vol. 916, no. 1. American Astronomical Society, 2021.","apa":"Vartanyan, D., Laplace, E., Renzo, M., Götberg, Y. L. L., Burrows, A., & de Mink, S. E. (2021). Binary-stripped stars as core-collapse supernovae progenitors. The Astrophysical Journal Letters. American Astronomical Society. https://doi.org/10.3847/2041-8213/ac0b42","ista":"Vartanyan D, Laplace E, Renzo M, Götberg YLL, Burrows A, de Mink SE. 2021. Binary-stripped stars as core-collapse supernovae progenitors. The Astrophysical Journal Letters. 916(1), L5.","ama":"Vartanyan D, Laplace E, Renzo M, Götberg YLL, Burrows A, de Mink SE. Binary-stripped stars as core-collapse supernovae progenitors. The Astrophysical Journal Letters. 2021;916(1). doi:10.3847/2041-8213/ac0b42"},"publication":"The Astrophysical Journal Letters","article_processing_charge":"No","day":"23","keyword":["Space and Planetary Science","Astronomy and Astrophysics"],"scopus_import":"1","oa_version":"Preprint","intvolume":" 916","title":"Binary-stripped stars as core-collapse supernovae progenitors","status":"public","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","_id":"13458","issue":"1","abstract":[{"text":"Most massive stars experience binary interactions in their lifetimes that can alter both the surface and core structure of the stripped star with significant effects on their ultimate fate as core-collapse supernovae. However, core-collapse supernovae simulations to date have focused almost exclusively on the evolution of single stars. We present a systematic simulation study of single and binary-stripped stars with the same initial mass as candidates for core-collapse supernovae (11–21 M⊙). Generally, we find that binary-stripped stars core tend to have a smaller compactness parameter, with a more prominent, deeper silicon/oxygen interface, and explode preferentially to the corresponding single stars of the same initial mass. Such a dichotomy of behavior between these two modes of evolution would have important implications for supernovae statistics, including the final neutron star masses, explosion energies, and nucleosynthetic yields. Binary-stripped remnants are also well poised to populate the possible mass gap between the heaviest neutron stars and the lightest black holes. Our work presents an improvement along two fronts, as we self-consistently account for the pre-collapse stellar evolution and the subsequent explosion outcome. Even so, our results emphasize the need for more detailed stellar evolutionary models to capture the sensitive nature of explosion outcome.","lang":"eng"}],"type":"journal_article"},{"month":"05","publication_identifier":{"issn":["0004-6256"],"eissn":["1538-3881"]},"quality_controlled":"1","main_file_link":[{"url":"https://arxiv.org/abs/2103.13642","open_access":"1"}],"oa":1,"external_id":{"arxiv":["2103.13642"]},"language":[{"iso":"eng"}],"doi":"10.3847/1538-3881/abf144","article_number":"248","extern":"1","publication_status":"published","publisher":"American Astronomical Society","year":"2021","date_updated":"2023-08-21T11:35:50Z","date_created":"2023-08-03T10:11:57Z","volume":161,"author":[{"first_name":"Luqian","last_name":"Wang","full_name":"Wang, Luqian"},{"full_name":"Gies, Douglas R.","first_name":"Douglas R.","last_name":"Gies"},{"full_name":"Peters, Geraldine J.","last_name":"Peters","first_name":"Geraldine J."},{"full_name":"Götberg, Ylva Louise Linsdotter","id":"d0648d0c-0f64-11ee-a2e0-dd0faa2e4f7d","orcid":"0000-0002-6960-6911","first_name":"Ylva Louise Linsdotter","last_name":"Götberg"},{"first_name":"S. Drew","last_name":"Chojnowski","full_name":"Chojnowski, S. Drew"},{"full_name":"Lester, Kathryn V.","last_name":"Lester","first_name":"Kathryn V."},{"last_name":"Howell","first_name":"Steve B.","full_name":"Howell, Steve B."}],"keyword":["Space and Planetary Science","Astronomy and Astrophysics"],"scopus_import":"1","day":"04","article_processing_charge":"No","article_type":"original","publication":"The Astronomical Journal","citation":{"ama":"Wang L, Gies DR, Peters GJ, et al. The detection and characterization of Be+sdO binaries from HST/STIS FUV spectroscopy. The Astronomical Journal. 2021;161(5). doi:10.3847/1538-3881/abf144","ieee":"L. Wang et al., “The detection and characterization of Be+sdO binaries from HST/STIS FUV spectroscopy,” The Astronomical Journal, vol. 161, no. 5. American Astronomical Society, 2021.","apa":"Wang, L., Gies, D. R., Peters, G. J., Götberg, Y. L. L., Chojnowski, S. D., Lester, K. V., & Howell, S. B. (2021). The detection and characterization of Be+sdO binaries from HST/STIS FUV spectroscopy. The Astronomical Journal. American Astronomical Society. https://doi.org/10.3847/1538-3881/abf144","ista":"Wang L, Gies DR, Peters GJ, Götberg YLL, Chojnowski SD, Lester KV, Howell SB. 2021. The detection and characterization of Be+sdO binaries from HST/STIS FUV spectroscopy. The Astronomical Journal. 161(5), 248.","short":"L. Wang, D.R. Gies, G.J. Peters, Y.L.L. Götberg, S.D. Chojnowski, K.V. Lester, S.B. Howell, The Astronomical Journal 161 (2021).","mla":"Wang, Luqian, et al. “The Detection and Characterization of Be+sdO Binaries from HST/STIS FUV Spectroscopy.” The Astronomical Journal, vol. 161, no. 5, 248, American Astronomical Society, 2021, doi:10.3847/1538-3881/abf144.","chicago":"Wang, Luqian, Douglas R. Gies, Geraldine J. Peters, Ylva Louise Linsdotter Götberg, S. Drew Chojnowski, Kathryn V. Lester, and Steve B. Howell. “The Detection and Characterization of Be+sdO Binaries from HST/STIS FUV Spectroscopy.” The Astronomical Journal. American Astronomical Society, 2021. https://doi.org/10.3847/1538-3881/abf144."},"date_published":"2021-05-04T00:00:00Z","type":"journal_article","abstract":[{"lang":"eng","text":"The B emission-line stars are rapid rotators that were probably spun up by mass and angular momentum accretion through mass transfer in an interacting binary. Mass transfer will strip the donor star of its envelope to create a small and hot subdwarf remnant. Here we report on Hubble Space Telescope/STIS far-ultraviolet spectroscopy of a sample of Be stars that reveals the presence of the hot sdO companion through the calculation of cross-correlation functions of the observed and model spectra. We clearly detect the spectral signature of the sdO star in 10 of the 13 stars in the sample, and the spectral signals indicate that the sdO stars are hot, relatively faint, and slowly rotating as predicted by models. A comparison of their temperatures and radii with evolutionary tracks indicates that the sdO stars occupy the relatively long-lived, He-core burning stage. Only 1 of the 10 detections was a known binary prior to this investigation, which emphasizes the difficulty of finding such Be+sdO binaries through optical spectroscopy. However, these results and others indicate that many Be stars probably host hot subdwarf companions."}],"issue":"5","status":"public","title":"The detection and characterization of Be+sdO binaries from HST/STIS FUV spectroscopy","intvolume":" 161","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","_id":"13459","oa_version":"Preprint"},{"status":"public","title":"The young massive SMC cluster NGC 330 seen by MUSE. II. Multiplicity properties of the massive-star population","intvolume":" 652","_id":"13457","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","oa_version":"Published Version","type":"journal_article","abstract":[{"text":"Context. Observations of massive stars in open clusters younger than ∼8 Myr have shown that a majority of them are in binary systems, most of which will interact during their life. While these can be used as a proxy of the initial multiplicity properties, studying populations of massive stars older than ∼20 Myr allows us to probe the outcome of these interactions after a significant number of systems have experienced mass and angular momentum transfer and may even have merged.\r\n\r\nAims. Using multi-epoch integral-field spectroscopy, we aim to investigate the multiplicity properties of the massive-star population in the dense core of the ∼40 Myr old cluster NGC 330 in the Small Magellanic Cloud in order to search for possible imprints of stellar evolution on the multiplicity properties.\r\n\r\nMethods. We obtained six epochs of VLT/MUSE observations operated in wide-field mode with the extended wavelength setup and supported by adaptive optics. We extracted spectra and measured radial velocities for stars brighter than mF814W = 19. We identified single-lined spectroscopic binaries through significant RV variability with a peak-to-peak amplitude larger than 20 km s−1. We also identified double-lined spectroscopic binaries, and quantified the observational biases for binary detection. In particular, we took into account that binary systems with similar line strengths are difficult to detect in our data set.\r\n\r\nResults. The observed spectroscopic binary fraction among stars brighter than mF814W = 19 (approximately 5.5 M⊙ on the main sequence) is fSBobs = 13.2 ± 2.0%. Considering period and mass ratio ranges from log(P) = 0.15−3.5 (about 1.4 to 3160 d), q = 0.1−1.0, and a representative set of orbital parameter distributions, we find a bias-corrected close binary fraction of fcl = 34−7+8%. This fraction seems to decline for the fainter stars, which indicates either that the close binary fraction drops in the B-type domain, or that the period distribution becomes more heavily weighted toward longer orbital periods. We further find that both fractions vary strongly in different regions of the color-magnitude diagram, which corresponds to different evolutionary stages. This probably reveals the imprint of the binary history of different groups of stars. In particular, we find that the observed spectroscopic binary fraction of Be stars (fSBobs = 2 ± 2%) is significantly lower than that of B-type stars (fSBobs = 9 ± 2%).\r\n\r\nConclusions. We provide the first homogeneous radial velocity study of a large sample of B-type stars at a low metallicity ([Fe/H] ≲ −1.0). The overall bias-corrected close binary fraction (log(P) < 3.5 d) of the B-star population in NGC 330 is lower than the fraction reported for younger Galactic and Large Magellanic Cloud clusters in previous works. More data are needed, however, to establish whether the observed differences are caused by an age or a metallicity effect.","lang":"eng"}],"article_type":"original","publication":"Astronomy & Astrophysics","citation":{"ama":"Bodensteiner J, Sana H, Wang C, et al. The young massive SMC cluster NGC 330 seen by MUSE. II. Multiplicity properties of the massive-star population. Astronomy & Astrophysics. 2021;652. doi:10.1051/0004-6361/202140507","ista":"Bodensteiner J, Sana H, Wang C, Langer N, Mahy L, Banyard G, de Koter A, de Mink SE, Evans CJ, Götberg YLL, Patrick LR, Schneider FRN, Tramper F. 2021. The young massive SMC cluster NGC 330 seen by MUSE. II. Multiplicity properties of the massive-star population. Astronomy & Astrophysics. 