---
_id: '13457'
abstract:
- lang: eng
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."
article_number: A70
article_processing_charge: No
article_type: original
author:
- first_name: J.
full_name: Bodensteiner, J.
last_name: Bodensteiner
- first_name: H.
full_name: Sana, H.
last_name: Sana
- first_name: C.
full_name: Wang, C.
last_name: Wang
- first_name: N.
full_name: Langer, N.
last_name: Langer
- first_name: L.
full_name: Mahy, L.
last_name: Mahy
- first_name: G.
full_name: Banyard, G.
last_name: Banyard
- first_name: A.
full_name: de Koter, A.
last_name: de Koter
- first_name: S. E.
full_name: de Mink, S. E.
last_name: de Mink
- first_name: C. J.
full_name: Evans, C. J.
last_name: Evans
- first_name: Ylva Louise Linsdotter
full_name: Götberg, Ylva Louise Linsdotter
id: d0648d0c-0f64-11ee-a2e0-dd0faa2e4f7d
last_name: Götberg
orcid: 0000-0002-6960-6911
- first_name: L. R.
full_name: Patrick, L. R.
last_name: Patrick
- first_name: F. R. N.
full_name: Schneider, F. R. N.
last_name: Schneider
- first_name: F.
full_name: Tramper, F.
last_name: Tramper
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
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
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.
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.
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.
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).
date_created: 2023-08-03T10:11:34Z
date_published: 2021-08-12T00:00:00Z
date_updated: 2023-08-21T11:49:36Z
day: '12'
doi: 10.1051/0004-6361/202140507
extern: '1'
external_id:
arxiv:
- '2104.13409'
intvolume: ' 652'
keyword:
- Space and Planetary Science
- Astronomy and Astrophysics
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://doi.org/10.1051/0004-6361/202140507
month: '08'
oa: 1
oa_version: Published Version
publication: Astronomy & Astrophysics
publication_identifier:
eissn:
- 1432-0746
issn:
- 0004-6361
publication_status: published
publisher: EDP Sciences
quality_controlled: '1'
scopus_import: '1'
status: public
title: The young massive SMC cluster NGC 330 seen by MUSE. II. Multiplicity properties
of the massive-star population
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 652
year: '2021'
...
---
_id: '13455'
abstract:
- lang: eng
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.
article_number: A58
article_processing_charge: No
article_type: original
author:
- first_name: E.
full_name: Laplace, E.
last_name: Laplace
- first_name: S.
full_name: Justham, S.
last_name: Justham
- first_name: M.
full_name: Renzo, M.
last_name: Renzo
- first_name: Ylva Louise Linsdotter
full_name: Götberg, Ylva Louise Linsdotter
id: d0648d0c-0f64-11ee-a2e0-dd0faa2e4f7d
last_name: Götberg
orcid: 0000-0002-6960-6911
- first_name: R.
full_name: Farmer, R.
last_name: Farmer
- first_name: D.
full_name: Vartanyan, D.
last_name: Vartanyan
- first_name: S. E.
full_name: de Mink, S. E.
last_name: de Mink
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'
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'
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.'
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.'
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.'
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).
date_created: 2023-08-03T10:11:09Z
date_published: 2021-12-02T00:00:00Z
date_updated: 2023-08-21T11:49:15Z
day: '02'
doi: 10.1051/0004-6361/202140506
external_id:
arxiv:
- '2102.05036'
intvolume: ' 656'
keyword:
- Space and Planetary Science
- Astronomy and Astrophysics
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://doi.org/10.1051/0004-6361/202140506
month: '12'
oa: 1
oa_version: Published Version
publication: Astronomy & Astrophysics
publication_identifier:
eissn:
- 1432-0746
issn:
- 0004-6361
publication_status: published
publisher: EDP Sciences
quality_controlled: '1'
scopus_import: '1'
status: public
title: 'Different to the core: The pre-supernova structures of massive single and
binary-stripped stars'
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 656
year: '2021'
...
---
_id: '13454'
abstract:
- lang: eng
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.
article_number: '241'
article_processing_charge: No
article_type: original
author:
- first_name: Tin Long Sunny
full_name: Wong, Tin Long Sunny
last_name: Wong
- first_name: Josiah
full_name: Schwab, Josiah
last_name: Schwab
- first_name: Ylva Louise Linsdotter
full_name: Götberg, Ylva Louise Linsdotter
id: d0648d0c-0f64-11ee-a2e0-dd0faa2e4f7d
last_name: Götberg
orcid: 0000-0002-6960-6911
citation:
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
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
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.
