--- _id: '17549' abstract: - lang: eng text: Studies of rest-frame optical emission in quasars at z>6 have historically been limited by the wavelengths accessible by ground-based telescopes. The James Webb Space Telescope (JWST) now offers the opportunity to probe this emission deep into the reionization epoch. We report the observations of eight quasars at z>6.5 using the JWST/NIRCam Wide Field Slitless Spectroscopy, as a part of the ''A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE)" program. Our JWST spectra cover the quasars' emission between rest frame ∼ 4100 and 5100 Å. The profiles of these quasars' broad Hβ emission lines span a FWHM from 3000 to 6000 km s−1. The Hβ-based virial black hole (BH) masses, ranging from 0.6 to 2.1 billion solar masses, are generally consistent with their MgII-based BH masses. The new measurements based on the more reliable Hβ tracer thus confirm the existence of billion solar-mass BHs in the reionization epoch. In the observed [OIII] λλ4960,5008 doublets of these luminous quasars, broad components are more common than narrow core components (≤ 1200 km s−1), and only one quasar shows stronger narrow components than broad. Two quasars exhibit significantly broad and blueshifted [OIII] emission, thought to trace galactic-scale outflows, with median velocities of −610 km s−1 and −1430 km s−1 relative to the [CII] 158μm line. All eight quasars show strong optical FeII emission, and follow the Eigenvector 1 relations defined by low-redshift quasars. The entire ASPIRE program will eventually cover 25 quasars and provide a statistical sample for the studies of the BHs and quasar spectral properties. article_number: L5 article_processing_charge: No article_type: original author: - first_name: Jinyi full_name: Yang, Jinyi last_name: Yang - first_name: Feige full_name: Wang, Feige last_name: Wang - first_name: Xiaohui full_name: Fan, Xiaohui last_name: Fan - first_name: Joseph F. full_name: Hennawi, Joseph F. last_name: Hennawi - first_name: Aaron J. full_name: Barth, Aaron J. last_name: Barth - first_name: Eduardo full_name: Bañados, Eduardo last_name: Bañados - first_name: Fengwu full_name: Sun, Fengwu last_name: Sun - first_name: Weizhe full_name: Liu, Weizhe last_name: Liu - first_name: Zheng full_name: Cai, Zheng last_name: Cai - first_name: Linhua full_name: Jiang, Linhua last_name: Jiang - first_name: Zihao full_name: Li, Zihao last_name: Li - first_name: Masafusa full_name: Onoue, Masafusa last_name: Onoue - first_name: Jan-Torge full_name: Schindler, Jan-Torge last_name: Schindler - first_name: Yue full_name: Shen, Yue last_name: Shen - first_name: Yunjing full_name: Wu, Yunjing last_name: Wu - first_name: Aklant K. full_name: Bhowmick, Aklant K. last_name: Bhowmick - first_name: Rebekka full_name: Bieri, Rebekka last_name: Bieri - first_name: Laura full_name: Blecha, Laura last_name: Blecha - first_name: Sarah full_name: Bosman, Sarah last_name: Bosman - first_name: Jaclyn B. full_name: Champagne, Jaclyn B. last_name: Champagne - first_name: Luis full_name: Colina, Luis last_name: Colina - first_name: Thomas full_name: Connor, Thomas last_name: Connor - first_name: Tiago full_name: Costa, Tiago last_name: Costa - first_name: Frederick B. full_name: Davies, Frederick B. last_name: Davies - first_name: Roberto full_name: Decarli, Roberto last_name: Decarli - first_name: Gisella full_name: De Rosa, Gisella last_name: De Rosa - first_name: Alyssa B. full_name: Drake, Alyssa B. last_name: Drake - first_name: Eiichi full_name: Egami, Eiichi last_name: Egami - first_name: Anna-Christina full_name: Eilers, Anna-Christina last_name: Eilers - first_name: Analis E. full_name: Evans, Analis E. last_name: Evans - first_name: Emanuele Paolo full_name: Farina, Emanuele Paolo last_name: Farina - first_name: Melanie full_name: Habouzit, Melanie last_name: Habouzit - first_name: Zoltán full_name: Haiman, Zoltán id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36 last_name: Haiman - first_name: Xiangyu full_name: Jin, Xiangyu last_name: Jin - first_name: Hyunsung D. full_name: Jun, Hyunsung D. last_name: Jun - first_name: Koki full_name: Kakiichi, Koki last_name: Kakiichi - first_name: Yana full_name: Khusanova, Yana last_name: Khusanova - first_name: Girish full_name: Kulkarni, Girish last_name: Kulkarni - first_name: Federica full_name: Loiacono, Federica last_name: Loiacono - first_name: Alessandro full_name: Lupi, Alessandro last_name: Lupi - first_name: Chiara full_name: Mazzucchelli, Chiara last_name: Mazzucchelli - first_name: Zhiwei full_name: Pan, Zhiwei last_name: Pan - first_name: Sofía full_name: Rojas-Ruiz, Sofía last_name: Rojas-Ruiz - first_name: Michael A. full_name: Strauss, Michael A. last_name: Strauss - first_name: Wei Leong full_name: Tee, Wei Leong last_name: Tee - first_name: Benny full_name: Trakhtenbrot, Benny last_name: Trakhtenbrot - first_name: Maxime full_name: Trebitsch, Maxime last_name: Trebitsch - first_name: Bram full_name: Venemans, Bram last_name: Venemans - first_name: Marianne full_name: Vestergaard, Marianne last_name: Vestergaard - first_name: Marta full_name: Volonteri, Marta last_name: Volonteri - first_name: Fabian full_name: Walter, Fabian last_name: Walter - first_name: Zhang-Liang full_name: Xie, Zhang-Liang last_name: Xie - first_name: Minghao full_name: Yue, Minghao last_name: Yue - first_name: Haowen full_name: Zhang, Haowen last_name: Zhang - first_name: Huanian full_name: Zhang, Huanian last_name: Zhang - first_name: Siwei full_name: Zou, Siwei last_name: Zou citation: ama: 'Yang J, Wang F, Fan X, et al. A SPectroscopic survey of biased halos in the reionization Era (ASPIRE): A first look at the rest-frame optical spectra of > 6.5 quasars using JWST. The Astrophysical Journal Letters. 2023;951(1). doi:10.3847/2041-8213/acc9c8' apa: 'Yang, J., Wang, F., Fan, X., Hennawi, J. F., Barth, A. J., Bañados, E., … Zou, S. (2023). A SPectroscopic survey of biased halos in the reionization Era (ASPIRE): A first look at the rest-frame optical spectra of > 6.5 quasars using JWST. The Astrophysical Journal Letters. American Astronomical Society. https://doi.org/10.3847/2041-8213/acc9c8' chicago: 'Yang, Jinyi, Feige Wang, Xiaohui Fan, Joseph F. Hennawi, Aaron J. Barth, Eduardo Bañados, Fengwu Sun, et al. “A SPectroscopic Survey of Biased Halos in the Reionization Era (ASPIRE): A First Look at the Rest-Frame Optical Spectra of > 6.5 Quasars Using JWST.” The Astrophysical Journal Letters. American Astronomical Society, 2023. https://doi.org/10.3847/2041-8213/acc9c8.' ieee: 'J. Yang et al., “A SPectroscopic survey of biased halos in the reionization Era (ASPIRE): A first look at the rest-frame optical spectra of > 6.5 quasars using JWST,” The Astrophysical Journal Letters, vol. 951, no. 1. American Astronomical Society, 2023.' ista: 'Yang J, Wang F, Fan X, Hennawi JF, Barth AJ, Bañados E, Sun F, Liu W, Cai Z, Jiang L, Li Z, Onoue M, Schindler J-T, Shen Y, Wu Y, Bhowmick AK, Bieri R, Blecha L, Bosman S, Champagne JB, Colina L, Connor T, Costa T, Davies FB, Decarli R, De Rosa G, Drake AB, Egami E, Eilers A-C, Evans AE, Farina EP, Habouzit M, Haiman Z, Jin X, Jun HD, Kakiichi K, Khusanova Y, Kulkarni G, Loiacono F, Lupi A, Mazzucchelli C, Pan Z, Rojas-Ruiz S, Strauss MA, Tee WL, Trakhtenbrot B, Trebitsch M, Venemans B, Vestergaard M, Volonteri M, Walter F, Xie Z-L, Yue M, Zhang H, Zhang H, Zou S. 2023. A SPectroscopic survey of biased halos in the reionization Era (ASPIRE): A first look at the rest-frame optical spectra of > 6.5 quasars using JWST. The Astrophysical Journal Letters. 951(1), L5.' mla: 'Yang, Jinyi, et al. “A SPectroscopic Survey of Biased Halos in the Reionization Era (ASPIRE): A First Look at the Rest-Frame Optical Spectra of > 6.5 Quasars Using JWST.” The Astrophysical Journal Letters, vol. 951, no. 1, L5, American Astronomical Society, 2023, doi:10.3847/2041-8213/acc9c8.' short: J. Yang, F. Wang, X. Fan, J.F. Hennawi, A.J. Barth, E. Bañados, F. Sun, W. Liu, Z. Cai, L. Jiang, Z. Li, M. Onoue, J.-T. Schindler, Y. Shen, Y. Wu, A.K. Bhowmick, R. Bieri, L. Blecha, S. Bosman, J.B. Champagne, L. Colina, T. Connor, T. Costa, F.B. Davies, R. Decarli, G. De Rosa, A.B. Drake, E. Egami, A.-C. Eilers, A.E. Evans, E.P. Farina, M. Habouzit, Z. Haiman, X. Jin, H.D. Jun, K. Kakiichi, Y. Khusanova, G. Kulkarni, F. Loiacono, A. Lupi, C. Mazzucchelli, Z. Pan, S. Rojas-Ruiz, M.A. Strauss, W.L. Tee, B. Trakhtenbrot, M. Trebitsch, B. Venemans, M. Vestergaard, M. Volonteri, F. Walter, Z.