652, A70.","apa":"Bodensteiner, J., Sana, H., Wang, C., Langer, N., Mahy, L., Banyard, G., … Tramper, F. (2021). The young massive SMC cluster NGC 330 seen by MUSE. II. Multiplicity properties of the massive-star population. Astronomy & Astrophysics. EDP Sciences. https://doi.org/10.1051/0004-6361/202140507","ieee":"J. Bodensteiner et al., “The young massive SMC cluster NGC 330 seen by MUSE. II. Multiplicity properties of the massive-star population,” Astronomy & Astrophysics, vol. 652. EDP Sciences, 2021.","mla":"Bodensteiner, J., et al. “The Young Massive SMC Cluster NGC 330 Seen by MUSE. II. Multiplicity Properties of the Massive-Star Population.” Astronomy & Astrophysics, vol. 652, A70, EDP Sciences, 2021, doi:10.1051/0004-6361/202140507.","short":"J. Bodensteiner, H. Sana, C. Wang, N. Langer, L. Mahy, G. Banyard, A. de Koter, S.E. de Mink, C.J. Evans, Y.L.L. Götberg, L.R. Patrick, F.R.N. Schneider, F. Tramper, Astronomy & Astrophysics 652 (2021).","chicago":"Bodensteiner, J., H. Sana, C. Wang, N. Langer, L. Mahy, G. Banyard, A. de Koter, et al. “The Young Massive SMC Cluster NGC 330 Seen by MUSE. II. Multiplicity Properties of the Massive-Star Population.” Astronomy & Astrophysics. EDP Sciences, 2021. https://doi.org/10.1051/0004-6361/202140507."},"date_published":"2021-08-12T00:00:00Z","keyword":["Space and Planetary Science","Astronomy and Astrophysics"],"scopus_import":"1","day":"12","article_processing_charge":"No","publication_status":"published","publisher":"EDP Sciences","year":"2021","date_created":"2023-08-03T10:11:34Z","date_updated":"2023-08-21T11:49:36Z","volume":652,"author":[{"last_name":"Bodensteiner","first_name":"J.","full_name":"Bodensteiner, J."},{"full_name":"Sana, H.","last_name":"Sana","first_name":"H."},{"full_name":"Wang, C.","first_name":"C.","last_name":"Wang"},{"last_name":"Langer","first_name":"N.","full_name":"Langer, N."},{"full_name":"Mahy, L.","last_name":"Mahy","first_name":"L."},{"last_name":"Banyard","first_name":"G.","full_name":"Banyard, G."},{"full_name":"de Koter, A.","first_name":"A.","last_name":"de Koter"},{"last_name":"de Mink","first_name":"S. E.","full_name":"de Mink, S. E."},{"full_name":"Evans, C. J.","last_name":"Evans","first_name":"C. J."},{"orcid":"0000-0002-6960-6911","id":"d0648d0c-0f64-11ee-a2e0-dd0faa2e4f7d","last_name":"Götberg","first_name":"Ylva Louise Linsdotter","full_name":"Götberg, Ylva Louise Linsdotter"},{"full_name":"Patrick, L. R.","last_name":"Patrick","first_name":"L. R."},{"last_name":"Schneider","first_name":"F. R. N.","full_name":"Schneider, F. R. N."},{"last_name":"Tramper","first_name":"F.","full_name":"Tramper, F."}],"article_number":"A70","extern":"1","quality_controlled":"1","main_file_link":[{"open_access":"1","url":"https://doi.org/10.1051/0004-6361/202140507"}],"oa":1,"external_id":{"arxiv":["2104.13409"]},"language":[{"iso":"eng"}],"doi":"10.1051/0004-6361/202140507","month":"08","publication_identifier":{"eissn":["1432-0746"],"issn":["0004-6361"]}},{"publication_status":"published","publisher":"EDP Sciences","year":"2021","date_updated":"2023-08-21T11:49:15Z","date_created":"2023-08-03T10:11:09Z","volume":656,"author":[{"last_name":"Laplace","first_name":"E.","full_name":"Laplace, E."},{"first_name":"S.","last_name":"Justham","full_name":"Justham, S."},{"full_name":"Renzo, M.","first_name":"M.","last_name":"Renzo"},{"full_name":"Götberg, Ylva Louise Linsdotter","orcid":"0000-0002-6960-6911","id":"d0648d0c-0f64-11ee-a2e0-dd0faa2e4f7d","last_name":"Götberg","first_name":"Ylva Louise Linsdotter"},{"first_name":"R.","last_name":"Farmer","full_name":"Farmer, R."},{"last_name":"Vartanyan","first_name":"D.","full_name":"Vartanyan, D."},{"full_name":"de Mink, S. E.","last_name":"de Mink","first_name":"S. E."}],"article_number":"A58","quality_controlled":"1","external_id":{"arxiv":["2102.05036"]},"oa":1,"main_file_link":[{"url":"https://doi.org/10.1051/0004-6361/202140506","open_access":"1"}],"language":[{"iso":"eng"}],"doi":"10.1051/0004-6361/202140506","month":"12","publication_identifier":{"eissn":["1432-0746"],"issn":["0004-6361"]},"status":"public","title":"Different to the core: The pre-supernova structures of massive single and binary-stripped stars","intvolume":" 656","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","_id":"13455","oa_version":"Published Version","type":"journal_article","abstract":[{"text":"The majority of massive stars live in binary or multiple systems and will interact with a companion during their lifetimes, which helps to explain the observed diversity of core-collapse supernovae. Donor stars in binary systems can lose most of their hydrogen-rich envelopes through mass transfer. As a result, not only are the surface properties affected, but so is the core structure. However, most calculations of the core-collapse properties of massive stars rely on single-star models. We present a systematic study of the difference between the pre-supernova structures of single stars and stars of the same initial mass (11–21 M⊙) that have been stripped due to stable post-main-sequence mass transfer at solar metallicity. We present the pre-supernova core composition with novel diagrams that give an intuitive representation of the isotope distribution. As shown in previous studies, at the edge of the carbon-oxygen core, the binary-stripped star models contain an extended gradient of carbon, oxygen, and neon. This layer remains until core collapse and is more extended in mass for higher initial stellar masses. It originates from the receding of the convective helium core during core helium burning in binary-stripped stars, which does not occur in single-star models. We find that this same evolutionary phase leads to systematic differences in the final density and nuclear energy generation profiles. Binary-stripped star models have systematically higher total masses of carbon at the moment of core collapse compared to single-star models, which likely results in systematically different supernova yields. In about half of our models, the silicon-burning and oxygen-rich layers merge after core silicon burning. We discuss the implications of our findings for the “explodability”, supernova observations, and nucleosynthesis of these stars. Our models are publicly available and can be readily used as input for detailed supernova simulations.","lang":"eng"}],"article_type":"original","publication":"Astronomy & Astrophysics","citation":{"ama":"Laplace E, Justham S, Renzo M, et al. Different to the core: The pre-supernova structures of massive single and binary-stripped stars. Astronomy & Astrophysics. 2021;656. doi:10.1051/0004-6361/202140506","ista":"Laplace E, Justham S, Renzo M, Götberg YLL, Farmer R, Vartanyan D, de Mink SE. 2021. Different to the core: The pre-supernova structures of massive single and binary-stripped stars. Astronomy & Astrophysics. 656, A58.","apa":"Laplace, E., Justham, S., Renzo, M., Götberg, Y. L. L., Farmer, R., Vartanyan, D., & de Mink, S. E. (2021). Different to the core: The pre-supernova structures of massive single and binary-stripped stars. Astronomy & Astrophysics. EDP Sciences. https://doi.org/10.1051/0004-6361/202140506","ieee":"E. Laplace et al., “Different to the core: The pre-supernova structures of massive single and binary-stripped stars,” Astronomy & Astrophysics, vol. 656. EDP Sciences, 2021.","mla":"Laplace, E., et al. “Different to the Core: The Pre-Supernova Structures of Massive Single and Binary-Stripped Stars.” Astronomy & Astrophysics, vol. 656, A58, EDP Sciences, 2021, doi:10.1051/0004-6361/202140506.","short":"E. Laplace, S. Justham, M. Renzo, Y.L.L. Götberg, R. Farmer, D. Vartanyan, S.E. de Mink, Astronomy & Astrophysics 656 (2021).","chicago":"Laplace, E., S. Justham, M. Renzo, Ylva Louise Linsdotter Götberg, R. Farmer, D. Vartanyan, and S. E. de Mink. “Different to the Core: The Pre-Supernova Structures of Massive Single and Binary-Stripped Stars.” Astronomy & Astrophysics. EDP Sciences, 2021. https://doi.org/10.1051/0004-6361/202140506."},"date_published":"2021-12-02T00:00:00Z","keyword":["Space and Planetary Science","Astronomy and Astrophysics"],"scopus_import":"1","day":"02","article_processing_charge":"No"},{"abstract":[{"text":"Helium star–carbon-oxygen white dwarf (CO WD) binaries are potential single-degenerate progenitor systems of thermonuclear supernovae. Revisiting a set of binary evolution calculations using the stellar evolution code MESA, we refine our previous predictions about which systems can lead to a thermonuclear supernova and then characterize the properties of the helium star donor at the time of explosion. We convert these model properties to near-UV/optical magnitudes assuming a blackbody spectrum and support this approach using a matched stellar atmosphere model. These models will be valuable to compare with pre-explosion imaging for future supernovae, though we emphasize the observational difficulty of detecting extremely blue companions. The pre-explosion source detected in association with SN 2012Z has been interpreted as a helium star binary containing an initially ultra-massive WD in a multiday orbit. However, extending our binary models to initial CO WD masses of up to 1.2 M⊙, we find that these systems undergo off-center carbon ignitions and thus are not expected to produce thermonuclear supernovae. This tension suggests that, if SN 2012Z is associated with a helium star–WD binary, then the pre-explosion optical light from the system must be significantly modified by the binary environment and/or the WD does not have a carbon-rich interior composition.","lang":"eng"}],"issue":"2","type":"journal_article","oa_version":"Preprint","title":"Pre-explosion properties of Helium star donors to thermonuclear supernovae","status":"public","intvolume":" 922","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","_id":"13454","day":"03","article_processing_charge":"No","keyword":["Space and Planetary Science","Astronomy and Astrophysics"],"scopus_import":"1","date_published":"2021-12-03T00:00:00Z","article_type":"original","publication":"The Astrophysical Journal","citation":{"mla":"Wong, Tin Long Sunny, et al. “Pre-Explosion Properties of Helium Star Donors to Thermonuclear Supernovae.” The Astrophysical Journal, vol. 922, no. 2, 241, American Astronomical Society, 2021, doi:10.3847/1538-4357/ac27ae.","short":"T.L.S. Wong, J. Schwab, Y.L.L. Götberg, The Astrophysical Journal 922 (2021).","chicago":"Wong, Tin Long Sunny, Josiah Schwab, and Ylva Louise Linsdotter Götberg. “Pre-Explosion Properties of Helium Star Donors to Thermonuclear Supernovae.” The Astrophysical Journal. American Astronomical Society, 2021. https://doi.org/10.3847/1538-4357/ac27ae.","ama":"Wong TLS, Schwab J, Götberg YLL. Pre-explosion properties of Helium star donors to thermonuclear supernovae. The Astrophysical Journal. 2021;922(2). doi:10.3847/1538-4357/ac27ae","ista":"Wong TLS, Schwab J, Götberg YLL. 2021. Pre-explosion properties of Helium star donors to thermonuclear supernovae. The Astrophysical Journal. 922(2), 241.","apa":"Wong, T. L. S., Schwab, J., & Götberg, Y. L. L. (2021). Pre-explosion properties of Helium star donors to thermonuclear supernovae. The Astrophysical Journal. American Astronomical Society. https://doi.org/10.3847/1538-4357/ac27ae","ieee":"T. L. S. Wong, J. Schwab, and Y. L. L. Götberg, “Pre-explosion properties of Helium star donors to thermonuclear supernovae,” The Astrophysical Journal, vol. 922, no. 2. American Astronomical Society, 2021."