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.
ista: Wong TLS, Schwab J, Götberg YLL. 2021. Pre-explosion properties of Helium
star donors to thermonuclear supernovae. The Astrophysical Journal. 922(2), 241.
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).
date_created: 2023-08-03T10:10:58Z
date_published: 2021-12-03T00:00:00Z
date_updated: 2023-08-21T11:52:05Z
day: '03'
doi: 10.3847/1538-4357/ac27ae
extern: '1'
external_id:
arxiv:
- '2109.14817'
intvolume: ' 922'
issue: '2'
keyword:
- Space and Planetary Science
- Astronomy and Astrophysics
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://arxiv.org/abs/2109.14817
month: '12'
oa: 1
oa_version: Preprint
publication: The Astrophysical Journal
publication_identifier:
eissn:
- 1538-4357
issn:
- 0004-637X
publication_status: published
publisher: American Astronomical Society
quality_controlled: '1'
scopus_import: '1'
status: public
title: Pre-explosion properties of Helium star donors to thermonuclear supernovae
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 922
year: '2021'
...
---
_id: '13453'
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.
article_number: '277'
article_processing_charge: No
article_type: original
author:
- first_name: M.
full_name: Renzo, M.
last_name: Renzo
- first_name: Ylva Louise Linsdotter
full_name: Götberg, Ylva Louise Linsdotter
id: d0648d0c-0f64-11ee-a2e0-dd0faa2e4f7d
last_name: Götberg
orcid: 0000-0002-6960-6911
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'
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'
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.'
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.'
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.'
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).
date_created: 2023-08-03T10:10:48Z
date_published: 2021-12-29T00:00:00Z
date_updated: 2023-08-21T11:59:34Z
day: '29'
doi: 10.3847/1538-4357/ac29c5
extern: '1'
external_id:
arxiv:
- '2107.10933'
intvolume: ' 923'
issue: '2'
keyword:
- Space and Planetary Science
- Astronomy and Astrophysics
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://arxiv.org/abs/2107.10933
month: '12'
oa: 1
oa_version: Preprint
publication: The Astrophysical Journal
publication_identifier:
eissn:
- 1538-4357
issn:
- 0004-637X
publication_status: published
publisher: American Astronomical Society
quality_controlled: '1'
scopus_import: '1'
status: public
title: 'Evolution of accretor stars in massive binaries: Broader implications from
modeling ζ Ophiuchi'
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 923
year: '2021'
...
---
_id: '13996'
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.
article_processing_charge: No
article_type: original
author:
- first_name: Denitsa Rangelova
full_name: Baykusheva, Denitsa Rangelova
id: 71b4d059-2a03-11ee-914d-dfa3beed6530
last_name: Baykusheva
- first_name: Alexis
full_name: Chacón, Alexis
last_name: Chacón
- first_name: Jian
full_name: Lu, Jian
last_name: Lu
- first_name: Trevor P.
full_name: Bailey, Trevor P.
last_name: Bailey
- first_name: Jonathan A.
full_name: Sobota, Jonathan A.
last_name: Sobota
- first_name: Hadas
full_name: Soifer, Hadas
last_name: Soifer
- first_name: Patrick S.
full_name: Kirchmann, Patrick S.
last_name: Kirchmann
- first_name: Costel
full_name: Rotundu, Costel
last_name: Rotundu
- first_name: Ctirad
full_name: Uher, Ctirad
last_name: Uher
- first_name: Tony F.
full_name: Heinz, Tony F.
last_name: Heinz
- first_name: David A.
full_name: Reis, David A.
last_name: Reis
- first_name: Shambhu
full_name: Ghimire, Shambhu
last_name: Ghimire
citation:
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
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
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.
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.
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.
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.
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.
date_created: 2023-08-09T13:09:15Z
date_published: 2021-10-22T00:00:00Z
date_updated: 2023-08-22T07:32:00Z
day: '22'
doi: 10.1021/acs.nanolett.1c02145
extern: '1'
external_id:
arxiv:
- '2109.15291'
pmid:
- '34676752'
intvolume: ' 21'
issue: '21'
keyword:
- Mechanical Engineering
- Condensed Matter Physics
- General Materials Science
- General Chemistry
- Bioengineering
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://doi.org/10.1021/acs.nanolett.1c02145
month: '10'
oa: 1
oa_version: Published Version
page: 8970-8978
pmid: 1
publication: Nano Letters
publication_identifier:
eissn:
- 1530-6992
issn:
- 1530-6984
publication_status: published
publisher: American Chemical Society
quality_controlled: '1'
scopus_import: '1'
status: public
title: All-optical probe of three-dimensional topological insulators based on high-harmonic
generation by circularly polarized laser fields
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 21
year: '2021'
...