-L. Xie, M. Yue, H. Zhang, H. Zhang, S. Zou, The Astrophysical Journal Letters 951 (2023). date_created: 2024-09-05T10:11:02Z date_published: 2023-06-29T00:00:00Z date_updated: 2024-09-18T09:53:12Z day: '29' doi: 10.3847/2041-8213/acc9c8 extern: '1' intvolume: ' 951' issue: '1' language: - iso: eng main_file_link: - open_access: '1' url: https://doi.org/10.3847/2041-8213/acc9c8 month: '06' oa: 1 oa_version: Published Version publication: The Astrophysical Journal Letters publication_identifier: issn: - 2041-8205 - 2041-8213 publication_status: published publisher: American Astronomical Society quality_controlled: '1' scopus_import: '1' status: public title: 'A SPectroscopic survey of biased halos in the reionization Era (ASPIRE): A first look at the rest-frame optical spectra of > 6.5 quasars using JWST' type: journal_article user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345 volume: 951 year: '2023' ... --- _id: '17551' abstract: - lang: eng text: We present cosmological constraints from the Subaru Hyper Suprime-Cam (HSC) first-year weak lensing shear catalogue using convolutional neural networks (CNNs) and conventional summary statistics. We crop 19 3×3deg2 sub-fields from the first-year area, divide the galaxies with redshift 0.3≤z≤1.5 into four equally-spaced redshift bins, and perform tomographic analyses. We develop a pipeline to generate simulated convergence maps from cosmological N-body simulations, where we account for effects such as intrinsic alignments (IAs), baryons, photometric redshift errors, and point spread function errors, to match characteristics of the real catalogue. We train CNNs that can predict the underlying parameters from the simulated maps, and we use them to construct likelihood functions for Bayesian analyses. In the Λ cold dark matter model with two free cosmological parameters Ωm and σ8, we find Ωm=0.278+0.037−0.035, S8≡(Ωm/0.3)0.5σ8=0.793+0.017−0.018, and the IA amplitude AIA=0.20+0.55−0.58. In a model with four additional free baryonic parameters, we find Ωm=0.268+0.040−0.036, S8=0.819+0.034−0.024, and AIA=−0.16+0.59−0.58, with the baryonic parameters not being well-constrained. We also find that statistical uncertainties of the parameters by the CNNs are smaller than those from the power spectrum (5--24 percent smaller for S8 and a factor of 2.5--3.0 smaller for Ωm), showing the effectiveness of CNNs for uncovering additional cosmological information from the HSC data. With baryons, the S8 discrepancy between HSC first-year data and Planck 2018 is reduced from ∼2.2σ to 0.3--0.5σ. article_processing_charge: No article_type: original author: - first_name: Tianhuan full_name: Lu, Tianhuan last_name: Lu - first_name: Zoltán full_name: Haiman, Zoltán id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36 last_name: Haiman - first_name: Xiangchong full_name: Li, Xiangchong last_name: Li citation: ama: Lu T, Haiman Z, Li X. Cosmological constraints from HSC survey first-year data using deep learning. Monthly Notices of the Royal Astronomical Society. 2023;521(2):2050-2066. doi:10.1093/mnras/stad686 apa: Lu, T., Haiman, Z., & Li, X. (2023). Cosmological constraints from HSC survey first-year data using deep learning. Monthly Notices of the Royal Astronomical Society. Oxford University Press. https://doi.org/10.1093/mnras/stad686 chicago: Lu, Tianhuan, Zoltán Haiman, and Xiangchong Li. “Cosmological Constraints from HSC Survey First-Year Data Using Deep Learning.” Monthly Notices of the Royal Astronomical Society. Oxford University Press, 2023. https://doi.org/10.1093/mnras/stad686. ieee: T. Lu, Z. Haiman, and X. Li, “Cosmological constraints from HSC survey first-year data using deep learning,” Monthly Notices of the Royal Astronomical Society, vol. 521, no. 2. Oxford University Press, pp. 2050–2066, 2023. ista: Lu T, Haiman Z, Li X. 2023. Cosmological constraints from HSC survey first-year data using deep learning. Monthly Notices of the Royal Astronomical Society. 521(2), 2050–2066. mla: Lu, Tianhuan, et al. “Cosmological Constraints from HSC Survey First-Year Data Using Deep Learning.” Monthly Notices of the Royal Astronomical Society, vol. 521, no. 2, Oxford University Press, 2023, pp. 2050–66, doi:10.1093/mnras/stad686. short: T. Lu, Z. Haiman, X. Li, Monthly Notices of the Royal Astronomical Society 521 (2023) 2050–2066. date_created: 2024-09-05T10:14:34Z date_published: 2023-03-06T00:00:00Z date_updated: 2024-09-18T10:09:01Z day: '06' doi: 10.1093/mnras/stad686 extern: '1' intvolume: ' 521' issue: '2' language: - iso: eng main_file_link: - open_access: '1' url: https://doi.org/10.1093/mnras/stad686 month: '03' oa: 1 oa_version: Published Version page: 2050-2066 publication: Monthly Notices of the Royal Astronomical Society publication_identifier: issn: - 0035-8711 - 1365-2966 publication_status: published publisher: Oxford University Press quality_controlled: '1' scopus_import: '1' status: public title: Cosmological constraints from HSC survey first-year data using deep learning type: journal_article user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345 volume: 521 year: '2023' ... --- _id: '17557' abstract: - lang: eng text: The black hole (BH) binaries in active galactic nuclei (AGN) are expected to form mainly through scattering encounters in the ambient gaseous medium. Recent simulations, including our own, have confirmed this formation pathway is highly efficient. We perform 3D smoothed particle hydrodynamics (SPH) simulations of BH scattering encounters in AGN discs. Using a range of impact parameters, we probe the necessary conditions for binary capture and how different orbital trajectories affect the dissipative effects from the gas. We identify a single range of impact parameters, typically of width ∼0.86−1.59 binary Hill radii depending on AGN disc density, that reliably leads to binary formation. The periapsis of the first encounter is the primary variable that determines the outcome of the initial scattering. We find an associated power law between the energy dissipated and the periapsis depth to be ΔE ∝ r−b with b = 0.42 ± 0.16, where deeper encounters dissipate more energy. Excluding accretion physics does not significantly alter these results. We identify the region of parameter space in initial energy versus impact parameter where a scattering leads to binary formation. Based on our findings, we provide a ready-to-use analytic criterion that utilizes these two pre-encounter parameters to determine the outcome of an encounter, with a reliability rate of >90 per cent. As the criterion is based directly on our simulations, it provides a reliable and highly physically motivated criterion for predicting binary scattering outcomes which can be used in population studies of BH binaries and mergers around AGN. article_processing_charge: No article_type: original author: - first_name: Connar full_name: Rowan, Connar last_name: Rowan - first_name: Henry full_name: Whitehead, Henry last_name: Whitehead - first_name: Tjarda full_name: Boekholt, Tjarda last_name: Boekholt - first_name: Bence full_name: Kocsis, Bence last_name: Kocsis - first_name: Zoltán full_name: Haiman, Zoltán id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36 last_name: Haiman citation: ama: Rowan C, Whitehead H, Boekholt T, Kocsis B, Haiman Z. Black hole binaries in AGN accretion discs – II. Gas effects on black hole satellite scatterings. Monthly Notices of the Royal Astronomical Society. 2023;527(4):10448-10468. doi:10.1093/mnras/stad3641 apa: Rowan, C., Whitehead, H., Boekholt, T., Kocsis, B., & Haiman, Z. (2023). Black hole binaries in AGN accretion discs – II. Gas effects on black hole satellite scatterings. Monthly Notices of the Royal Astronomical Society. Oxford University Press (OUP). https://doi.org/10.1093/mnras/stad3641 chicago: Rowan, Connar, Henry Whitehead, Tjarda Boekholt, Bence Kocsis, and Zoltán Haiman. “Black Hole Binaries in AGN Accretion Discs – II. Gas Effects on Black Hole Satellite Scatterings.” Monthly Notices of the Royal Astronomical Society. Oxford University Press (OUP), 2023. https://doi.org/10.1093/mnras/stad3641. ieee: C. Rowan, H. Whitehead, T. Boekholt, B. Kocsis, and Z. Haiman, “Black hole binaries in AGN accretion discs – II. Gas effects on black hole satellite scatterings,” Monthly Notices of the Royal Astronomical Society, vol. 527, no. 4. Oxford University Press (OUP), pp. 10448–10468, 2023. ista: Rowan C, Whitehead H, Boekholt T, Kocsis B, Haiman Z. 2023. Black hole binaries in AGN accretion discs – II. Gas effects on black hole satellite scatterings. Monthly Notices of the Royal Astronomical Society. 