},"extern":"1","article_number":"241","date_updated":"2023-08-21T11:52:05Z","date_created":"2023-08-03T10:10:58Z","volume":922,"author":[{"last_name":"Wong","first_name":"Tin Long Sunny","full_name":"Wong, Tin Long Sunny"},{"last_name":"Schwab","first_name":"Josiah","full_name":"Schwab, Josiah"},{"full_name":"Götberg, Ylva Louise Linsdotter","first_name":"Ylva Louise Linsdotter","last_name":"Götberg","id":"d0648d0c-0f64-11ee-a2e0-dd0faa2e4f7d","orcid":"0000-0002-6960-6911"}],"publication_status":"published","publisher":"American Astronomical Society","year":"2021","month":"12","publication_identifier":{"eissn":["1538-4357"],"issn":["0004-637X"]},"language":[{"iso":"eng"}],"doi":"10.3847/1538-4357/ac27ae","quality_controlled":"1","external_id":{"arxiv":["2109.14817"]},"main_file_link":[{"url":"https://arxiv.org/abs/2109.14817","open_access":"1"}],"oa":1},{"date_published":"2021-12-29T00:00:00Z","publication":"The Astrophysical Journal","citation":{"ama":"Renzo M, Götberg YLL. Evolution of accretor stars in massive binaries: Broader implications from modeling ζ Ophiuchi. The Astrophysical Journal. 2021;923(2). doi:10.3847/1538-4357/ac29c5","ista":"Renzo M, Götberg YLL. 2021. Evolution of accretor stars in massive binaries: Broader implications from modeling ζ Ophiuchi. The Astrophysical Journal. 923(2), 277.","apa":"Renzo, M., & Götberg, Y. L. L. (2021). Evolution of accretor stars in massive binaries: Broader implications from modeling ζ Ophiuchi. The Astrophysical Journal. American Astronomical Society. https://doi.org/10.3847/1538-4357/ac29c5","ieee":"M. Renzo and Y. L. L. Götberg, “Evolution of accretor stars in massive binaries: Broader implications from modeling ζ Ophiuchi,” The Astrophysical Journal, vol. 923, no. 2. American Astronomical Society, 2021.","mla":"Renzo, M., and Ylva Louise Linsdotter Götberg. “Evolution of Accretor Stars in Massive Binaries: Broader Implications from Modeling ζ Ophiuchi.” The Astrophysical Journal, vol. 923, no. 2, 277, American Astronomical Society, 2021, doi:10.3847/1538-4357/ac29c5.","short":"M. Renzo, Y.L.L. Götberg, The Astrophysical Journal 923 (2021).","chicago":"Renzo, M., and Ylva Louise Linsdotter Götberg. “Evolution of Accretor Stars in Massive Binaries: Broader Implications from Modeling ζ Ophiuchi.” The Astrophysical Journal. American Astronomical Society, 2021. https://doi.org/10.3847/1538-4357/ac29c5."},"article_type":"original","day":"29","article_processing_charge":"No","scopus_import":"1","keyword":["Space and Planetary Science","Astronomy and Astrophysics"],"oa_version":"Preprint","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","_id":"13453","status":"public","title":"Evolution of accretor stars in massive binaries: Broader implications from modeling ζ Ophiuchi","intvolume":" 923","abstract":[{"lang":"eng","text":"Most massive stars are born in binaries close enough for mass transfer episodes. These modify the appearance, structure, and future evolution of both stars. We compute the evolution of a 100-day-period binary, consisting initially of a 25 M⊙ star and a 17 M⊙ star, which experiences stable mass transfer. We focus on the impact of mass accretion on the surface composition, internal rotation, and structure of the accretor. To anchor our models, we show that our accretor broadly reproduces the properties of ζ Ophiuchi, which has long been proposed to have accreted mass before being ejected as a runaway star when the companion exploded. We compare our accretor to models of single rotating stars and find that the later and stronger spin-up provided by mass accretion produces significant differences. Specifically, the core of the accretor retains higher spin at the end of the main sequence, and a convective layer develops that changes its density profile. Moreover, the surface of the accretor star is polluted by CNO-processed material donated by the companion. Our models show effects of mass accretion in binaries that are not captured in single rotating stellar models. This possibly impacts the further evolution (either in a binary or as single stars), the final collapse, and the resulting spin of the compact object."}],"issue":"2","type":"journal_article","doi":"10.3847/1538-4357/ac29c5","language":[{"iso":"eng"}],"main_file_link":[{"url":"https://arxiv.org/abs/2107.10933","open_access":"1"}],"external_id":{"arxiv":["2107.10933"]},"oa":1,"quality_controlled":"1","month":"12","publication_identifier":{"issn":["0004-637X"],"eissn":["1538-4357"]},"author":[{"first_name":"M.","last_name":"Renzo","full_name":"Renzo, M."},{"full_name":"Götberg, Ylva Louise Linsdotter","orcid":"0000-0002-6960-6911","id":"d0648d0c-0f64-11ee-a2e0-dd0faa2e4f7d","last_name":"Götberg","first_name":"Ylva Louise Linsdotter"}],"date_updated":"2023-08-21T11:59:34Z","date_created":"2023-08-03T10:10:48Z","volume":923,"year":"2021","publication_status":"published","publisher":"American Astronomical Society","extern":"1","article_number":"277"},{"abstract":[{"lang":"eng","text":"We report the observation of an anomalous nonlinear optical response of the prototypical three-dimensional topological insulator bismuth selenide through the process of high-order harmonic generation. We find that the generation efficiency increases as the laser polarization is changed from linear to elliptical, and it becomes maximum for circular polarization. With the aid of a microscopic theory and a detailed analysis of the measured spectra, we reveal that such anomalous enhancement encodes the characteristic topology of the band structure that originates from the interplay of strong spin–orbit coupling and time-reversal symmetry protection. The implications are in ultrafast probing of topological phase transitions, light-field driven dissipationless electronics, and quantum computation."}],"issue":"21","type":"journal_article","oa_version":"Published Version","status":"public","title":"All-optical probe of three-dimensional topological insulators based on high-harmonic generation by circularly polarized laser fields","intvolume":" 21","_id":"13996","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","day":"22","article_processing_charge":"No","keyword":["Mechanical Engineering","Condensed Matter Physics","General Materials Science","General Chemistry","Bioengineering"],"scopus_import":"1","date_published":"2021-10-22T00:00:00Z","article_type":"original","page":"8970-8978","publication":"Nano Letters","citation":{"chicago":"Baykusheva, Denitsa Rangelova, Alexis Chacón, Jian Lu, Trevor P. Bailey, Jonathan A. Sobota, Hadas Soifer, Patrick S. Kirchmann, et al. “All-Optical Probe of Three-Dimensional Topological Insulators Based on High-Harmonic Generation by Circularly Polarized Laser Fields.” Nano Letters. American Chemical Society, 2021. https://doi.org/10.1021/acs.nanolett.1c02145.","short":"D.R. Baykusheva, A. Chacón, J. Lu, T.P. Bailey, J.A. Sobota, H. Soifer, P.S. Kirchmann, C. Rotundu, C. Uher, T.F. Heinz, D.A. Reis, S. Ghimire, Nano Letters 21 (2021) 8970–8978.","mla":"Baykusheva, Denitsa Rangelova, et al. “All-Optical Probe of Three-Dimensional Topological Insulators Based on High-Harmonic Generation by Circularly Polarized Laser Fields.” Nano Letters, vol. 21, no. 21, American Chemical Society, 2021, pp. 8970–78, doi:10.1021/acs.nanolett.1c02145.","ieee":"D. R. Baykusheva et al., “All-optical probe of three-dimensional topological insulators based on high-harmonic generation by circularly polarized laser fields,” Nano Letters, vol. 21, no. 21. American Chemical Society, pp. 8970–8978, 2021.","apa":"Baykusheva, D. R., Chacón, A., Lu, J., Bailey, T. P., Sobota, J. A., Soifer, H., … Ghimire, S. (2021). All-optical probe of three-dimensional topological insulators based on high-harmonic generation by circularly polarized laser fields. Nano Letters. American Chemical Society. https://doi.org/10.1021/acs.nanolett.1c02145","ista":"Baykusheva DR, Chacón A, Lu J, Bailey TP, Sobota JA, Soifer H, Kirchmann PS, Rotundu C, Uher C, Heinz TF, Reis DA, Ghimire S. 2021. All-optical probe of three-dimensional topological insulators based on high-harmonic generation by circularly polarized laser fields. Nano Letters. 21(21), 8970–8978.","ama":"Baykusheva DR, Chacón A, Lu J, et al. All-optical probe of three-dimensional topological insulators based on high-harmonic generation by circularly polarized laser fields. Nano Letters. 2021;21(21):8970-8978. doi:10.1021/acs.nanolett.1c02145"},"extern":"1","date_created":"2023-08-09T13:09:15Z","date_updated":"2023-08-22T07:32:00Z","volume":21,"author":[{"id":"71b4d059-2a03-11ee-914d-dfa3beed6530","first_name":"Denitsa Rangelova","last_name":"Baykusheva","full_name":"Baykusheva, Denitsa Rangelova"},{"full_name":"Chacón, Alexis","last_name":"Chacón","first_name":"Alexis"},{"full_name":"Lu, Jian","first_name":"Jian","last_name":"Lu"},{"full_name":"Bailey, Trevor P.","first_name":"Trevor P.","last_name":"Bailey"},{"full_name":"Sobota, Jonathan A.","first_name":"Jonathan A.","last_name":"Sobota"},{"last_name":"Soifer","first_name":"Hadas","full_name":"Soifer, Hadas"},{"last_name":"Kirchmann","first_name":"Patrick S.","full_name":"Kirchmann, Patrick S."},{"last_name":"Rotundu","first_name":"Costel","full_name":"Rotundu, Costel"},{"last_name":"Uher","first_name":"Ctirad","full_name":"Uher, Ctirad"},{"last_name":"Heinz","first_name":"Tony F.","full_name":"Heinz, Tony F."},{"last_name":"Reis","first_name":"David A.","full_name":"Reis, David A."},{"full_name":"Ghimire, Shambhu","last_name":"Ghimire","first_name":"Shambhu"}],"publication_status":"published","publisher":"American Chemical Society","year":"2021","pmid":1,"month":"10","publication_identifier":{"issn":["1530-6984"],"eissn":["1530-6992"]},"language":[{"iso":"eng"}],"doi":"10.1021/acs.nanolett.1c02145","quality_controlled":"1","main_file_link":[{"url":"https://doi.org/10.1021/acs.nanolett.1c02145","open_access":"1"}],"oa":1,"external_id":{"pmid":["34676752"],"arxiv":["2109.15291"]}},{"citation":{"short":"D.R. Baykusheva, A. Chacón, D. Kim, D.E. Kim, D.A. Reis, S. Ghimire, Physical Review A 103 (2021).","mla":"Baykusheva, Denitsa Rangelova, et al. “Strong-Field Physics in Three-Dimensional Topological Insulators.” Physical Review A, vol. 103, no. 2, 023101, American Physical Society, 2021, doi:10.1103/physreva.103.023101.","chicago":"Baykusheva, Denitsa Rangelova, Alexis Chacón, Dasol Kim, Dong Eon Kim, David A. Reis, and Shambhu Ghimire. “Strong-Field Physics in Three-Dimensional Topological Insulators.” Physical Review A. American Physical Society, 2021. https://doi.org/10.1103/physreva.103.023101.","ama":"Baykusheva DR, Chacón A, Kim D, Kim DE, Reis DA, Ghimire S. Strong-field physics in three-dimensional topological insulators. Physical Review A. 2021;103(2). doi:10.1103/physreva.103.023101","ieee":"D. R. Baykusheva, A. Chacón, D. Kim, D. E. Kim, D. A. Reis, and S. Ghimire, “Strong-field physics in three-dimensional topological insulators,” Physical Review A, vol. 103, no. 2. American Physical Society, 2021.","apa":"Baykusheva, D. R., Chacón, A., Kim, D., Kim, D. E., Reis, D. A., & Ghimire, S. (2021). Strong-field physics in three-dimensional topological insulators. Physical Review A. American Physical Society. https://doi.org/10.1103/physreva.103.023101","ista":"Baykusheva DR, Chacón A, Kim D, Kim DE, Reis DA, Ghimire S. 2021. Strong-field physics in three-dimensional topological insulators. Physical Review A. 103(2), 023101."},"publication":"Physical Review A","article_type":"original","date_published":"2021-02-01T00:00:00Z","scopus_import":"1","article_processing_charge":"No","day":"01","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","_id":"13997","intvolume":" 103","status":"public","title":"Strong-field physics in three-dimensional topological insulators","oa_version":"Preprint","type":"journal_article","issue":"2","abstract":[{"lang":"eng","text":"We investigate theoretically the strong-field regime of light-matter interactions in the topological-insulator class of quantum materials. In particular, we focus on the process of nonperturbative high-order harmonic generation from the paradigmatic three-dimensional topological insulator bismuth selenide (Bi2Se3) subjected to intense midinfrared laser fields. We analyze the contributions from the spin-orbit-coupled bulk states and the topological surface bands separately and reveal a major difference in how their harmonic yields depend on the ellipticity of the laser field. Bulk harmonics show a monotonic decrease in their yield as the ellipticity increases, in a manner reminiscent of high harmonic generation in gaseous media. However, the surface contribution exhibits a highly nontrivial dependence, culminating with a maximum for circularly polarized fields. We attribute the observed anomalous behavior to (i) the enhanced amplitude and the circular pattern of the interband dipole and the Berry connections in the vicinity of the Dirac point and (ii) the influence of the higher-order, hexagonal warping terms in the Hamiltonian, which are responsible for the hexagonal deformation of the energy surface at higher momenta. The latter are associated directly with spin-orbit-coupling parameters. Our results thus establish the sensitivity of strong-field-driven high harmonic emission to the topology of the band structure as well as to the manifestations of spin-orbit interaction."}],"main_file_link":[{"open_access":"1","url":"https://arxiv.org/abs/2008.01265"}],"oa":1,"external_id":{"arxiv":["2008.01265"]},"quality_controlled":"1","doi":"10.1103/physreva.103.023101","language":[{"iso":"eng"}],"publication_identifier":{"issn":["2469-9926"],"eissn":["2469-9934"]},"month":"02","year":"2021","publisher":"American Physical Society","publication_status":"published","author":[{"id":"71b4d059-2a03-11ee-914d-dfa3beed6530","first_name":"Denitsa Rangelova","last_name":"Baykusheva","full_name":"Baykusheva, Denitsa Rangelova"},{"full_name":"Chacón, Alexis","last_name":"Chacón","first_name":"Alexis"},{"last_name":"Kim","first_name":"Dasol","full_name":"Kim, Dasol"},{"first_name":"Dong Eon","last_name":"Kim","full_name":"Kim, Dong Eon"},{"full_name":"Reis, David A.","last_name":"Reis","first_name":"David A."},{"first_name":"Shambhu","last_name":"Ghimire","full_name":"Ghimire, Shambhu"}],"volume":103,"date_created":"2023-08-09T13:09:26Z","date_updated":"2023-08-22T07:33:43Z","article_number":"023101","extern":"1"},{"author":[{"first_name":"Saijoscha","last_name":"Heck","full_name":"Heck, Saijoscha"},{"full_name":"Baykusheva, Denitsa Rangelova","last_name":"Baykusheva","first_name":"Denitsa Rangelova","id":"71b4d059-2a03-11ee-914d-dfa3beed6530"},{"first_name":"Meng","last_name":"Han","full_name":"Han, Meng"},{"full_name":"Ji, Jia-Bao","last_name":"Ji","first_name":"Jia-Bao"},{"full_name":"Perry, Conaill","last_name":"Perry","first_name":"Conaill"},{"full_name":"Gong, Xiaochun","last_name":"Gong","first_name":"Xiaochun"},{"last_name":"Wörner","first_name":"Hans Jakob","full_name":"Wörner, Hans Jakob"}],"volume":7,"date_updated":"2023-08-22T07:30:25Z","date_created":"2023-08-09T13:09:02Z","pmid":1,"year":"2021","publisher":"American Association for the Advancement of Science","publication_status":"published","extern":"1","article_number":"abj8121","doi":"10.1126/sciadv.abj8121","language":[{"iso":"eng"}],"external_id":{"pmid":["34860540"]},"main_file_link":[{"url":"https://doi.org/10.1126/sciadv.abj8121","open_access":"1"}],"oa":1,"quality_controlled":"1","publication_identifier":{"eissn":["2375-2548"]},"month":"12","oa_version":"Published Version","_id":"13995","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","intvolume":" 7","title":"Attosecond interferometry of shape resonances in the recoil frame of CF4","status":"public","issue":"49","abstract":[{"text":"Shape resonances play a central role in many areas of science, but the real-time measurement of the associated many-body dynamics remains challenging. Here, we present measurements of recoil frame angle-resolved photoionization delays in the vicinity of shape resonances of CF4. This technique provides insights into the spatiotemporal photoionization dynamics of molecular shape resonances. We find delays of up to ∼600 as in the ionization out of the highest occupied molecular orbital (HOMO) with a strong dependence on the emission direction and a pronounced asymmetry along the dissociation axis. Comparison with quantum-scattering calculations traces the asymmetries to the interference of a small subset of partial waves at low kinetic energies and, additionally, to the interference of two overlapping shape resonances in the HOMO-1 channel. Our experimental and theoretical results establish a broadly applicable approach to space- and time-resolved photoionization dynamics in the molecular frame.","lang":"eng"}],"type":"journal_article","date_published":"2021-12-03T00:00:00Z","citation":{"ista":"Heck S, Baykusheva DR, Han M, Ji J-B, Perry C, Gong X, Wörner HJ. 2021. Attosecond interferometry of shape resonances in the recoil frame of CF4. Science Advances. 7(49), abj8121.","apa":"Heck, S., Baykusheva, D. R., Han, M., Ji, J.-B., Perry, C., Gong, X., & Wörner, H. J. (2021). Attosecond interferometry of shape resonances in the recoil frame of CF4. Science Advances. American Association for the Advancement of Science. https://doi.org/10.1126/sciadv.abj8121","ieee":"S. Heck et al., “Attosecond interferometry of shape resonances in the recoil frame of CF4,” Science Advances, vol. 7, no. 49. American Association for the Advancement of Science, 2021.","ama":"Heck S, Baykusheva DR, Han M, et al. Attosecond interferometry of shape resonances in the recoil frame of CF4. Science Advances. 2021;7(49). doi:10.1126/sciadv.abj8121","chicago":"Heck, Saijoscha, Denitsa Rangelova Baykusheva, Meng Han, Jia-Bao Ji, Conaill Perry, Xiaochun Gong, and Hans Jakob Wörner. “Attosecond Interferometry of Shape Resonances in the Recoil Frame of CF4.” Science Advances. American Association for the Advancement of Science, 2021. https://doi.org/10.1126/sciadv.abj8121.","mla":"Heck, Saijoscha, et al. “Attosecond Interferometry of Shape Resonances in the Recoil Frame of CF4.” Science Advances, vol. 7, no. 49, abj8121, American Association for the Advancement of Science, 2021, doi:10.1126/sciadv.abj8121.","short":"S. Heck, D.R. Baykusheva, M. Han, J.-B. Ji, C. Perry, X. Gong, H.J. Wörner, Science Advances 7 (2021)."},"publication":"Science Advances","article_type":"original","article_processing_charge":"No","day":"03","scopus_import":"1","keyword":["Multidisciplinary"]},{"article_processing_charge":"No","day":"30","month":"11","main_file_link":[{"url":" https://doi.org/10.48550/arXiv.2111.15608","open_access":"1"}],"citation":{"ama":"Kulkarni SR, Harrison FA, Grefenstette BW, et al. Science with the ultraviolet explorer (UVEX). arXiv. doi:10.48550/arXiv.2111.15608","ista":"Kulkarni SR, Harrison FA, Grefenstette BW, Earnshaw HP, Andreoni I, Berg DA, Bloom JS, Cenko SB, Chornock R, Christiansen JL, Coughlin MW, Criswell AW, Darvish B, Das KK, De K, Dessart L, Dixon D, Dorsman B, Kareem El-Badry KE-B, Evans C, Ford KES, Fremling C, Gansicke BT, Gezari S, Götberg YLL, Green GM, Graham MJ, Heida M, Ho AYQ, Jaodand AD, Christopher M. Johns-Krull CMJ-K, Kasliwal MM, Lazzarini M, Lu W, Margutti R, Martin DC, Masters DC, McKernan B, Naze Y, Nissanke SM, Parazin B, Perley DA, Phinney ES, Piro AL, Raaijmakers G, Rauw G, Rodriguez AC, Sana H, Senchyna P, Singer LP, Spake JJ, Stassun KG, Stern D, Teplitz HI, Weisz DR, Yao Y. Science with the ultraviolet explorer (UVEX). arXiv, 2111.15608.","apa":"Kulkarni, S. R., Harrison, F. A., Grefenstette, B. W., Earnshaw, H. P., Andreoni, I., Berg, D. A., … Yao, Y. (n.d.). Science with the ultraviolet explorer (UVEX). arXiv. https://doi.org/10.48550/arXiv.2111.15608","ieee":"S. R. Kulkarni et al., “Science with the ultraviolet explorer (UVEX),” arXiv. .","mla":"Kulkarni, S. R., et al. “Science with the Ultraviolet Explorer (UVEX).” ArXiv, 2111.15608, doi:10.48550/arXiv.2111.15608.","short":"S.R. Kulkarni, F.A. Harrison, B.W. Grefenstette, H.P. Earnshaw, I. Andreoni, D.A. Berg, J.S. Bloom, S.B. Cenko, R. Chornock, J.L. Christiansen, M.W. Coughlin, A.W. Criswell, B. Darvish, K.K. Das, K. De, L. Dessart, D. Dixon, B. Dorsman, K.E.-B. Kareem El-Badry, C. Evans, K.E.S. Ford, C. Fremling, B.T. Gansicke, S. Gezari, Y.L.L. Götberg, G.M. Green, M.J. Graham, M. Heida, A.Y.Q. Ho, A.D. Jaodand, C.M.J.-K. Christopher M. Johns-Krull, M.M. Kasliwal, M. Lazzarini, W. Lu, R. Margutti, D.C. Martin, D.C. Masters, B. McKernan, Y. Naze, S.M. Nissanke, B. Parazin, D.A. Perley, E.S. Phinney, A.L. Piro, G. Raaijmakers, G. Rauw, A.C. Rodriguez, H. Sana, P. Senchyna, L.P. Singer, J.J. Spake, K.G. Stassun, D. Stern, H.I. Teplitz, D.R. Weisz, Y. Yao, ArXiv (n.d.).","chicago":"Kulkarni, S. R., Fiona A. Harrison, Brian W. Grefenstette, Hannah P. Earnshaw, Igor Andreoni, Danielle A. Berg, Joshua S. Bloom, et al. “Science with the Ultraviolet Explorer (UVEX).” ArXiv, n.d. https://doi.org/10.48550/arXiv.2111.15608."},"oa":1,"external_id":{"arxiv":["2111.15608"]},"publication":"arXiv","date_published":"2021-11-30T00:00:00Z","doi":"10.48550/arXiv.2111.15608","language":[{"iso":"eng"}],"type":"preprint","article_number":"2111.15608","abstract":[{"text":"UVEX is a proposed medium class Explorer mission designed to provide crucial missing capabilities that will address objectives central to a broad range of modern astrophysics. The UVEX design has two co-aligned wide-field imagers operating in the FUV and NUV and a powerful broadband medium resolution spectrometer. In its two-year baseline mission, UVEX will perform a multi-cadence synoptic all-sky survey 50/100 times deeper than GALEX in the NUV/FUV, cadenced surveys of the Large and Small Magellanic Clouds, rapid target of opportunity followup, as well as spectroscopic followup of samples of stars and galaxies. The science program is built around three pillars. First, UVEX will explore the low-mass, low-metallicity galaxy frontier through imaging and spectroscopic surveys that will probe key aspects of the evolution of galaxies by understanding how star formation and stellar evolution at low metallicities affect the growth and evolution of low-metallicity, low-mass galaxies in the local universe. Such galaxies contain half the mass in the local universe, and are analogs for the first galaxies, but observed at distances that make them accessible to detailed study. Second, UVEX will explore the dynamic universe through time-domain surveys and prompt spectroscopic followup capability will probe the environments, energetics, and emission processes in the early aftermaths of gravitational wave-discovered compact object mergers, discover hot, fast UV transients, and diagnose the early stages of stellar explosions. Finally, UVEX will become a key community resource by leaving a large all-sky legacy data set, enabling a wide range of scientific studies and filling a gap in the new generation of wide-field, sensitive optical and infrared surveys provided by the Rubin, Euclid, and Roman observatories. This paper discusses the scientific potential of UVEX, and the broad scientific program.","lang":"eng"}],"extern":"1","_id":"14097","year":"2021","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","status":"public","title":"Science with the ultraviolet explorer (UVEX)","publication_status":"submitted","author":[{"full_name":"Kulkarni, S. R.","first_name":"S. R.","last_name":"Kulkarni"},{"full_name":"Harrison, Fiona A.","first_name":"Fiona A.","last_name":"Harrison"},{"first_name":"Brian W.","last_name":"Grefenstette","full_name":"Grefenstette, Brian W."