527(4), 10448–10468. mla: Rowan, Connar, et al. “Black Hole Binaries in AGN Accretion Discs – II. Gas Effects on Black Hole Satellite Scatterings.” Monthly Notices of the Royal Astronomical Society, vol. 527, no. 4, Oxford University Press (OUP), 2023, pp. 10448–68, doi:10.1093/mnras/stad3641. short: C. Rowan, H. Whitehead, T. Boekholt, B. Kocsis, Z. Haiman, Monthly Notices of the Royal Astronomical Society 527 (2023) 10448–10468. date_created: 2024-09-05T10:32:08Z date_published: 2023-01-01T00:00:00Z date_updated: 2024-09-18T12:11:28Z doi: 10.1093/mnras/stad3641 extern: '1' intvolume: ' 527' issue: '4' language: - iso: eng main_file_link: - open_access: '1' url: https://doi.org/10.1093/mnras/stad3641 month: '01' oa: 1 oa_version: Published Version page: 10448-10468 publication: Monthly Notices of the Royal Astronomical Society publication_identifier: issn: - 0035-8711 - 1365-2966 publication_status: published publisher: Oxford University Press (OUP) quality_controlled: '1' scopus_import: '1' status: public title: Black hole binaries in AGN accretion discs – II. Gas effects on black hole satellite scatterings type: journal_article user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345 volume: 527 year: '2023' ... --- _id: '17558' abstract: - lang: eng text: The detection of starlight from the host galaxies of quasars during the reionization epoch (z > 6) has been elusive, even with deep Hubble Space Telescope observations1,2. The current highest redshift quasar host detected3, at z = 4.5, required the magnifying effect of a foreground lensing galaxy. Low-luminosity quasars4,5,6 from the Hyper Suprime-Cam Subaru Strategic Program (HSC-SSP)7 mitigate the challenge of detecting their underlying, previously undetected host galaxies. Here we report rest-frame optical images and spectroscopy of two HSC-SSP quasars at z > 6 with the JWST. Using near-infrared camera imaging at 3.6 and 1.5 μm and subtracting the light from the unresolved quasars, we find that the host galaxies are massive (stellar masses of 13 × and 3.4 × 1010 M☉, respectively), compact and disc-like. Near-infrared spectroscopy at medium resolution shows stellar absorption lines in the more massive quasar, confirming the detection of the host. Velocity-broadened gas in the vicinity of these quasars enables measurements of their black hole masses (1.4 × 109 and 2.0 × 108 M☉, respectively). Their location in the black hole mass–stellar mass plane is consistent with the distribution at low redshift, suggesting that the relation between black holes and their host galaxies was already in place less than a billion years after the Big Bang. article_processing_charge: No article_type: original arxiv: 1 author: - first_name: Xuheng full_name: Ding, Xuheng last_name: Ding - first_name: Masafusa full_name: Onoue, Masafusa last_name: Onoue - first_name: John D. full_name: Silverman, John D. last_name: Silverman - first_name: Yoshiki full_name: Matsuoka, Yoshiki last_name: Matsuoka - first_name: Takuma full_name: Izumi, Takuma last_name: Izumi - first_name: Michael A. full_name: Strauss, Michael A. last_name: Strauss - first_name: Knud full_name: Jahnke, Knud last_name: Jahnke - first_name: Camryn L. full_name: Phillips, Camryn L. last_name: Phillips - first_name: Junyao full_name: Li, Junyao last_name: Li - first_name: Marta full_name: Volonteri, Marta last_name: Volonteri - first_name: Zoltán full_name: Haiman, Zoltán id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36 last_name: Haiman - first_name: Irham Taufik full_name: Andika, Irham Taufik last_name: Andika - first_name: Kentaro full_name: Aoki, Kentaro last_name: Aoki - first_name: Shunsuke full_name: Baba, Shunsuke last_name: Baba - first_name: Rebekka full_name: Bieri, Rebekka last_name: Bieri - first_name: Sarah E. I. full_name: Bosman, Sarah E. I. last_name: Bosman - first_name: Connor full_name: Bottrell, Connor last_name: Bottrell - first_name: Anna-Christina full_name: Eilers, Anna-Christina last_name: Eilers - first_name: Seiji full_name: Fujimoto, Seiji last_name: Fujimoto - first_name: Melanie full_name: Habouzit, Melanie last_name: Habouzit - first_name: Masatoshi full_name: Imanishi, Masatoshi last_name: Imanishi - first_name: Kohei full_name: Inayoshi, Kohei last_name: Inayoshi - first_name: Kazushi full_name: Iwasawa, Kazushi last_name: Iwasawa - first_name: Nobunari full_name: Kashikawa, Nobunari last_name: Kashikawa - first_name: Toshihiro full_name: Kawaguchi, Toshihiro last_name: Kawaguchi - first_name: Kotaro full_name: Kohno, Kotaro last_name: Kohno - first_name: Chien-Hsiu full_name: Lee, Chien-Hsiu last_name: Lee - first_name: Alessandro full_name: Lupi, Alessandro last_name: Lupi - first_name: Jianwei full_name: Lyu, Jianwei last_name: Lyu - first_name: Tohru full_name: Nagao, Tohru last_name: Nagao - first_name: Roderik full_name: Overzier, Roderik last_name: Overzier - first_name: Jan-Torge full_name: Schindler, Jan-Torge last_name: Schindler - first_name: Malte full_name: Schramm, Malte last_name: Schramm - first_name: Kazuhiro full_name: Shimasaku, Kazuhiro last_name: Shimasaku - first_name: Yoshiki full_name: Toba, Yoshiki last_name: Toba - first_name: Benny full_name: Trakhtenbrot, Benny last_name: Trakhtenbrot - first_name: Maxime full_name: Trebitsch, Maxime last_name: Trebitsch - first_name: Tommaso full_name: Treu, Tommaso last_name: Treu - first_name: Hideki full_name: Umehata, Hideki last_name: Umehata - first_name: Bram P. full_name: Venemans, Bram P. last_name: Venemans - first_name: Marianne full_name: Vestergaard, Marianne last_name: Vestergaard - first_name: Fabian full_name: Walter, Fabian last_name: Walter - first_name: Feige full_name: Wang, Feige last_name: Wang - first_name: Jinyi full_name: Yang, Jinyi last_name: Yang citation: ama: Ding X, Onoue M, Silverman JD, et al. Detection of stellar light from quasar host galaxies at redshifts above 6. Nature. 2023;621(7977):51-55. doi:10.1038/s41586-023-06345-5 apa: Ding, X., Onoue, M., Silverman, J. D., Matsuoka, Y., Izumi, T., Strauss, M. A., … Yang, J. (2023). Detection of stellar light from quasar host galaxies at redshifts above 6. Nature. Springer Science and Business Media LLC. https://doi.org/10.1038/s41586-023-06345-5 chicago: Ding, Xuheng, Masafusa Onoue, John D. Silverman, Yoshiki Matsuoka, Takuma Izumi, Michael A. Strauss, Knud Jahnke, et al. “Detection of Stellar Light from Quasar Host Galaxies at Redshifts above 6.” Nature. Springer Science and Business Media LLC, 2023. https://doi.org/10.1038/s41586-023-06345-5. ieee: X. Ding et al., “Detection of stellar light from quasar host galaxies at redshifts above 6,” Nature, vol. 621, no. 7977. Springer Science and Business Media LLC, pp. 51–55, 2023. ista: Ding X, Onoue M, Silverman JD, Matsuoka Y, Izumi T, Strauss MA, Jahnke K, Phillips CL, Li J, Volonteri M, Haiman Z, Andika IT, Aoki K, Baba S, Bieri R, Bosman SEI, Bottrell C, Eilers A-C, Fujimoto S, Habouzit M, Imanishi M, Inayoshi K, Iwasawa K, Kashikawa N, Kawaguchi T, Kohno K, Lee C-H, Lupi A, Lyu J, Nagao T, Overzier R, Schindler J-T, Schramm M, Shimasaku K, Toba Y, Trakhtenbrot B, Trebitsch M, Treu T, Umehata H, Venemans BP, Vestergaard M, Walter F, Wang F, Yang J. 2023. Detection of stellar light from quasar host galaxies at redshifts above 6. Nature. 621(7977), 51–55. mla: Ding, Xuheng, et al. “Detection of Stellar Light from Quasar Host Galaxies at Redshifts above 6.” Nature, vol. 621, no. 7977, Springer Science and Business Media LLC, 2023, pp. 51–55, doi:10.1038/s41586-023-06345-5. short: X. Ding, M. Onoue, J.D. Silverman, Y. Matsuoka, T. Izumi, M.A. Strauss, K. Jahnke, C.L. Phillips, J. Li, M. Volonteri, Z. Haiman, I.T. Andika, K. Aoki, S. Baba, R. Bieri, S.E.I. Bosman, C. Bottrell, A.-C. Eilers, S. Fujimoto, M. Habouzit, M. Imanishi, K. Inayoshi, K. Iwasawa, N. Kashikawa, T. Kawaguchi, K. Kohno, C.-H. Lee, A. Lupi, J. Lyu, T. Nagao, R. Overzier, J.-T. Schindler, M. Schramm, K. Shimasaku, Y. Toba, B. Trakhtenbrot, M. Trebitsch, T. Treu, H. Umehata, B.P. Venemans, M. Vestergaard, F. Walter, F. Wang, J. Yang, Nature 621 (2023) 51–55. date_created: 2024-09-05T11:28:21Z date_published: 2023-06-28T00:00:00Z date_updated: 2024-09-18T12:19:50Z day: '28' doi: 10.1038/s41586-023-06345-5 extern: '1' external_id: arxiv: - '2211.14329' intvolume: ' 621' issue: '7977' language: - iso: eng main_file_link: - open_access: '1' url: ' https://doi.org/10.48550/arXiv.2211.14329' month: '06' oa: 1 oa_version: Preprint page: 51-55 publication: Nature publication_identifier: issn: - 0028-0836 - 1476-4687 publication_status: published publisher: Springer Science and Business Media LLC quality_controlled: '1' scopus_import: '1' status: public title: Detection of stellar light from quasar host galaxies at redshifts above 6 type: journal_article user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345 volume: 621 year: '2023' ... --- _id: '17573' abstract: - lang: eng text: The Laser Interferometer Space Antenna (LISA) will be a transformative experiment for gravitational wave astronomy, and, as such, it will offer unique opportunities to address many key astrophysical questions in a completely novel way. The synergy with ground-based and space-born instruments in the electromagnetic domain, by enabling multi-messenger observations, will add further to the discovery potential of LISA. The next decade is crucial to prepare the astrophysical community for LISA’s first observations. This review outlines the extensive landscape of astrophysical theory, numerical simulations, and astronomical observations that are instrumental for modeling and interpreting the upcoming LISA datastream. To this aim, the current knowledge in three main source classes for LISA is reviewed; ultra-compact stellar-mass binaries, massive black hole binaries, and extreme or interme-diate mass ratio inspirals. The relevant astrophysical processes and the established modeling techniques are summarized. Likewise, open issues and gaps in our understanding of these sources are highlighted, along with an indication of how LISA could help making progress in the different areas. New research avenues that LISA itself, or its joint exploitation with upcoming studies in the electromagnetic domain, will enable, are also illustrated. Improvements in modeling and analysis approaches, such as the combination of numerical simulations and modern data science techniques, are discussed. This review is intended to be a starting point for using LISA as a new discovery tool for understanding our Universe. article_number: '2' article_processing_charge: No article_type: original author: - first_name: Pau full_name: Amaro-Seoane, Pau last_name: Amaro-Seoane - first_name: Jeff full_name: Andrews, Jeff last_name: Andrews - first_name: Manuel full_name: Arca Sedda, Manuel last_name: Arca Sedda - first_name: Abbas full_name: Askar, Abbas last_name: Askar - first_name: Quentin full_name: Baghi, Quentin last_name: Baghi - first_name: Razvan full_name: Balasov, Razvan last_name: Balasov - first_name: Imre full_name: Bartos, Imre last_name: Bartos - first_name: Simone S. full_name: Bavera, Simone S. last_name: Bavera - first_name: Jillian full_name: Bellovary, Jillian last_name: Bellovary - first_name: Christopher P. L. full_name: Berry, Christopher P. L. last_name: Berry - first_name: Emanuele full_name: Berti, Emanuele last_name: Berti - first_name: Stefano full_name: Bianchi, Stefano last_name: Bianchi - first_name: Laura full_name: Blecha, Laura last_name: Blecha - first_name: Stéphane full_name: Blondin, Stéphane last_name: Blondin - first_name: Tamara full_name: Bogdanović, Tamara last_name: Bogdanović - first_name: Samuel full_name: Boissier, Samuel last_name: Boissier - first_name: Matteo full_name: Bonetti, Matteo last_name: Bonetti - first_name: Silvia full_name: Bonoli, Silvia last_name: Bonoli - first_name: Elisa full_name: Bortolas, Elisa last_name: Bortolas - first_name: Katelyn full_name: Breivik, Katelyn last_name: Breivik - first_name: Pedro R. full_name: Capelo, Pedro R. last_name: Capelo - first_name: Laurentiu full_name: Caramete, Laurentiu last_name: Caramete - first_name: Federico full_name: Cattorini, Federico last_name: Cattorini - first_name: Maria full_name: Charisi, Maria last_name: Charisi - first_name: Sylvain full_name: Chaty, Sylvain last_name: Chaty - first_name: Xian full_name: Chen, Xian last_name: Chen - first_name: Martyna full_name: Chruślińska, Martyna last_name: Chruślińska - first_name: Alvin J. K. full_name: Chua, Alvin J. K. last_name: Chua - first_name: Ross full_name: Church, Ross last_name: Church - first_name: Monica full_name: Colpi, Monica last_name: Colpi - first_name: Daniel full_name: D’Orazio, Daniel last_name: D’Orazio - first_name: Camilla full_name: Danielski, Camilla last_name: Danielski - first_name: Melvyn B. full_name: Davies, Melvyn B. last_name: Davies - first_name: Pratika full_name: Dayal, Pratika last_name: Dayal - first_name: Alessandra full_name: De Rosa, Alessandra last_name: De Rosa - first_name: Andrea full_name: Derdzinski, Andrea last_name: Derdzinski - first_name: Kyriakos full_name: Destounis, Kyriakos last_name: Destounis - first_name: Massimo full_name: Dotti, Massimo last_name: Dotti - first_name: Ioana full_name: Duţan, Ioana last_name: Duţan - first_name: Irina full_name: Dvorkin, Irina last_name: Dvorkin - first_name: Gaia full_name: Fabj, Gaia last_name: Fabj - first_name: Thierry full_name: Foglizzo, Thierry last_name: Foglizzo - first_name: Saavik full_name: Ford, Saavik last_name: Ford - first_name: Jean-Baptiste full_name: Fouvry, Jean-Baptiste last_name: Fouvry - first_name: Alessia full_name: Franchini, Alessia last_name: Franchini - first_name: Tassos full_name: Fragos, Tassos last_name: Fragos - first_name: Chris full_name: Fryer, Chris last_name: Fryer - first_name: Massimo full_name: Gaspari, Massimo last_name: Gaspari - first_name: Davide full_name: Gerosa, Davide last_name: Gerosa - first_name: Luca full_name: Graziani, Luca last_name: Graziani - first_name: Paul full_name: Groot, Paul last_name: Groot - first_name: Melanie full_name: Habouzit, Melanie last_name: Habouzit - first_name: Daryl full_name: Haggard, Daryl last_name: Haggard - first_name: Zoltán full_name: Haiman, Zoltán id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36 last_name: Haiman - first_name: Wen-Biao full_name: Han, Wen-Biao last_name: Han - first_name: Alina full_name: Istrate, Alina last_name: Istrate - first_name: Peter H. full_name: Johansson, Peter H. last_name: Johansson - first_name: Fazeel Mahmood full_name: Khan, Fazeel Mahmood last_name: Khan - first_name: Tomas full_name: Kimpson, Tomas last_name: Kimpson - first_name: Kostas full_name: Kokkotas, Kostas last_name: Kokkotas - first_name: Albert full_name: Kong, Albert last_name: Kong - first_name: Valeriya full_name: Korol, Valeriya last_name: Korol - first_name: Kyle full_name: Kremer, Kyle last_name: Kremer - first_name: Thomas full_name: Kupfer, Thomas last_name: Kupfer - first_name: Astrid full_name: Lamberts, Astrid last_name: Lamberts - first_name: Shane full_name: Larson, Shane last_name: Larson - first_name: Mike full_name: Lau, Mike last_name: Lau - first_name: Dongliang full_name: Liu, Dongliang last_name: Liu - first_name: Nicole full_name: Lloyd-Ronning, Nicole last_name: Lloyd-Ronning - first_name: Giuseppe full_name: Lodato, Giuseppe last_name: Lodato - first_name: Alessandro full_name: Lupi, Alessandro last_name: Lupi - first_name: Chung-Pei full_name: Ma, Chung-Pei last_name: Ma - first_name: Tomas full_name: Maccarone, Tomas last_name: Maccarone - first_name: Ilya full_name: Mandel, Ilya last_name: Mandel - first_name: Alberto full_name: Mangiagli, Alberto last_name: Mangiagli - first_name: Michela full_name: Mapelli, Michela last_name: Mapelli - first_name: Stéphane full_name: Mathis, Stéphane last_name: Mathis - first_name: Lucio full_name: Mayer, Lucio last_name: Mayer - first_name: Sean full_name: McGee, Sean last_name: McGee - first_name: Berry full_name: McKernan, Berry last_name: McKernan - first_name: M. Coleman full_name: Miller, M. Coleman last_name: Miller - first_name: David F. full_name: Mota, David F. last_name: Mota - first_name: Matthew full_name: Mumpower, Matthew last_name: Mumpower - first_name: Syeda S. full_name: Nasim, Syeda S. last_name: Nasim - first_name: Gijs full_name: Nelemans, Gijs last_name: Nelemans - first_name: Scott full_name: Noble, Scott last_name: Noble - first_name: Fabio full_name: Pacucci, Fabio last_name: Pacucci - first_name: Francesca full_name: Panessa, Francesca last_name: Panessa - first_name: Vasileios full_name: Paschalidis, Vasileios last_name: Paschalidis - first_name: Hugo full_name: Pfister, Hugo last_name: Pfister - first_name: Delphine full_name: Porquet, Delphine last_name: Porquet - first_name: John full_name: Quenby, John last_name: Quenby - first_name: Angelo full_name: Ricarte, Angelo last_name: Ricarte - first_name: Friedrich K. full_name: Röpke, Friedrich K. last_name: Röpke - first_name: John full_name: Regan, John last_name: Regan - first_name: Stephan full_name: Rosswog, Stephan last_name: Rosswog - first_name: Ashley full_name: Ruiter, Ashley last_name: Ruiter - first_name: Milton full_name: Ruiz, Milton last_name: Ruiz - first_name: Jessie full_name: Runnoe, Jessie last_name: Runnoe - first_name: Raffaella full_name: Schneider, Raffaella last_name: Schneider - first_name: Jeremy full_name: Schnittman, Jeremy last_name: Schnittman - first_name: Amy full_name: Secunda, Amy last_name: Secunda - first_name: Alberto full_name: Sesana, Alberto last_name: Sesana - first_name: Naoki full_name: Seto, Naoki last_name: Seto - first_name: Lijing full_name: Shao, Lijing last_name: Shao - first_name: Stuart full_name: Shapiro, Stuart last_name: Shapiro - first_name: Carlos full_name: Sopuerta, Carlos last_name: Sopuerta - first_name: Nicholas C. full_name: Stone, Nicholas C. last_name: Stone - first_name: Arthur full_name: Suvorov, Arthur last_name: Suvorov - first_name: Nicola full_name: Tamanini, Nicola last_name: Tamanini - first_name: Tomas full_name: Tamfal, Tomas last_name: Tamfal - first_name: Thomas full_name: Tauris, Thomas last_name: Tauris - first_name: Karel full_name: Temmink, Karel last_name: Temmink - first_name: John full_name: Tomsick, John last_name: Tomsick - first_name: Silvia full_name: Toonen, Silvia last_name: Toonen - first_name: Alejandro full_name: Torres-Orjuela, Alejandro last_name: Torres-Orjuela - first_name: Martina full_name: Toscani, Martina last_name: Toscani - first_name: Antonios full_name: Tsokaros, Antonios last_name: Tsokaros - first_name: Caner full_name: Unal, Caner last_name: Unal - first_name: Verónica full_name: Vázquez-Aceves, Verónica last_name: Vázquez-Aceves - first_name: Rosa full_name: Valiante, Rosa last_name: Valiante - first_name: Maurice full_name: van Putten, Maurice last_name: van Putten - first_name: Jan full_name: van Roestel, Jan last_name: van Roestel - first_name: Christian full_name: Vignali, Christian last_name: Vignali - first_name: Marta full_name: Volonteri, Marta last_name: Volonteri - first_name: Kinwah full_name: Wu, Kinwah last_name: Wu - first_name: Ziri full_name: Younsi, Ziri last_name: Younsi - first_name: Shenghua full_name: Yu, Shenghua last_name: Yu - first_name: Silvia full_name: Zane, Silvia last_name: Zane - first_name: Lorenz full_name: Zwick, Lorenz last_name: Zwick - first_name: Fabio full_name: Antonini, Fabio last_name: Antonini - first_name: Vishal full_name: Baibhav, Vishal last_name: Baibhav - first_name: Enrico full_name: Barausse, Enrico last_name: Barausse - first_name: Alexander full_name: Bonilla Rivera, Alexander last_name: Bonilla Rivera - first_name: Marica full_name: Branchesi, Marica last_name: Branchesi - first_name: Graziella full_name: Branduardi-Raymont, Graziella last_name: Branduardi-Raymont - first_name: Kevin full_name: Burdge, Kevin last_name: Burdge - first_name: Srija full_name: Chakraborty, Srija last_name: Chakraborty - first_name: Jorge full_name: Cuadra, Jorge last_name: Cuadra - first_name: Kristen full_name: Dage, Kristen last_name: Dage - first_name: Benjamin full_name: Davis, Benjamin last_name: Davis - first_name: Selma E. full_name: de Mink, Selma E. last_name: de Mink - first_name: Roberto full_name: Decarli, Roberto last_name: Decarli - first_name: Daniela full_name: Doneva, Daniela last_name: Doneva - first_name: Stephanie full_name: Escoffier, Stephanie last_name: Escoffier - first_name: Poshak full_name: Gandhi, Poshak last_name: Gandhi - first_name: Francesco full_name: Haardt, Francesco last_name: Haardt - first_name: Carlos O. full_name: Lousto, Carlos O. last_name: Lousto - first_name: Samaya full_name: Nissanke, Samaya last_name: Nissanke - first_name: Jason full_name: Nordhaus, Jason last_name: Nordhaus - first_name: Richard full_name: O’Shaughnessy, Richard last_name: O’Shaughnessy - first_name: Simon full_name: Portegies Zwart, Simon last_name: Portegies Zwart - first_name: Adam full_name: Pound, Adam last_name: Pound - first_name: Fabian full_name: Schussler, Fabian last_name: Schussler - first_name: Olga full_name: Sergijenko, Olga last_name: Sergijenko - first_name: Alessandro full_name: Spallicci, Alessandro last_name: Spallicci - first_name: Daniele full_name: Vernieri, Daniele last_name: Vernieri - first_name: Alejandro full_name: Vigna-Gómez, Alejandro last_name: Vigna-Gómez citation: ama: Amaro-Seoane P, Andrews J, Arca Sedda M, et al. Astrophysics with the laser interferometer space antenna. Living Reviews in Relativity. 2023;26(1). doi:10.1007/s41114-022-00041-y apa: Amaro-Seoane, P., Andrews, J., Arca Sedda, M., Askar, A., Baghi, Q., Balasov, R., … Vigna-Gómez, A. (2023). Astrophysics with the laser interferometer space antenna. Living Reviews in Relativity. Springer Science and Business Media LLC. https://doi.org/10.1007/s41114-022-00041-y chicago: Amaro-Seoane, Pau, Jeff Andrews, Manuel Arca Sedda, Abbas Askar, Quentin Baghi, Razvan Balasov, Imre Bartos, et al. “Astrophysics with the Laser Interferometer Space Antenna.” Living Reviews in Relativity. Springer Science and Business Media LLC, 2023. https://doi.org/10.1007/s41114-022-00041-y. ieee: P. Amaro-Seoane et al., “Astrophysics with the laser interferometer space antenna,” Living Reviews in Relativity, vol. 26, no. 1. Springer Science and Business Media LLC, 2023. ista: Amaro-Seoane P et al. 2023. Astrophysics with the laser interferometer space antenna. Living Reviews in Relativity. 26(1), 2. mla: Amaro-Seoane, Pau, et al. “Astrophysics with the Laser Interferometer Space Antenna.” Living Reviews in Relativity, vol. 26, no. 1, 2, Springer Science and Business Media LLC, 2023, doi:10.1007/s41114-022-00041-y. short: P. Amaro-Seoane, J. Andrews, M. Arca Sedda, A. Askar, Q. Baghi, R. Balasov, I. Bartos, S.S. Bavera, J. Bellovary, C.P.L. Berry, E. Berti, S. Bianchi, L. Blecha, S. Blondin, T. Bogdanović, S. Boissier, M. Bonetti, S. Bonoli, E. Bortolas, K. Breivik, P.R. Capelo, L. Caramete, F. Cattorini, M. Charisi, S. Chaty, X. Chen, M. Chruślińska, A.J.K. Chua, R. Church, M. Colpi, D. D’Orazio, C. Danielski, M.B. Davies, P. Dayal, A. De Rosa, A. Derdzinski, K. Destounis, M. Dotti, I. Duţan, I. Dvorkin, G. Fabj, T. Foglizzo, S. Ford, J.-B. Fouvry, A. Franchini, T. Fragos, C. Fryer, M. Gaspari, D. Gerosa, L. Graziani, P. Groot, M. Habouzit, D. Haggard, Z. Haiman, W.-B. Han, A. Istrate, P.H. Johansson, F.M. Khan, T. Kimpson, K. Kokkotas, A. Kong, V. Korol, K. Kremer, T. Kupfer, A. Lamberts, S. Larson, M. Lau, D. Liu, N. Lloyd-Ronning, G. Lodato, A. Lupi, C.-P. Ma, T. Maccarone, I. Mandel, A. Mangiagli, M. Mapelli, S. Mathis, L. Mayer, S. McGee, B. McKernan, M.C. Miller, D.F. Mota, M. Mumpower, S.S. Nasim, G. Nelemans, S. Noble, F. Pacucci, F. Panessa, V. Paschalidis, H. Pfister, D. Porquet, J. Quenby, A. Ricarte, F.K. Röpke, J. Regan, S. Rosswog, A. Ruiter, M. Ruiz, J. Runnoe, R. Schneider, J. Schnittman, A. Secunda, A. Sesana, N. Seto, L. Shao, S. Shapiro, C. Sopuerta, N.C. Stone, A. Suvorov, N. Tamanini, T. Tamfal, T. Tauris, K. Temmink, J. Tomsick, S. Toonen, A. Torres-Orjuela, M. Toscani, A. Tsokaros, C. Unal, V. Vázquez-Aceves, R. Valiante, M. van Putten, J. van Roestel, C. Vignali, M. Volonteri, K. Wu, Z. Younsi, S. Yu, S. Zane, L. Zwick, F. Antonini, V. Baibhav, E. Barausse, A. Bonilla Rivera, M. Branchesi, G. Branduardi-Raymont, K. Burdge, S. Chakraborty, J. Cuadra, K. Dage, B. Davis, S.E. de Mink, R. Decarli, D. Doneva, S. Escoffier, P. Gandhi, F. Haardt, C.O. Lousto, S. Nissanke, J. Nordhaus, R. O’Shaughnessy, S. Portegies Zwart, A. Pound, F. Schussler, O. Sergijenko, A. Spallicci, D. Vernieri, A. Vigna-Gómez, Living Reviews in Relativity 26 (2023). date_created: 2024-09-05T12:16:33Z date_published: 2023-03-14T00:00:00Z date_updated: 2024-09-19T07:31:45Z day: '14' doi: 10.1007/s41114-022-00041-y extern: '1' intvolume: ' 26' issue: '1' language: - iso: eng main_file_link: - open_access: '1' url: https://doi.org/10.1007/s41114-022-00041-y month: '03' oa: 1 oa_version: Published Version publication: Living Reviews in Relativity publication_identifier: issn: - 1433-8351 publication_status: published publisher: Springer Science and Business Media LLC quality_controlled: '1' scopus_import: '1' status: public title: Astrophysics with the laser interferometer space antenna type: journal_article user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345 volume: 26 year: '2023' ... --- _id: '17584' abstract: - lang: eng text: Some Seyfert galaxies are detected in high-energy gamma rays, but the mechanism and site of gamma-ray emission are unknown. Also, the origins of the cosmic high-energy neutrino and MeV gamma-ray backgrounds have been veiled in mystery since their discoveries. We propose emission from stellar-mass BHs (sBHs) embedded in disks of active galactic nuclei as their possible sources. These sBHs are predicted to launch jets due to the Blandford–Znajek mechanism, which can produce intense electromagnetic, neutrino, and cosmic-ray emissions. We investigate whether these emissions can be the sources of cosmic high-energy particles. We find that emission from internal shocks in the jets can explain gamma rays from nearby radio-quiet Seyfert galaxies including NGC 1068, if the Lorentz factor of the jets (Γj) is high. On the other hand, for moderate Γj, the emission can significantly contribute to the background gamma-ray and neutrino intensities in the ~MeV and ≲PeV bands, respectively. Furthermore, for moderate Γj with efficient amplification of the magnetic field and cosmic-ray acceleration, the neutrino emission from NGC 1068 and the ultrahigh-energy cosmic rays can be explained. These results suggest that the neutrino flux from NGC 1068 as well as the background intensities of MeV gamma rays, neutrinos, and the ultrahigh-energy cosmic rays can be explained by a unified model. Future MeV gamma-ray satellites will test our scenario for neutrino emission. article_number: '23' article_processing_charge: No article_type: original author: - first_name: Hiromichi full_name: Tagawa, Hiromichi last_name: Tagawa - first_name: Shigeo S. full_name: Kimura, Shigeo S. last_name: Kimura - first_name: Zoltán full_name: Haiman, Zoltán id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36 last_name: Haiman citation: ama: Tagawa H, Kimura SS, Haiman Z. High-energy electromagnetic, neutrino, and cosmic-ray emission by stellar-mass black holes in disks of active galactic nuclei. The Astrophysical Journal. 2023;955(1). doi:10.3847/1538-4357/ace71d apa: Tagawa, H., Kimura, S. S., & Haiman, Z. (2023). High-energy electromagnetic, neutrino, and cosmic-ray emission by stellar-mass black holes in disks of active galactic nuclei. The Astrophysical Journal. American Astronomical Society. https://doi.org/10.3847/1538-4357/ace71d chicago: Tagawa, Hiromichi, Shigeo S. Kimura, and Zoltán Haiman. “High-Energy Electromagnetic, Neutrino, and Cosmic-Ray Emission by Stellar-Mass Black Holes in Disks of Active Galactic Nuclei.” The Astrophysical Journal. American Astronomical Society, 2023. https://doi.org/10.3847/1538-4357/ace71d. ieee: H. Tagawa, S. S. Kimura, and Z. Haiman, “High-energy electromagnetic, neutrino, and cosmic-ray emission by stellar-mass black holes in disks of active galactic nuclei,” The Astrophysical Journal, vol. 955, no. 1. American Astronomical Society, 2023. ista: Tagawa H, Kimura SS, Haiman Z. 2023. High-energy electromagnetic, neutrino, and cosmic-ray emission by stellar-mass black holes in disks of active galactic nuclei. The Astrophysical Journal. 