},{"last_name":"Earnshaw","first_name":"Hannah P.","full_name":"Earnshaw, Hannah P."},{"full_name":"Andreoni, Igor","first_name":"Igor","last_name":"Andreoni"},{"full_name":"Berg, Danielle A.","first_name":"Danielle A.","last_name":"Berg"},{"last_name":"Bloom","first_name":"Joshua S.","full_name":"Bloom, Joshua S."},{"last_name":"Cenko","first_name":"S. Bradley","full_name":"Cenko, S. Bradley"},{"full_name":"Chornock, Ryan","last_name":"Chornock","first_name":"Ryan"},{"last_name":"Christiansen","first_name":"Jessie L.","full_name":"Christiansen, Jessie L."},{"full_name":"Coughlin, Michael W.","first_name":"Michael W.","last_name":"Coughlin"},{"last_name":"Criswell","first_name":"Alexander Wuollet","full_name":"Criswell, Alexander Wuollet"},{"full_name":"Darvish, Behnam","last_name":"Darvish","first_name":"Behnam"},{"first_name":"Kaustav K.","last_name":"Das","full_name":"Das, Kaustav K."},{"full_name":"De, Kishalay","last_name":"De","first_name":"Kishalay"},{"full_name":"Dessart, Luc","first_name":"Luc","last_name":"Dessart"},{"full_name":"Dixon, Don","last_name":"Dixon","first_name":"Don"},{"full_name":"Dorsman, Bas","first_name":"Bas","last_name":"Dorsman"},{"first_name":"Kareem El-Badry","last_name":"Kareem El-Badry","full_name":"Kareem El-Badry, Kareem El-Badry"},{"last_name":"Evans","first_name":"Christopher","full_name":"Evans, Christopher"},{"full_name":"Ford, K. E. Saavik","last_name":"Ford","first_name":"K. E. Saavik"},{"first_name":"Christoffer","last_name":"Fremling","full_name":"Fremling, Christoffer"},{"full_name":"Gansicke, Boris T.","first_name":"Boris T.","last_name":"Gansicke"},{"full_name":"Gezari, Suvi","first_name":"Suvi","last_name":"Gezari"},{"full_name":"Götberg, Ylva Louise Linsdotter","orcid":"0000-0002-6960-6911","id":"d0648d0c-0f64-11ee-a2e0-dd0faa2e4f7d","last_name":"Götberg","first_name":"Ylva Louise Linsdotter"},{"full_name":"Green, Gregory M.","last_name":"Green","first_name":"Gregory M."},{"first_name":"Matthew J.","last_name":"Graham","full_name":"Graham, Matthew J."},{"first_name":"Marianne","last_name":"Heida","full_name":"Heida, Marianne"},{"full_name":"Ho, Anna Y. Q.","first_name":"Anna Y. Q.","last_name":"Ho"},{"full_name":"Jaodand, Amruta D.","first_name":"Amruta D.","last_name":"Jaodand"},{"full_name":"Christopher M. Johns-Krull, Christopher M. Johns-Krull","first_name":"Christopher M. Johns-Krull","last_name":"Christopher M. Johns-Krull"},{"first_name":"Mansi M.","last_name":"Kasliwal","full_name":"Kasliwal, Mansi M."},{"full_name":"Lazzarini, Margaret","first_name":"Margaret","last_name":"Lazzarini"},{"full_name":"Lu, Wenbin","first_name":"Wenbin","last_name":"Lu"},{"first_name":"Raffaella","last_name":"Margutti","full_name":"Margutti, Raffaella"},{"last_name":"Martin","first_name":"D. Christopher","full_name":"Martin, D. Christopher"},{"first_name":"Daniel Charles","last_name":"Masters","full_name":"Masters, Daniel Charles"},{"full_name":"McKernan, Barry","first_name":"Barry","last_name":"McKernan"},{"last_name":"Naze","first_name":"Yael","full_name":"Naze, Yael"},{"first_name":"Samaya M.","last_name":"Nissanke","full_name":"Nissanke, Samaya M."},{"full_name":"Parazin, B.","first_name":"B.","last_name":"Parazin"},{"full_name":"Perley, Daniel A.","first_name":"Daniel A.","last_name":"Perley"},{"last_name":"Phinney","first_name":"E. Sterl","full_name":"Phinney, E. Sterl"},{"full_name":"Piro, Anthony L.","first_name":"Anthony L.","last_name":"Piro"},{"full_name":"Raaijmakers, G.","first_name":"G.","last_name":"Raaijmakers"},{"full_name":"Rauw, Gregor","first_name":"Gregor","last_name":"Rauw"},{"full_name":"Rodriguez, Antonio C.","last_name":"Rodriguez","first_name":"Antonio C."},{"full_name":"Sana, Hugues","first_name":"Hugues","last_name":"Sana"},{"first_name":"Peter","last_name":"Senchyna","full_name":"Senchyna, Peter"},{"last_name":"Singer","first_name":"Leo P.","full_name":"Singer, Leo P."},{"full_name":"Spake, Jessica J.","first_name":"Jessica J.","last_name":"Spake"},{"full_name":"Stassun, Keivan G.","first_name":"Keivan G.","last_name":"Stassun"},{"first_name":"Daniel","last_name":"Stern","full_name":"Stern, Daniel"},{"first_name":"Harry I.","last_name":"Teplitz","full_name":"Teplitz, Harry I."},{"last_name":"Weisz","first_name":"Daniel R.","full_name":"Weisz, Daniel R."},{"full_name":"Yao, Yuhan","first_name":"Yuhan","last_name":"Yao"}],"oa_version":"Preprint","date_created":"2023-08-21T10:11:00Z","date_updated":"2023-08-22T13:15:02Z"},{"publication_status":"published","department":[{"_id":"JuFi"}],"publisher":"World Scientific","year":"2021","acknowledgement":"M. Bulíček and J. Málek acknowledge the support of the project No. 18-12719S financed by the Czech\r\nScience foundation (GAČR). E. Maringová acknowledges support from Charles University Research program \r\nUNCE/SCI/023, the grant SVV-2020-260583 by the Ministry of Education, Youth and Sports, Czech Republic\r\nand from the Austrian Science Fund (FWF), grants P30000, W1245, and F65. M. Bulíček and J. Málek are\r\nmembers of the Nečas Center for Mathematical Modelling.\r\n","date_created":"2021-09-12T22:01:25Z","date_updated":"2023-09-04T11:43:45Z","volume":31,"author":[{"first_name":"Miroslav","last_name":"Bulíček","full_name":"Bulíček, Miroslav"},{"full_name":"Maringová, Erika","first_name":"Erika","last_name":"Maringová","id":"dbabca31-66eb-11eb-963a-fb9c22c880b4"},{"first_name":"Josef","last_name":"Málek","full_name":"Málek, Josef"}],"quality_controlled":"1","isi":1,"project":[{"name":"Taming Complexity in Partial Differential Systems","grant_number":"F6504","_id":"fc31cba2-9c52-11eb-aca3-ff467d239cd2"}],"oa":1,"main_file_link":[{"open_access":"1","url":"https://arxiv.org/abs/2009.06917"}],"external_id":{"arxiv":["2009.06917"],"isi":["000722222900004"]},"language":[{"iso":"eng"}],"doi":"10.1142/S0218202521500457","month":"08","publication_identifier":{"issn":["0218-2025"],"eissn":["1793-6314"]},"status":"public","title":"On nonlinear problems of parabolic type with implicit constitutive equations involving flux","intvolume":" 31","_id":"10005","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","oa_version":"Preprint","type":"journal_article","abstract":[{"text":"We study systems of nonlinear partial differential equations of parabolic type, in which the elliptic operator is replaced by the first-order divergence operator acting on a flux function, which is related to the spatial gradient of the unknown through an additional implicit equation. This setting, broad enough in terms of applications, significantly expands the paradigm of nonlinear parabolic problems. Formulating four conditions concerning the form of the implicit equation, we first show that these conditions describe a maximal monotone p-coercive graph. We then establish the global-in-time and large-data existence of a (weak) solution and its uniqueness. To this end, we adopt and significantly generalize Minty’s method of monotone mappings. A unified theory, containing several novel tools, is developed in a way to be tractable from the point of view of numerical approximations.","lang":"eng"}],"issue":"09","article_type":"original","publication":"Mathematical Models and Methods in Applied Sciences","citation":{"short":"M. Bulíček, E. Maringová, J. Málek, Mathematical Models and Methods in Applied Sciences 31 (2021).","mla":"Bulíček, Miroslav, et al. “On Nonlinear Problems of Parabolic Type with Implicit Constitutive Equations Involving Flux.” Mathematical Models and Methods in Applied Sciences, vol. 31, no. 09, World Scientific, 2021, doi:10.1142/S0218202521500457.","chicago":"Bulíček, Miroslav, Erika Maringová, and Josef Málek. “On Nonlinear Problems of Parabolic Type with Implicit Constitutive Equations Involving Flux.” Mathematical Models and Methods in Applied Sciences. World Scientific, 2021. https://doi.org/10.1142/S0218202521500457.","ama":"Bulíček M, Maringová E, Málek J. On nonlinear problems of parabolic type with implicit constitutive equations involving flux. Mathematical Models and Methods in Applied Sciences. 2021;31(09). doi:10.1142/S0218202521500457","apa":"Bulíček, M., Maringová, E., & Málek, J. (2021). On nonlinear problems of parabolic type with implicit constitutive equations involving flux. Mathematical Models and Methods in Applied Sciences. World Scientific. https://doi.org/10.1142/S0218202521500457","ieee":"M. Bulíček, E. Maringová, and J. Málek, “On nonlinear problems of parabolic type with implicit constitutive equations involving flux,” Mathematical Models and Methods in Applied Sciences, vol. 31, no. 09. World Scientific, 2021.","ista":"Bulíček M, Maringová E, Málek J. 2021. On nonlinear problems of parabolic type with implicit constitutive equations involving flux. Mathematical Models and Methods in Applied Sciences. 31(09)."