955(1), 23. mla: Tagawa, Hiromichi, et al. “High-Energy Electromagnetic, Neutrino, and Cosmic-Ray Emission by Stellar-Mass Black Holes in Disks of Active Galactic Nuclei.” The Astrophysical Journal, vol. 955, no. 1, 23, American Astronomical Society, 2023, doi:10.3847/1538-4357/ace71d. short: H. Tagawa, S.S. Kimura, Z. Haiman, The Astrophysical Journal 955 (2023). date_created: 2024-09-05T12:28:06Z date_published: 2023-09-12T00:00:00Z date_updated: 2024-09-19T11:45:10Z day: '12' doi: 10.3847/1538-4357/ace71d extern: '1' intvolume: ' 955' issue: '1' language: - iso: eng main_file_link: - open_access: '1' url: https://doi.org/10.3847/1538-4357/ace71d month: '09' oa: 1 oa_version: Published Version publication: The Astrophysical Journal publication_identifier: issn: - 0004-637X - 1538-4357 publication_status: published publisher: American Astronomical Society quality_controlled: '1' scopus_import: '1' status: public title: High-energy electromagnetic, neutrino, and cosmic-ray emission by stellar-mass black holes in disks of active galactic nuclei type: journal_article user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345 volume: 955 year: '2023' ... --- _id: '17594' abstract: - lang: eng text: The origin of stellar-mass black hole mergers discovered through gravitational waves is being widely debated. Mergers in the disks of active galactic nuclei (AGNs) represent a promising source of origin, with possible observational clues in the gravitational-wave data. Beyond gravitational waves, a unique signature of AGN-assisted mergers is electromagnetic emission from the accreting black holes. Here we show that jets launched by accreting black holes merging in an AGN disk can be detected as peculiar transients by infrared, optical, and X-ray observatories. We further show that this emission mechanism can explain the possible associations between gravitational-wave events and the optical transient ZTF 19abanrhr and the proposed gamma-ray counterparts GW150914-GBM and LVT151012-GBM. We demonstrate how these associations, if genuine, can be used to reconstruct the properties of these events’ environments. Searching for infrared and X-ray counterparts to similar electromagnetic transients in the future, once host galaxies are localized by optical observations, could provide a smoking-gun signature of the mergers’ AGN origin. article_number: '13' article_processing_charge: No article_type: original author: - first_name: Hiromichi full_name: Tagawa, Hiromichi last_name: Tagawa - first_name: Shigeo S. full_name: Kimura, Shigeo S. last_name: Kimura - first_name: Zoltán full_name: Haiman, Zoltán id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36 last_name: Haiman - first_name: Rosalba full_name: Perna, Rosalba last_name: Perna - first_name: Imre full_name: Bartos, Imre last_name: Bartos citation: ama: Tagawa H, Kimura SS, Haiman Z, Perna R, Bartos I. Observable signature of merging stellar-mass black holes in active galactic nuclei. The Astrophysical Journal. 2023;950(1). doi:10.3847/1538-4357/acc4bb apa: Tagawa, H., Kimura, S. S., Haiman, Z., Perna, R., & Bartos, I. (2023). Observable signature of merging stellar-mass black holes in active galactic nuclei. The Astrophysical Journal. American Astronomical Society. https://doi.org/10.3847/1538-4357/acc4bb chicago: Tagawa, Hiromichi, Shigeo S. Kimura, Zoltán Haiman, Rosalba Perna, and Imre Bartos. “Observable Signature of Merging Stellar-Mass Black Holes in Active Galactic Nuclei.” The Astrophysical Journal. American Astronomical Society, 2023. https://doi.org/10.3847/1538-4357/acc4bb. ieee: H. Tagawa, S. S. Kimura, Z. Haiman, R. Perna, and I. Bartos, “Observable signature of merging stellar-mass black holes in active galactic nuclei,” The Astrophysical Journal, vol. 950, no. 1. American Astronomical Society, 2023. ista: Tagawa H, Kimura SS, Haiman Z, Perna R, Bartos I. 2023. Observable signature of merging stellar-mass black holes in active galactic nuclei. The Astrophysical Journal. 950(1), 13. mla: Tagawa, Hiromichi, et al. “Observable Signature of Merging Stellar-Mass Black Holes in Active Galactic Nuclei.” The Astrophysical Journal, vol. 950, no. 1, 13, American Astronomical Society, 2023, doi:10.3847/1538-4357/acc4bb. short: H. Tagawa, S.S. Kimura, Z. Haiman, R. Perna, I. Bartos, The Astrophysical Journal 950 (2023). date_created: 2024-09-05T12:41:47Z date_published: 2023-06-06T00:00:00Z date_updated: 2024-09-23T12:36:58Z day: '06' doi: 10.3847/1538-4357/acc4bb extern: '1' intvolume: ' 950' issue: '1' language: - iso: eng main_file_link: - open_access: '1' url: https://doi.org/10.3847/1538-4357/acc4bb month: '06' oa: 1 oa_version: Published Version publication: The Astrophysical Journal publication_identifier: issn: - 0004-637X - 1538-4357 publication_status: published publisher: American Astronomical Society quality_controlled: '1' scopus_import: '1' status: public title: Observable signature of merging stellar-mass black holes in active galactic nuclei type: journal_article user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345 volume: 950 year: '2023' ... --- _id: '17602' abstract: - lang: eng text: Motivated by the increasing number of detections of merging black holes by LIGO-VIRGO-KAGRA, black hole (BH) binary mergers in the discs of active galactic nuclei (AGNs) is investigated as a possible merger channel. In this pathway, BH encounters in the gas disc form mutually bound BH binary systems through interaction with the gas in the disc and subsequently inspiral through gravitational torques induced by the local gas. To determine the feasibility of this merger pathway, we present the first three-dimensional global hydrodynamic simulations of the formation and evolution of a stellar-mass BH binaries AGN discs with three different AGN disc masses and five different initial radial separations. These 15 simulations show binary capture of prograde and retrograde binaries can be successful in a range of disc densities including cases well below that of a standard radiatively efficient alpha disc, identifying that the majority of these captured binaries are then subsequently hardened by the surrounding gas. The eccentricity evolution depends strongly on the orbital rotation where prograde binaries are governed by gravitational torques form their circumbinary mini disc, with eccentricities being damped, while for retrograde binaries the eccentricities are excited to >∼ 0.9 by accretion torques. In two cases, retrograde binaries ultimately undergo a close periapsis passage which results in a merger via gravitational waves after only a few thousand binary orbits. Thus, the merger time-scale can be far shorter than the AGN disc lifetime. These simulations support an efficient AGN disc merger pathway for BHs. article_processing_charge: No article_type: original author: - first_name: Connar full_name: Rowan, Connar last_name: Rowan - first_name: Tjarda full_name: Boekholt, Tjarda last_name: Boekholt - first_name: Bence full_name: Kocsis, Bence last_name: Kocsis - first_name: Zoltán full_name: Haiman, Zoltán id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36 last_name: Haiman citation: ama: 'Rowan C, Boekholt T, Kocsis B, Haiman Z. Black hole binary formation in AGN discs: from isolation to merger. Monthly Notices of the Royal Astronomical Society. 2023;524(2):2770-2796. doi:10.1093/mnras/stad1926' apa: 'Rowan, C., Boekholt, T., Kocsis, B., & Haiman, Z. (2023). Black hole binary formation in AGN discs: from isolation to merger. Monthly Notices of the Royal Astronomical Society. Oxford University Press. https://doi.org/10.1093/mnras/stad1926' chicago: 'Rowan, Connar, Tjarda Boekholt, Bence Kocsis, and Zoltán Haiman. “Black Hole Binary Formation in AGN Discs: From Isolation to Merger.” Monthly Notices of the Royal Astronomical Society. Oxford University Press, 2023. https://doi.org/10.1093/mnras/stad1926.' ieee: 'C. Rowan, T. Boekholt, B. Kocsis, and Z. Haiman, “Black hole binary formation in AGN discs: from isolation to merger,” Monthly Notices of the Royal Astronomical Society, vol. 524, no. 2. Oxford University Press, pp. 2770–2796, 2023.' ista: 'Rowan C, Boekholt T, Kocsis B, Haiman Z. 2023. Black hole binary formation in AGN discs: from isolation to merger. Monthly Notices of the Royal Astronomical Society. 524(2), 2770–2796.' mla: 'Rowan, Connar, et al. “Black Hole Binary Formation in AGN Discs: From Isolation to Merger.” Monthly Notices of the Royal Astronomical Society, vol. 524, no. 2, Oxford University Press, 2023, pp. 2770–96, doi:10.1093/mnras/stad1926.' short: C. Rowan, T. Boekholt, B. Kocsis, Z. Haiman, Monthly Notices of the Royal Astronomical Society 524 (2023) 2770–2796. date_created: 2024-09-05T13:09:11Z date_published: 2023-07-03T00:00:00Z date_updated: 2024-09-23T13:42:19Z day: '03' doi: 10.1093/mnras/stad1926 extern: '1' intvolume: ' 524' issue: '2' language: - iso: eng main_file_link: - open_access: '1' url: https://doi.org/10.1093/mnras/stad1926 month: '07' oa: 1 oa_version: Published Version page: 2770-2796 publication: Monthly Notices of the Royal Astronomical Society publication_identifier: issn: - 0035-8711 - 1365-2966 publication_status: published publisher: Oxford University Press quality_controlled: '1' scopus_import: '1' status: public title: 'Black hole binary formation in AGN discs: from isolation to merger' type: journal_article user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345 volume: 524 year: '2023' ... --- _id: '17606' abstract: - lang: eng text: We present the first results from the JWST ASPIRE program (A SPectroscopic survey of biased halos In the Reionization Era). This program represents an imaging and spectroscopic survey of 25 reionization-era quasars and their environments by utilizing the unprecedented capabilities of NIRCam Wide Field Slitless Spectroscopy (WFSS) mode. ASPIRE will deliver the largest (∼280 arcmin^2) galaxy redshift survey at 3-4 μm among JWST Cycle-1 programs and provide extensive legacy values for studying the formation of the earliest supermassive black holes (SMBHs), the assembly of galaxies, early metal enrichment, and cosmic reionization. In this first ASPIRE paper, we report the discovery of a filamentary structure traced by the luminous quasar J0305-3150 and ten [OIII] emitters at z=6.6. This structure has a 3D galaxy overdensity of δgal=12.6 over 637 cMpc3, one of the most overdense structures known in the early universe, and could eventually evolve into a massive galaxy cluster. Together with existing VLT/MUSE and ALMA observations of this field, our JWST observations reveal that J0305-3150 traces a complex environment where both UV-bright and dusty galaxies are present, and indicate that the early evolution of galaxies around the quasar is not simultaneous. In addition, we discovered 31 [OIII] emitters in this field at other redshifts, 5.3The Astrophysical Journal Letters. 2023;951(1). doi:10.3847/2041-8213/accd6f' apa: 'Wang, F., Yang, J., Hennawi, J. F., Fan, X., Sun, F., Champagne, J. B., … Zou, S. (2023). A SPectroscopic survey of biased halos in the reionization era (ASPIRE): JWST reveals a filamentary structure around a z = 6.61 Quasar. The Astrophysical Journal Letters. American Astronomical Society. https://doi.org/10.3847/2041-8213/accd6f' chicago: 'Wang, Feige, Jinyi Yang, Joseph F. Hennawi, Xiaohui Fan, Fengwu Sun, Jaclyn B. Champagne, Tiago Costa, et al. “A SPectroscopic Survey of Biased Halos in the Reionization Era (ASPIRE): JWST Reveals a Filamentary Structure around a z = 6.61 Quasar.” The Astrophysical Journal Letters. American Astronomical Society, 2023. https://doi.org/10.3847/2041-8213/accd6f.' ieee: 'F. Wang et al., “A SPectroscopic survey of biased halos in the reionization era (ASPIRE): JWST reveals a filamentary structure around a z = 6.61 Quasar,” The Astrophysical Journal Letters, vol. 951, no. 1. American Astronomical Society, 2023.' ista: 'Wang F, Yang J, Hennawi JF, Fan X, Sun F, Champagne JB, Costa T, Habouzit M, Endsley R, Li Z, Lin X, Meyer RA, Schindler J, Wu Y, Bañados E, Barth AJ, Bhowmick AK, Bieri R, Blecha L, Bosman S, Cai Z, Colina L, Connor T, Davies FB, Decarli R, De Rosa G, Drake AB, Egami E, Eilers A-C, Evans AE, Farina EP, Haiman Z, Jiang L, Jin X, Jun HD, Kakiichi K, Khusanova Y, Kulkarni G, Li M, Liu W, Loiacono F, Lupi A, Mazzucchelli C, Onoue M, Pudoka MA, Rojas-Ruiz S, Shen Y, Strauss MA, Tee WL, Trakhtenbrot B, Trebitsch M, Venemans B, Volonteri M, Walter F, Xie Z-L, Yue M, Zhang H, Zhang H, Zou S. 2023. A SPectroscopic survey of biased halos in the reionization era (ASPIRE): JWST reveals a filamentary structure around a z = 6.61 Quasar. The Astrophysical Journal Letters. 951(1), L4.' mla: 'Wang, Feige, et al. “A SPectroscopic Survey of Biased Halos in the Reionization Era (ASPIRE): JWST Reveals a Filamentary Structure around a z = 6.61 Quasar.” The Astrophysical Journal Letters, vol. 951, no. 1, L4, American Astronomical Society, 2023, doi:10.3847/2041-8213/accd6f.' short: F. Wang, J. Yang, J.F. Hennawi, X. Fan, F. Sun, J.B. Champagne, T. Costa, M. Habouzit, R. Endsley, Z. Li, X. Lin, R.A. Meyer, J. Schindler, Y. Wu, E. Bañados, A.J. Barth, A.K. Bhowmick, R. Bieri, L. Blecha, S. Bosman, Z. Cai, L. Colina, T. Connor, F.B. Davies, R. Decarli, G. De Rosa, A.B. Drake, E. Egami, A.-C. Eilers, A.E. Evans, E.P. Farina, Z. Haiman, L. Jiang, X. Jin, H.D. Jun, K. Kakiichi, Y. Khusanova, G. Kulkarni, M. Li, W. Liu, F. Loiacono, A. Lupi, C. Mazzucchelli, M. Onoue, M.A. Pudoka, S. Rojas-Ruiz, Y. Shen, M.A. Strauss, W.L. Tee, B. Trakhtenbrot, M. Trebitsch, B. Venemans, M. Volonteri, F. Walter, Z.-L. Xie, M. Yue, H. Zhang, H. Zhang, S. Zou, The Astrophysical Journal Letters 951 (2023). date_created: 2024-09-05T13:14:46Z date_published: 2023-06-29T00:00:00Z date_updated: 2024-09-23T14:08:58Z day: '29' doi: 10.3847/2041-8213/accd6f extern: '1' intvolume: ' 951' issue: '1' language: - iso: eng main_file_link: - open_access: '1' url: https://doi.org/10.3847/2041-8213/accd6f month: '06' oa: 1 oa_version: Published Version publication: The Astrophysical Journal Letters publication_identifier: issn: - 2041-8205 - 2041-8213 publication_status: published publisher: American Astronomical Society quality_controlled: '1' scopus_import: '1' status: public title: 'A SPectroscopic survey of biased halos in the reionization era (ASPIRE): JWST reveals a filamentary structure around a z = 6.61 Quasar' type: journal_article user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345 volume: 951 year: '2023' ... --- _id: '17611' abstract: - lang: eng text: The project MOMO (Multiwavelength Observations and Modelling of OJ 287) was set up to test predictions of binary supermassive black hole (SMBH) scenarios and to understand disc–jet physics of the blazar OJ 287. After a correction, the precessing binary (PB) SMBH model predicted the next main outburst of OJ 287 in 2022 October, making the outburst well observable and the model testable. We have densely covered this period in our ongoing multifrequency radio, optical, ultraviolet (UV), and X-ray monitoring. The predicted outburst was not detected. Instead, OJ 287 was at low optical–UV emission levels, declining further into November. The predicted thermal bremsstrahlung spectrum was not observed either, at any epoch. Further, applying scaling relations, we estimate an SMBH mass of OJ 287 of 108 M⊙. The latest in a sequence of deep low states that recur every 1–2 yr is used to determine an upper limit on the Eddington ratio and on the accretion-disc luminosity. This limit is at least a factor of 10 lower than required by the PB model with its massive primary SMBH of >1010 M⊙. All these results favour alternative binary SMBH models of OJ 287 that require neither strong orbital precession nor a very large mass of the primary SMBH. article_processing_charge: No article_type: original author: - first_name: S full_name: Komossa, S last_name: Komossa - first_name: D full_name: Grupe, D last_name: Grupe - first_name: A full_name: Kraus, A last_name: Kraus - first_name: M A full_name: Gurwell, M A last_name: Gurwell - first_name: Zoltán full_name: Haiman, Zoltán id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36 last_name: Haiman - first_name: F K full_name: Liu, F K last_name: Liu - first_name: A full_name: Tchekhovskoy, A last_name: Tchekhovskoy - first_name: L C full_name: Gallo, L C last_name: Gallo - first_name: M full_name: Berton, M last_name: Berton - first_name: R full_name: Blandford, R last_name: Blandford - first_name: J L full_name: Gómez, J L last_name: Gómez - first_name: A G full_name: Gonzalez, A G last_name: Gonzalez citation: ama: 'Komossa S, Grupe D, Kraus A, et al. Absence of the predicted 2022 October outburst of OJ 287 and implications for binary SMBH scenarios. Monthly Notices of the Royal Astronomical Society: Letters. 2023;522(1):L84-L88. doi:10.1093/mnrasl/slad016' apa: 'Komossa, S., Grupe, D., Kraus, A., Gurwell, M. A., Haiman, Z., Liu, F. K., … Gonzalez, A. G. (2023). Absence of the predicted 2022 October outburst of OJ 287 and implications for binary SMBH scenarios. Monthly Notices of the Royal Astronomical Society: Letters. Oxford University Press. https://doi.org/10.1093/mnrasl/slad016' chicago: 'Komossa, S, D Grupe, A Kraus, M A Gurwell, Zoltán Haiman, F K Liu, A Tchekhovskoy, et al. “Absence of the Predicted 2022 October Outburst of OJ 287 and Implications for Binary SMBH Scenarios.” Monthly Notices of the Royal Astronomical Society: Letters. Oxford University Press, 2023. https://doi.org/10.1093/mnrasl/slad016.' ieee: 'S. Komossa et al., “Absence of the predicted 2022 October outburst of OJ 287 and implications for binary SMBH scenarios,” Monthly Notices of the Royal Astronomical Society: Letters, vol. 522, no. 1. Oxford University Press, pp. L84–L88, 2023.' ista: 'Komossa S, Grupe D, Kraus A, Gurwell MA, Haiman Z, Liu FK, Tchekhovskoy A, Gallo LC, Berton M, Blandford R, Gómez JL, Gonzalez AG. 2023. Absence of the predicted 2022 October outburst of OJ 287 and implications for binary SMBH scenarios. Monthly Notices of the Royal Astronomical Society: Letters. 