},"date_published":"2021-08-25T00:00:00Z","keyword":["Nonlinear parabolic systems","implicit constitutive theory","weak solutions","existence","uniqueness"],"scopus_import":"1","day":"25","article_processing_charge":"No"},{"article_processing_charge":"No","day":"21","keyword":["optimal","state machine replication","fallback","asynchrony","byzantine faults"],"scopus_import":"1","date_published":"2021-07-21T00:00:00Z","page":"187-190","citation":{"ama":"Gelashvili R, Kokoris Kogias E, Spiegelman A, Xiang Z. Brief announcement: Be prepared when network goes bad: An asynchronous view-change protocol. In: Proceedings of the 2021 ACM Symposium on Principles of Distributed Computing. Association for Computing Machinery; 2021:187-190. doi:10.1145/3465084.3467941","apa":"Gelashvili, R., Kokoris Kogias, E., Spiegelman, A., & Xiang, Z. (2021). Brief announcement: Be prepared when network goes bad: An asynchronous view-change protocol. In Proceedings of the 2021 ACM Symposium on Principles of Distributed Computing (pp. 187–190). Virtual, Italy: Association for Computing Machinery. https://doi.org/10.1145/3465084.3467941","ieee":"R. Gelashvili, E. Kokoris Kogias, A. Spiegelman, and Z. Xiang, “Brief announcement: Be prepared when network goes bad: An asynchronous view-change protocol,” in Proceedings of the 2021 ACM Symposium on Principles of Distributed Computing, Virtual, Italy, 2021, pp. 187–190.","ista":"Gelashvili R, Kokoris Kogias E, Spiegelman A, Xiang Z. 2021. Brief announcement: Be prepared when network goes bad: An asynchronous view-change protocol. Proceedings of the 2021 ACM Symposium on Principles of Distributed Computing. PODC: Principles of Distributed Computing, 187–190.","short":"R. Gelashvili, E. Kokoris Kogias, A. Spiegelman, Z. Xiang, in:, Proceedings of the 2021 ACM Symposium on Principles of Distributed Computing, Association for Computing Machinery, 2021, pp. 187–190.","mla":"Gelashvili, Rati, et al. “Brief Announcement: Be Prepared When Network Goes Bad: An Asynchronous View-Change Protocol.” Proceedings of the 2021 ACM Symposium on Principles of Distributed Computing, Association for Computing Machinery, 2021, pp. 187–90, doi:10.1145/3465084.3467941.","chicago":"Gelashvili, Rati, Eleftherios Kokoris Kogias, Alexander Spiegelman, and Zhuolun Xiang. “Brief Announcement: Be Prepared When Network Goes Bad: An Asynchronous View-Change Protocol.” In Proceedings of the 2021 ACM Symposium on Principles of Distributed Computing, 187–90. Association for Computing Machinery, 2021. https://doi.org/10.1145/3465084.3467941."},"publication":"Proceedings of the 2021 ACM Symposium on Principles of Distributed Computing","abstract":[{"lang":"eng","text":"The popularity of permissioned blockchain systems demands BFT SMR protocols that are efficient under good network conditions (synchrony) and robust under bad network conditions (asynchrony). The state-of-the-art partially synchronous BFT SMR protocols provide optimal linear communication cost per decision under synchrony and good leaders, but lose liveness under asynchrony. On the other hand, the state-of-the-art asynchronous BFT SMR protocols are live even under asynchrony, but always pay quadratic cost even under synchrony. In this paper, we propose a BFT SMR protocol that achieves the best of both worlds -- optimal linear cost per decision under good networks and leaders, optimal quadratic cost per decision under bad networks, and remains always live."}],"type":"conference","oa_version":"Preprint","title":"Brief announcement: Be prepared when network goes bad: An asynchronous view-change protocol","status":"public","_id":"10553","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","publication_identifier":{"isbn":["9-781-4503-8548-0"]},"month":"07","language":[{"iso":"eng"}],"doi":"10.1145/3465084.3467941","conference":{"end_date":"2021-07-30","location":"Virtual, Italy","start_date":"2021-07-26","name":"PODC: Principles of Distributed Computing"},"quality_controlled":"1","isi":1,"oa":1,"main_file_link":[{"url":"https://arxiv.org/abs/2103.03181","open_access":"1"}],"external_id":{"isi":["000744439800018"],"arxiv":["2103.03181"]},"date_created":"2021-12-16T13:20:19Z","date_updated":"2023-09-04T11:42:10Z","author":[{"full_name":"Gelashvili, Rati","first_name":"Rati","last_name":"Gelashvili"},{"full_name":"Kokoris Kogias, Eleftherios","first_name":"Eleftherios","last_name":"Kokoris Kogias","id":"f5983044-d7ef-11ea-ac6d-fd1430a26d30"},{"last_name":"Spiegelman","first_name":"Alexander","full_name":"Spiegelman, Alexander"},{"full_name":"Xiang, Zhuolun","last_name":"Xiang","first_name":"Zhuolun"}],"publisher":"Association for Computing Machinery","department":[{"_id":"ElKo"}],"publication_status":"published","year":"2021"},{"volume":126,"date_created":"2021-02-01T09:20:00Z","date_updated":"2023-09-05T12:08:58Z","author":[{"last_name":"De Nicola","first_name":"Stefano","orcid":"0000-0002-4842-6671","id":"42832B76-F248-11E8-B48F-1D18A9856A87","full_name":"De Nicola, Stefano"},{"last_name":"Michailidis","first_name":"Alexios","orcid":"0000-0002-8443-1064","id":"36EBAD38-F248-11E8-B48F-1D18A9856A87","full_name":"Michailidis, Alexios"},{"full_name":"Serbyn, Maksym","id":"47809E7E-F248-11E8-B48F-1D18A9856A87","orcid":"0000-0002-2399-5827","first_name":"Maksym","last_name":"Serbyn"}],"publisher":"American Physical Society","department":[{"_id":"MaSe"}],"publication_status":"published","year":"2021","acknowledgement":"S. D. N. acknowledges funding from the Institute of Science and Technology (IST) Austria and from the European Union’s Horizon 2020 Research and Innovation Programme under the Marie Skłodowska-Curie Grant Agreement No. 754411. A. M. and M. S. were supported by the European Research Council (ERC) under the European Union’s Horizon 2020 Research and\r\nInnovation Programme (Grant Agreement No. 850899).","ec_funded":1,"file_date_updated":"2021-02-03T12:47:04Z","article_number":"040602","language":[{"iso":"eng"}],"doi":"10.1103/physrevlett.126.040602","project":[{"_id":"260C2330-B435-11E9-9278-68D0E5697425","grant_number":"754411","call_identifier":"H2020","name":"ISTplus - Postdoctoral Fellowships"},{"grant_number":"850899","_id":"23841C26-32DE-11EA-91FC-C7463DDC885E","name":"Non-Ergodic Quantum Matter: Universality, Dynamics and Control","call_identifier":"H2020"}],"quality_controlled":"1","isi":1,"external_id":{"arxiv":["2008.04894"],"isi":["000613148200001"]},"tmp":{"name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)","image":"/images/cc_by.png"},"oa":1,"publication_identifier":{"eissn":["1079-7114"],"issn":["0031-9007"]},"month":"01","oa_version":"Published Version","file":[{"content_type":"application/pdf","file_size":398075,"creator":"dernst","file_name":"2021_PhysicalRevLett_DeNicola.pdf","access_level":"open_access","date_updated":"2021-02-03T12:47:04Z","date_created":"2021-02-03T12:47:04Z","checksum":"d9acbc502390ed7a97e631d23ae19ecd","success":1,"relation":"main_file","file_id":"9074"}],"intvolume":" 126","ddc":["530"],"title":"Entanglement view of dynamical quantum phase transitions","status":"public","user_id":"c635000d-4b10-11ee-a964-aac5a93f6ac1","_id":"9048","issue":"4","abstract":[{"lang":"eng","text":"The analogy between an equilibrium partition function and the return probability in many-body unitary dynamics has led to the concept of dynamical quantum phase transition (DQPT). DQPTs are defined by nonanalyticities in the return amplitude and are present in many models. In some cases, DQPTs can be related to equilibrium concepts, such as order parameters, yet their universal description is an open question. In this Letter, we provide first steps toward a classification of DQPTs by using a matrix product state description of unitary dynamics in the thermodynamic limit. This allows us to distinguish the two limiting cases of “precession” and “entanglement” DQPTs, which are illustrated using an analytical description in the quantum Ising model. While precession DQPTs are characterized by a large entanglement gap and are semiclassical in their nature, entanglement DQPTs occur near avoided crossings in the entanglement spectrum and can be distinguished by a complex pattern of nonlocal correlations. We demonstrate the existence of precession and entanglement DQPTs beyond Ising models, discuss observables that can distinguish them, and relate their interplay to complex DQPT phenomenology."}],"type":"journal_article","date_published":"2021-01-29T00:00:00Z","article_type":"original","citation":{"mla":"De Nicola, Stefano, et al. “Entanglement View of Dynamical Quantum Phase Transitions.” Physical Review Letters, vol. 126, no. 4, 040602, American Physical Society, 2021, doi:10.1103/physrevlett.126.040602.","short":"S. De Nicola, A. Michailidis, M. Serbyn, Physical Review Letters 126 (2021).","chicago":"De Nicola, Stefano, Alexios Michailidis, and Maksym Serbyn. “Entanglement View of Dynamical Quantum Phase Transitions.” Physical Review Letters. American Physical Society, 2021. https://doi.org/10.1103/physrevlett.126.040602.","ama":"De Nicola S, Michailidis A, Serbyn M. Entanglement view of dynamical quantum phase transitions. Physical Review Letters. 2021;126(4). doi:10.1103/physrevlett.126.040602","ista":"De Nicola S, Michailidis A, Serbyn M. 2021. Entanglement view of dynamical quantum phase transitions. Physical Review Letters. 126(4), 040602.","apa":"De Nicola, S., Michailidis, A., & Serbyn, M. (2021). Entanglement view of dynamical quantum phase transitions. Physical Review Letters. American Physical Society. https://doi.org/10.1103/physrevlett.126.040602","ieee":"S. De Nicola, A. Michailidis, and M. Serbyn, “Entanglement view of dynamical quantum phase transitions,” Physical Review Letters, vol. 126, no. 4. American Physical Society, 2021."},"publication":"Physical Review Letters","has_accepted_license":"1","article_processing_charge":"Yes","day":"29","keyword":["General Physics and Astronomy"]},{"publication_status":"published","publisher":"American Society of Plant Biologists","department":[{"_id":"JiFr"}],"acknowledgement":"We gratefully acknowledge the Arabidopsis Biological Resource Centre (ABRC) for providing T-DNA insertional mutants, and Prof. Remko Offringa for sharing published seeds. We thank Yuchuan Liu (Shanghai OE Biotech Co., Ltd) for help with proteomics data analysis, Xixi Zhang (IST Austria) for providing the pDONR-P4P1r-mCherry plasmid, and Yao Xiao (Technical University of Munich), Alexander Johnson (IST Austria) and Hana Semeradova (IST Austria) for helpful discussions. The study was supported by National Natural Science Foundation of China (NSFC, 31721001, 91954206, to H.-W. X.), “Ten-Thousand Talent Program” (to H.-W. X.) and Collaborative Innovation Center of Crop Stress Biology, Henan Province, and Austrian Science Fund (FWF): I 3630-B25 (to J. F.). S.T. was funded by a European Molecular Biology Organization (EMBO) long-term postdoctoral fellowship (ALTF 723-2015).","year":"2021","pmid":1,"date_created":"2021-05-03T13:28:20Z","date_updated":"2023-09-05T12:20:27Z","volume":186,"author":[{"full_name":"Kong, W","first_name":"W","last_name":"Kong"},{"first_name":"Shutang","last_name":"Tan","id":"2DE75584-F248-11E8-B48F-1D18A9856A87","orcid":"0000-0002-0471-8285","full_name":"Tan, Shutang"},{"full_name":"Zhao, Q","first_name":"Q","last_name":"Zhao"},{"first_name":"DL","last_name":"Lin","full_name":"Lin, DL"},{"full_name":"Xu, ZH","first_name":"ZH","last_name":"Xu"},{"full_name":"Friml, Jiří","last_name":"Friml","first_name":"Jiří","orcid":"0000-0002-8302-7596","id":"4159519E-F248-11E8-B48F-1D18A9856A87"},{"first_name":"HW","last_name":"Xue","full_name":"Xue, HW"}],"license":"https://creativecommons.org/licenses/by-nc-nd/4.0/","quality_controlled":"1","isi":1,"project":[{"name":"Long Term Fellowship","_id":"256FEF10-B435-11E9-9278-68D0E5697425","grant_number":"723-2015"},{"grant_number":"I03630","_id":"26538374-B435-11E9-9278-68D0E5697425","name":"Molecular mechanisms of endocytic cargo recognition in plants","call_identifier":"FWF"}],"main_file_link":[{"url":"https://doi.org/10.1093/plphys/kiab199","open_access":"1"}],"tmp":{"name":"Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND 4.0)","legal_code_url":"https://creativecommons.org/licenses/by-nc-nd/4.0/legalcode","short":"CC BY-NC-ND (4.0)","image":"/images/cc_by_nc_nd.png"},"external_id":{"isi":["000703922000025"],"pmid":["33930167"]},"oa":1,"language":[{"iso":"eng"}],"doi":"10.1093/plphys/kiab199","month":"04","publication_identifier":{"issn":["0032-0889"],"eissn":["1532-2548"]},"title":"mRNA surveillance complex PELOTA-HBS1 eegulates phosphoinositide-sependent protein kinase1 and plant growth","status":"public","intvolume":" 186","user_id":"c635000d-4b10-11ee-a964-aac5a93f6ac1","_id":"9368","oa_version":"Published Version","type":"journal_article","abstract":[{"text":"The quality control system for messenger RNA (mRNA) is fundamental for cellular activities in eukaryotes. To elucidate the molecular mechanism of 3'-Phosphoinositide-Dependent Protein Kinase1 (PDK1), a master regulator that is essential throughout eukaryotic growth and development, we employed a forward genetic approach to screen for suppressors of the loss-of-function T-DNA insertion double mutant pdk1.1 pdk1.2 in Arabidopsis thaliana. Notably, the severe growth attenuation of pdk1.1 pdk1.2 was rescued by sop21 (suppressor of pdk1.1 pdk1.2), which harbours a loss-of-function mutation in PELOTA1 (PEL1). PEL1 is a homologue of mammalian PELOTA and yeast (Saccharomyces cerevisiae) DOM34p, which each form a heterodimeric complex with the GTPase HBS1 (HSP70 SUBFAMILY B SUPPRESSOR1, also called SUPERKILLER PROTEIN7, SKI7), a protein that is responsible for ribosomal rescue and thereby assures the quality and fidelity of mRNA molecules during translation. Genetic analysis further revealed that a dysfunctional PEL1-HBS1 complex failed to degrade the T-DNA-disrupted PDK1 transcripts, which were truncated but functional, and thus rescued the growth and developmental defects of pdk1.1 pdk1.2. Our studies demonstrated the functionality of a homologous PELOTA-HBS1 complex and identified its essential regulatory role in plants, providing insights into the mechanism of mRNA quality control.","lang":"eng"}],"issue":"4","article_type":"original","page":"2003-2020","publication":"Plant Physiology","citation":{"mla":"Kong, W., et al. “MRNA Surveillance Complex PELOTA-HBS1 Eegulates Phosphoinositide-Sependent Protein Kinase1 and Plant Growth.” Plant Physiology, vol. 186, no. 4, American Society of Plant Biologists, 2021, pp. 2003–20, doi:10.1093/plphys/kiab199.","short":"W. Kong, S. Tan, Q. Zhao, D. Lin, Z. Xu, J. Friml, H. Xue, Plant Physiology 186 (2021) 2003–2020.","chicago":"Kong, W, Shutang Tan, Q Zhao, DL Lin, ZH Xu, Jiří Friml, and HW Xue. “MRNA Surveillance Complex PELOTA-HBS1 Eegulates Phosphoinositide-Sependent Protein Kinase1 and Plant Growth.” Plant Physiology. American Society of Plant Biologists, 2021. https://doi.org/10.1093/plphys/kiab199.","ama":"Kong W, Tan S, Zhao Q, et al. mRNA surveillance complex PELOTA-HBS1 eegulates phosphoinositide-sependent protein kinase1 and plant growth. Plant Physiology. 2021;186(4):2003-2020. doi:10.1093/plphys/kiab199","ista":"Kong W, Tan S, Zhao Q, Lin D, Xu Z, Friml J, Xue H. 2021. mRNA surveillance complex PELOTA-HBS1 eegulates phosphoinositide-sependent protein kinase1 and plant growth. Plant Physiology. 186(4), 2003–2020.","ieee":"W. Kong et al., “mRNA surveillance complex PELOTA-HBS1 eegulates phosphoinositide-sependent protein kinase1 and plant growth,” Plant Physiology, vol. 186, no. 4. American Society of Plant Biologists, pp. 2003–2020, 2021.","apa":"Kong, W., Tan, S., Zhao, Q., Lin, D., Xu, Z., Friml, J., & Xue, H. (2021). mRNA surveillance complex PELOTA-HBS1 eegulates phosphoinositide-sependent protein kinase1 and plant growth. Plant Physiology. American Society of Plant Biologists. https://doi.org/10.1093/plphys/kiab199"},"date_published":"2021-04-30T00:00:00Z","day":"30","article_processing_charge":"No"},{"abstract":[{"text":"A tight frame is the orthogonal projection of some orthonormal basis of Rn onto Rk. We show that a set of vectors is a tight frame if and only if the set of all cross products of these vectors is a tight frame. We reformulate a range of problems on the volume of projections (or sections) of regular polytopes in terms of tight frames and write a first-order necessary condition for local extrema of these problems. As applications, we prove new results for the problem of maximization of the volume of zonotopes.","lang":"eng"}],"issue":"4","type":"journal_article","oa_version":"Preprint","title":"Tight frames and related geometric problems","status":"public","intvolume":" 64","_id":"10860","user_id":"c635000d-4b10-11ee-a964-aac5a93f6ac1","day":"18","article_processing_charge":"No","keyword":["General Mathematics","Tight frame","Grassmannian","zonotope"],"scopus_import":"1","date_published":"2021-12-18T00:00:00Z","article_type":"original","page":"942-963","publication":"Canadian Mathematical Bulletin","citation":{"ama":"Ivanov G. Tight frames and related geometric problems. Canadian Mathematical Bulletin. 2021;64(4):942-963. doi:10.4153/s000843952000096x","ieee":"G. Ivanov, “Tight frames and related geometric problems,” Canadian Mathematical Bulletin, vol. 64, no. 4. Canadian Mathematical Society, pp. 942–963, 2021.","apa":"Ivanov, G. (2021). Tight frames and related geometric problems. Canadian Mathematical Bulletin. Canadian Mathematical Society. https://doi.org/10.4153/s000843952000096x","ista":"Ivanov G. 2021. Tight frames and related geometric problems. Canadian Mathematical Bulletin. 64(4), 942–963.","short":"G. Ivanov, Canadian Mathematical Bulletin 64 (2021) 942–963.","mla":"Ivanov, Grigory. “Tight Frames and Related Geometric Problems.” Canadian Mathematical Bulletin, vol. 64, no. 4, Canadian Mathematical Society, 2021, pp. 942–63, doi:10.4153/s000843952000096x.","chicago":"Ivanov, Grigory. “Tight Frames and Related Geometric Problems.” Canadian Mathematical Bulletin. Canadian Mathematical Society, 2021. https://doi.org/10.4153/s000843952000096x."},"date_updated":"2023-09-05T12:43:09Z","date_created":"2022-03-18T09:55:59Z","volume":64,"author":[{"last_name":"Ivanov","first_name":"Grigory","id":"87744F66-5C6F-11EA-AFE0-D16B3DDC885E","full_name":"Ivanov, Grigory"}],"publication_status":"published","publisher":"Canadian Mathematical Society","department":[{"_id":"UlWa"}],"year":"2021","acknowledgement":"The author was supported by the Swiss National Science Foundation grant 200021_179133. The author acknowledges the financial support from the Ministry of Education and Science of the Russian Federation in the framework of MegaGrant no. 075-15-2019-1926.","month":"12","publication_identifier":{"issn":["0008-4395"],"eissn":["1496-4287"]},"language":[{"iso":"eng"}],"doi":"10.4153/s000843952000096x","isi":1,"quality_controlled":"1","oa":1,"external_id":{"arxiv":["1804.10055"],"isi":["000730165300021"]},"main_file_link":[{"open_access":"1","url":"https://arxiv.org/abs/1804.10055"}]},{"user_id":"c635000d-4b10-11ee-a964-aac5a93f6ac1","_id":"9290","intvolume":" 31","ddc":["580"],"title":"AGC kinases and MAB4/MEL proteins maintain PIN polarity by limiting lateral diffusion in plant cells","status":"public","file":[{"date_updated":"2021-04-01T10:53:42Z","date_created":"2021-04-01T10:53:42Z","success":1,"checksum":"b1723040ecfd8c81194185472eb62546","file_id":"9303","relation":"main_file","creator":"dernst","content_type":"application/pdf","file_size":4324371,"file_name":"2021_CurrentBiology_Glanc.pdf","access_level":"open_access"}],"oa_version":"Published Version","type":"journal_article","issue":"9","abstract":[{"lang":"eng","text":"Polar subcellular localization of the PIN exporters of the phytohormone auxin is a key determinant of directional, intercellular auxin transport and thus a central topic of both plant cell and developmental biology. Arabidopsis mutants lacking PID, a kinase that phosphorylates PINs, or the MAB4/MEL proteins of unknown molecular function display PIN polarity defects and phenocopy pin mutants, but mechanistic insights into how these factors convey PIN polarity are missing. Here, by combining protein biochemistry with quantitative live-cell imaging, we demonstrate that PINs, MAB4/MELs, and AGC kinases interact in the same complex at the plasma membrane. MAB4/MELs are recruited to the plasma membrane by the PINs and in concert with the AGC kinases maintain PIN polarity through limiting lateral diffusion-based escape of PINs from the polar domain. The PIN-MAB4/MEL-PID protein complex has self-reinforcing properties thanks to positive feedback between AGC kinase-mediated PIN phosphorylation and MAB4/MEL recruitment. We thus uncover the molecular mechanism by which AGC kinases and MAB4/MEL proteins regulate PIN localization and plant development."}],"citation":{"apa":"Glanc, M., Van Gelderen, K., Hörmayer, L., Tan, S., Naramoto, S., Zhang, X., … Friml, J. (2021). AGC kinases and MAB4/MEL proteins maintain PIN polarity by limiting lateral diffusion in plant cells. Current Biology. Elsevier. https://doi.org/10.1016/j.cub.2021.02.028","ieee":"M. Glanc et al., “AGC kinases and MAB4/MEL proteins maintain PIN polarity by limiting lateral diffusion in plant cells,” Current Biology, vol. 31, no. 9. Elsevier, pp. 1918–1930, 2021.","ista":"Glanc M, Van Gelderen K, Hörmayer L, Tan S, Naramoto S, Zhang X, Domjan D, Vcelarova L, Hauschild R, Johnson AJ, de Koning E, van Dop M, Rademacher E, Janson S, Wei X, Molnar G, Fendrych M, De Rybel B, Offringa R, Friml J. 2021. AGC kinases and MAB4/MEL proteins maintain PIN polarity by limiting lateral diffusion in plant cells. Current Biology. 31(9), 1918–1930.","ama":"Glanc M, Van Gelderen K, Hörmayer L, et al. AGC kinases and MAB4/MEL proteins maintain PIN polarity by limiting lateral diffusion in plant cells. Current Biology. 2021;31(9):1918-1930. doi:10.1016/j.cub.2021.02.028","chicago":"Glanc, Matous, K Van Gelderen, Lukas Hörmayer, Shutang Tan, S Naramoto, Xixi Zhang, David Domjan, et al. “AGC Kinases and MAB4/MEL Proteins Maintain PIN Polarity by Limiting Lateral Diffusion in Plant Cells.” Current Biology. Elsevier, 2021. https://doi.org/10.1016/j.cub.2021.02.028.","short":"M. Glanc, K. Van Gelderen, L. Hörmayer, S. Tan, S. Naramoto, X. Zhang, D. Domjan, L. Vcelarova, R. Hauschild, A.J. Johnson, E. de Koning, M. van Dop, E. Rademacher, S. Janson, X. Wei, G. Molnar, M. Fendrych, B. De Rybel, R. Offringa, J. Friml, Current Biology 31 (2021) 1918–1930.","mla":"Glanc, Matous, et al. “AGC Kinases and MAB4/MEL Proteins Maintain PIN Polarity by Limiting Lateral Diffusion in Plant Cells.” Current Biology, vol. 31, no. 9, Elsevier, 2021, pp. 1918–30, doi:10.1016/j.cub.2021.02.028."},"publication":"Current Biology","page":"1918-1930","article_type":"original","date_published":"2021-03-10T00:00:00Z","article_processing_charge":"No","has_accepted_license":"1","day":"10","pmid":1,"year":"2021","acknowledgement":"We acknowledge Ben Scheres, Christian Luschnig, and Claus Schwechheimer for sharing published material. We thank Monika Hrtyan and Dorota Jaworska at IST Austria and Gerda Lamers and Ward de Winter at IBL Netherlands for technical assistance; Corinna Hartinger, Jakub Hajný, Lesia Rodriguez, Mingyue Li, and Lindy Abas for experimental support; and the Bioimaging Facility at IST Austria and the Bioimaging Core at VIB for imaging support. We are grateful to Christian Luschnig, Lindy Abas, and Roman Pleskot for valuable discussions. We also acknowledge the EMBO for supporting M.G. with a long-term fellowship ( ALTF 1005-2019 ) during the finalization and revision of this manuscript in the laboratory of B.D.R., and we thank R. Pierik for allowing K.V.G. to work on this manuscript during a postdoc in his laboratory at Utrecht University. This work was supported by grants from the European Research Council under the European Union’s Seventh Framework Programme (ERC grant agreements 742985 to J.F., 714055 to B.D.R., and 803048 to M.F.), the Austrian Science Fund (FWF; I 3630-B25 to J.F.), Chemical Sciences (partly) financed by the Dutch Research Council (NWO-CW TOP 700.58.301 to R.O.), the Dutch Research Council (NWO-VICI 865.17.002 to R. Pierik), Grants-in-Aid from the Ministry of Education, Culture, Sports, Science and Technology, Japan (KAKENHI grant 17K17595 to S.N.), the Ministry of Education, Youth and Sports of the Czech Republic (MŠMT project NPUI-LO1417 ), and a China Scholarship Council (to X.W.).","department":[{"_id":"JiFr"}],"publisher":"Elsevier","publication_status":"published","author":[{"orcid":"0000-0003-0619-7783","id":"1AE1EA24-02D0-11E9-9BAA-DAF4881429F2","last_name":"Glanc","first_name":"Matous","full_name":"Glanc, Matous"},{"first_name":"K","last_name":"Van Gelderen","full_name":"Van Gelderen, K"},{"full_name":"Hörmayer, Lukas","id":"2EEE7A2A-F248-11E8-B48F-1D18A9856A87","orcid":"0000-0001-8295-2926","first_name":"Lukas","last_name":"Hörmayer"},{"full_name":"Tan, Shutang","first_name":"Shutang","last_name":"Tan","id":"2DE75584-F248-11E8-B48F-1D18A9856A87","orcid":"0000-0002-0471-8285"},{"first_name":"S","last_name":"Naramoto","full_name":"Naramoto, S"},{"last_name":"Zhang","first_name":"Xixi","orcid":"0000-0001-7048-4627","id":"61A66458-47E9-11EA-85BA-8AEAAF14E49A","full_name":"Zhang, Xixi"},{"full_name":"Domjan, David","id":"C684CD7A-257E-11EA-9B6F-D8588B4F947F","orcid":"0000-0003-2267-106X","first_name":"David","last_name":"Domjan"},{"full_name":"Vcelarova, L","first_name":"L","last_name":"Vcelarova"},{"full_name":"Hauschild, Robert","last_name":"Hauschild","first_name":"Robert","orcid":"0000-0001-9843-3522","id":"4E01D6B4-F248-11E8-B48F-1D18A9856A87"},{"full_name":"Johnson, Alexander J","last_name":"Johnson","first_name":"Alexander J","orcid":"0000-0002-2739-8843","id":"46A62C3A-F248-11E8-B48F-1D18A9856A87"},{"full_name":"de Koning, E","last_name":"de Koning","first_name":"E"},{"last_name":"van Dop","first_name":"M","full_name":"van Dop, M"},{"full_name":"Rademacher, E","last_name":"Rademacher","first_name":"E"},{"first_name":"S","last_name":"Janson","full_name":"Janson, S"},{"last_name":"Wei","first_name":"X","full_name":"Wei, X"},{"first_name":"Gergely","last_name":"Molnar","id":"34F1AF46-F248-11E8-B48F-1D18A9856A87","full_name":"Molnar, Gergely"},{"id":"43905548-F248-11E8-B48F-1D18A9856A87","orcid":"0000-0002-9767-8699","first_name":"Matyas","last_name":"Fendrych","full_name":"Fendrych, Matyas"},{"first_name":"B","last_name":"De Rybel","full_name":"De Rybel, B"},{"first_name":"R","last_name":"Offringa","full_name":"Offringa, R"},{"id":"4159519E-F248-11E8-B48F-1D18A9856A87","orcid":"0000-0002-8302-7596","first_name":"Jiří","last_name":"Friml","full_name":"Friml, Jiří"}],"volume":31,"date_updated":"2023-09-05T13:03:34Z","date_created":"2021-03-26T12:09:33Z","ec_funded":1,"file_date_updated":"2021-04-01T10:53:42Z","oa":1,"tmp":{"name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)","image":"/images/cc_by.png"},"external_id":{"isi":["000653077800004"],"pmid":["33705718"]},"project":[{"name":"Tracing Evolution of Auxin Transport and Polarity in Plants","call_identifier":"H2020","grant_number":"742985","_id":"261099A6-B435-11E9-9278-68D0E5697425"},{"name":"Molecular mechanisms of endocytic cargo recognition in plants","call_identifier":"FWF","_id":"26538374-B435-11E9-9278-68D0E5697425","grant_number":"I03630"}],"quality_controlled":"1","isi":1,"doi":"10.1016/j.cub.2021.02.028","language":[{"iso":"eng"}],"acknowledged_ssus":[{"_id":"Bio"}],"publication_identifier":{"issn":["0960-9822"],"eissn":["1879-0445"]},"month":"03"},{"quality_controlled":"1","isi":1,"tmp":{"name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","short":"CC BY (4.0)","image":"/images/cc_by.png"},"oa":1,"external_id":{"pmid":["33157019"],"isi":["000614361000039"]},"language":[{"iso":"eng"}],"doi":"10.1016/j.cub.2020.10.011","month":"01","publication_identifier":{"eissn":["1879-0445"],"issn":["0960-9822"]},"publication_status":"published","department":[{"_id":"JiFr"}],"publisher":"Elsevier","acknowledgement":"We thank the SiCE group for discussions and comments; S. Yalovsky, B. Scheres, and the NASC/ABRC collection for providing transgenic Arabidopsis lines and plasmids; L. Kalmbach and M. Barberon for the gift of pLOK180_pFR7m34GW; A. Lacroix, J. Berger, and P. Bolland for plant care; and M. Fendrych for help with microfluidics in the J.F. lab. We acknowledge\r\nthe contribution of the SFR Biosciences (UMS3444/CNRS, US8/Inser m, ENS de Lyon, UCBL) facilities: C. Lionet, E. Chatre, and J. Brocard at LBIPLATIM-MICROSCOPY for assistance with imaging, and V. GuegenChaignon and A. Page at the Protein Science Facility (PSF) for assistance with protein purification and mass spectrometry. Y.J. was funded by ERC\r\ngrant 3363360-APPL under FP/2007–2013. Y.J. and Z.L.N. were funded by an ANR- and NSF-supported ERA-CAPS project (SICOPID: ANR-17-CAPS0003-01/NSF PGRP IOS-1841917). A.I.C.-D. is funded by an ERC consolidator grant (ERC-2015-CoG–683163) and BIO2016-78955 grant from the Spanish Ministry of Economy and Competitiveness. Exchanges between the Y.J. and T.B. laboratories were funded by Tournesol grant 35656NB. B.K.M. was\r\nfunded by the Omics@vib Marie Curie COFUND and Research Foundation Flanders for a postdoctoral fellowship.","year":"2021","pmid":1,"date_created":"2020-12-01T13:39:46Z","date_updated":"2023-09-05T13:03:15Z","volume":31,"author":[{"full_name":"Marquès-Bueno, MM","last_name":"Marquès-Bueno","first_name":"MM"},{"full_name":"Armengot, L","first_name":"L","last_name":"Armengot"},{"first_name":"LC","last_name":"Noack","full_name":"Noack, LC"},{"last_name":"Bareille","first_name":"J","full_name":"Bareille, J"},{"full_name":"Rodriguez Solovey, Lesia","id":"3922B506-F248-11E8-B48F-1D18A9856A87","orcid":"0000-0002-7244-7237","first_name":"Lesia","last_name":"Rodriguez Solovey"},{"full_name":"Platre, MP","first_name":"MP","last_name":"Platre"},{"full_name":"Bayle, V","first_name":"V","last_name":"Bayle"},{"last_name":"Liu","first_name":"M","full_name":"Liu, M"},{"first_name":"D","last_name":"Opdenacker","full_name":"Opdenacker, D"},{"full_name":"Vanneste, S","last_name":"Vanneste","first_name":"S"},{"first_name":"BK","last_name":"Möller","full_name":"Möller, BK"},{"full_name":"Nimchuk, ZL","first_name":"ZL","last_name":"Nimchuk"},{"full_name":"Beeckman, T","first_name":"T","last_name":"Beeckman"},{"first_name":"AI","last_name":"Caño-Delgado","full_name":"Caño-Delgado, AI"},{"last_name":"Friml","first_name":"Jiří","orcid":"0000-0002-8302-7596","id":"4159519E-F248-11E8-B48F-1D18A9856A87","full_name":"Friml, Jiří"},{"first_name":"Y","last_name":"Jaillais","full_name":"Jaillais, Y"}],"file_date_updated":"2021-02-04T11:37:50Z","article_type":"original","publication":"Current Biology","citation":{"chicago":"Marquès-Bueno, MM, L Armengot, LC Noack, J Bareille, Lesia Rodriguez Solovey, MP Platre, V Bayle, et al. “Auxin-Regulated Reversible Inhibition of TMK1 Signaling by MAKR2 Modulates the Dynamics of Root Gravitropism.” Current Biology. Elsevier, 2021. https://doi.org/10.1016/j.cub.2020.10.011.","mla":"Marquès-Bueno, MM, et al. “Auxin-Regulated Reversible Inhibition of TMK1 Signaling by MAKR2 Modulates the Dynamics of Root Gravitropism.” Current Biology, vol. 31, no. 1, Elsevier, 2021, doi:10.1016/j.cub.2020.10.011.","short":"M. Marquès-Bueno, L. Armengot, L. Noack, J. Bareille, L. Rodriguez Solovey, M. Platre, V. Bayle, M. Liu, D. Opdenacker, S. Vanneste, B. Möller, Z. Nimchuk, T. Beeckman, A. Caño-Delgado, J. Friml, Y. Jaillais, Current Biology 31 (2021).","ista":"Marquès-Bueno M, Armengot L, Noack L, Bareille J, Rodriguez Solovey L, Platre M, Bayle V, Liu M, Opdenacker D, Vanneste S, Möller B, Nimchuk Z, Beeckman T, Caño-Delgado A, Friml J, Jaillais Y. 2021. Auxin-regulated reversible inhibition of TMK1 signaling by MAKR2 modulates the dynamics of root gravitropism. Current Biology. 31(1).","ieee":"M. Marquès-Bueno et al., “Auxin-regulated reversible inhibition of TMK1 signaling by MAKR2 modulates the dynamics of root gravitropism,” Current Biology, vol. 31, no. 1. Elsevier, 2021.","apa":"Marquès-Bueno, M., Armengot, L., Noack, L., Bareille, J., Rodriguez Solovey, L., Platre, M., … Jaillais, Y. (2021). Auxin-regulated reversible inhibition of TMK1 signaling by MAKR2 modulates the dynamics of root gravitropism. Current Biology. Elsevier. https://doi.org/10.1016/j.cub.2020.10.011","ama":"Marquès-Bueno M, Armengot L, Noack L, et al. Auxin-regulated reversible inhibition of TMK1 signaling by MAKR2 modulates the dynamics of root gravitropism. Current Biology. 2021;31(1). doi:10.1016/j.cub.2020.10.011"},"date_published":"2021-01-11T00:00:00Z","day":"11","has_accepted_license":"1","article_processing_charge":"Yes (via OA deal)","title":"Auxin-regulated reversible inhibition of TMK1 signaling by MAKR2 modulates the dynamics of root gravitropism","ddc":["570"],"status":"public","intvolume":" 31","user_id":"c635000d-4b10-11ee-a964-aac5a93f6ac1","_id":"8824","oa_version":"Published Version","file":[{"creator":"dernst","content_type":"application/pdf","file_size":3458646,"access_level":"open_access","file_name":"2021_CurrentBiology_MarquesBueno.pdf","success":1,"checksum":"30b3393d841fb2b1e2b22fb42b5c8fff","date_updated":"2021-02-04T11:37:50Z","date_created":"2021-02-04T11:37:50Z","file_id":"9090","relation":"main_file"}],"type":"journal_article","abstract":[{"lang":"eng","text":"Plants are able to orient their growth according to gravity, which ultimately controls both shoot and root architecture.1 Gravitropism is a dynamic process whereby gravistimulation induces the asymmetric distribution of the plant hormone auxin, leading to asymmetric growth, organ bending, and subsequent reset of auxin distribution back to the original pre-gravistimulation situation.1, 2, 3 Differential auxin accumulation during the gravitropic response depends on the activity of polarly localized PIN-FORMED (PIN) auxin-efflux carriers.1, 2, 3, 4 In particular, the timing of this dynamic response is regulated by PIN2,5,6 but the underlying molecular mechanisms are poorly understood. Here, we show that MEMBRANE ASSOCIATED KINASE REGULATOR2 (MAKR2) controls the pace of the root gravitropic response. We found that MAKR2 is required for the PIN2 asymmetry during gravitropism by acting as a negative regulator of the cell-surface signaling mediated by the receptor-like kinase TRANSMEMBRANE KINASE1 (TMK1).2,7, 8, 9, 10 Furthermore, we show that the MAKR2 inhibitory effect on TMK1 signaling is antagonized by auxin itself, which triggers rapid MAKR2 membrane dissociation in a TMK1-dependent manner. Our findings suggest that the timing of the root gravitropic response is orchestrated by the reversible inhibition of the TMK1 signaling pathway at the cell surface."}],"issue":"1"}]