522(1), L84–L88.' mla: 'Komossa, S., et al. “Absence of the Predicted 2022 October Outburst of OJ 287 and Implications for Binary SMBH Scenarios.” Monthly Notices of the Royal Astronomical Society: Letters, vol. 522, no. 1, Oxford University Press, 2023, pp. L84–88, doi:10.1093/mnrasl/slad016.' short: 'S. Komossa, D. Grupe, A. Kraus, M.A. Gurwell, Z. Haiman, F.K. Liu, A. Tchekhovskoy, L.C. Gallo, M. Berton, R. Blandford, J.L. Gómez, A.G. Gonzalez, Monthly Notices of the Royal Astronomical Society: Letters 522 (2023) L84–L88.' date_created: 2024-09-05T13:23:29Z date_published: 2023-02-23T00:00:00Z date_updated: 2024-09-24T07:22:28Z day: '23' doi: 10.1093/mnrasl/slad016 extern: '1' intvolume: ' 522' issue: '1' language: - iso: eng main_file_link: - open_access: '1' url: https://doi.org/10.1093/mnrasl/slad016 month: '02' oa: 1 oa_version: Published Version page: L84-L88 publication: 'Monthly Notices of the Royal Astronomical Society: Letters' publication_identifier: issn: - 1745-3925 - 1745-3933 publication_status: published publisher: Oxford University Press quality_controlled: '1' scopus_import: '1' status: public title: Absence of the predicted 2022 October outburst of OJ 287 and implications for binary SMBH scenarios type: journal_article user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345 volume: 522 year: '2023' ... --- OA_type: closed access _id: '17860' abstract: - lang: eng text: Radicals are unique molecular systems for applications in electronic devices due to their open-shell electronic structures. Radicals can function as good electrical conductors and switches in molecular circuits while also holding great promise in the field of molecular spintronics. However, it is both challenging to create stable, persistent radicals and to understand their properties in molecular junctions. The goal of this Perspective is to address this dual challenge by providing design principles for the synthesis of stable radicals relevant to molecular junctions, as well as offering current insight into the electronic properties of radicals in single-molecule devices. By exploring both the chemical and physical properties of established radical systems, we will facilitate increased exploration and development of radical-based molecular systems. article_processing_charge: No article_type: original author: - first_name: Liang full_name: Li, Liang last_name: Li - first_name: Claudia R. full_name: Prindle, Claudia R. last_name: Prindle - first_name: Wanzhuo full_name: Shi, Wanzhuo last_name: Shi - first_name: Colin full_name: Nuckolls, Colin last_name: Nuckolls - first_name: Latha full_name: Venkataraman, Latha id: 9ebb78a5-cc0d-11ee-8322-fae086a32caf last_name: Venkataraman orcid: 0000-0002-6957-6089 citation: ama: Li L, Prindle CR, Shi W, Nuckolls C, Venkataraman L. Radical single-molecule junctions. Journal of the American Chemical Society. 2023;145(33):18182-18204. doi:10.1021/jacs.3c04487 apa: Li, L., Prindle, C. R., Shi, W., Nuckolls, C., & Venkataraman, L. (2023). Radical single-molecule junctions. Journal of the American Chemical Society. American Chemical Society. https://doi.org/10.1021/jacs.3c04487 chicago: Li, Liang, Claudia R. Prindle, Wanzhuo Shi, Colin Nuckolls, and Latha Venkataraman. “Radical Single-Molecule Junctions.” Journal of the American Chemical Society. American Chemical Society, 2023. https://doi.org/10.1021/jacs.3c04487. ieee: L. Li, C. R. Prindle, W. Shi, C. Nuckolls, and L. Venkataraman, “Radical single-molecule junctions,” Journal of the American Chemical Society, vol. 145, no. 33. American Chemical Society, pp. 18182–18204, 2023. ista: Li L, Prindle CR, Shi W, Nuckolls C, Venkataraman L. 2023. Radical single-molecule junctions. Journal of the American Chemical Society. 145(33), 18182–18204. mla: Li, Liang, et al. “Radical Single-Molecule Junctions.” Journal of the American Chemical Society, vol. 145, no. 33, American Chemical Society, 2023, pp. 18182–204, doi:10.1021/jacs.3c04487. short: L. Li, C.R. Prindle, W. Shi, C. Nuckolls, L. Venkataraman, Journal of the American Chemical Society 145 (2023) 18182–18204. date_created: 2024-09-06T12:49:27Z date_published: 2023-09-23T00:00:00Z date_updated: 2025-12-10T12:29:11Z day: '23' doi: 10.1021/jacs.3c04487 extern: '1' external_id: pmid: - '37555594' intvolume: ' 145' issue: '33' language: - iso: eng month: '09' oa_version: None page: 18182-18204 pmid: 1 publication: Journal of the American Chemical Society publication_identifier: eissn: - 1520-5126 issn: - 0002-7863 publication_status: published publisher: American Chemical Society quality_controlled: '1' scopus_import: '1' status: public title: Radical single-molecule junctions type: journal_article user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 volume: 145 year: '2023' ... --- OA_type: closed access _id: '17861' abstract: - lang: eng text: 'Molecular one-dimensional topological insulators (1D TIs), described by the Su-Schrieffer-Heeger (SSH) model, are a new class of molecular electronic wires whose low-energy topological edge states endow them with high electrical conductivity. However, when these 1D TIs become long, the high conductance is not sustained because the coupling between the edge states decreases with increasing length. Here, we present a new design where we connect multiple short 1D SSH TI units linearly or in a cycle to create molecular wires with a continuous topological state density. Using a tight-binding method, we show that the linear system gives a length-independent conductance. The cyclic systems show an interesting odd-even effect, with unit transmission in the topological limit, but zero transmission in the trivial limit. Furthermore, based on our calculations, we predict that these systems can support resonant transmission with a quantum of conductance. We can further expand these results to phenylene-based linear and cyclic 1D TI systems and confirm the length-dependent conductance in such systems. ' article_processing_charge: No article_type: original author: - first_name: Liang full_name: Li, Liang last_name: Li - first_name: Colin full_name: Nuckolls, Colin last_name: Nuckolls - first_name: Latha full_name: Venkataraman, Latha id: 9ebb78a5-cc0d-11ee-8322-fae086a32caf last_name: Venkataraman orcid: 0000-0002-6957-6089 citation: ama: Li L, Nuckolls C, Venkataraman L. Designing long and highly conducting molecular wires with multiple nontrivial topological states. The Journal of Physical Chemistry Letters. 2023;14(22):5141-5147. doi:10.1021/acs.jpclett.3c01081 apa: Li, L., Nuckolls, C., & Venkataraman, L. (2023). Designing long and highly conducting molecular wires with multiple nontrivial topological states. The Journal of Physical Chemistry Letters. American Chemical Society. https://doi.org/10.1021/acs.jpclett.3c01081 chicago: Li, Liang, Colin Nuckolls, and Latha Venkataraman. “Designing Long and Highly Conducting Molecular Wires with Multiple Nontrivial Topological States.” The Journal of Physical Chemistry Letters. American Chemical Society, 2023. https://doi.org/10.1021/acs.jpclett.3c01081. ieee: L. Li, C. Nuckolls, and L. Venkataraman, “Designing long and highly conducting molecular wires with multiple nontrivial topological states,” The Journal of Physical Chemistry Letters, vol. 14, no. 22. American Chemical Society, pp. 5141–5147, 2023. ista: Li L, Nuckolls C, Venkataraman L. 2023. Designing long and highly conducting molecular wires with multiple nontrivial topological states. The Journal of Physical Chemistry Letters. 14(22), 5141–5147. mla: Li, Liang, et al. “Designing Long and Highly Conducting Molecular Wires with Multiple Nontrivial Topological States.” The Journal of Physical Chemistry Letters, vol. 14, no. 22, American Chemical Society, 2023, pp. 5141–47, doi:10.1021/acs.jpclett.3c01081. short: L. Li, C. Nuckolls, L. Venkataraman, The Journal of Physical Chemistry Letters 14 (2023) 5141–5147. date_created: 2024-09-06T12:50:23Z date_published: 2023-05-30T00:00:00Z date_updated: 2025-01-03T11:36:41Z day: '30' doi: 10.1021/acs.jpclett.3c01081 extern: '1' external_id: pmid: - '37252687' intvolume: ' 14' issue: '22' language: - iso: eng month: '05' oa_version: None page: 5141-5147 pmid: 1 publication: The Journal of Physical Chemistry Letters publication_identifier: eissn: - 1948-7185 publication_status: published publisher: American Chemical Society quality_controlled: '1' scopus_import: '1' status: public title: Designing long and highly conducting molecular wires with multiple nontrivial topological states type: journal_article user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 volume: 14 year: '2023' ... --- _id: '17862' abstract: - lang: eng text: Electric field acceleration of alkyl hydroperoxide activation to acylate amines in the scanning tunneling microscope-based break-junction is reported. Alkyl hydroperoxide mixtures, generated from hydrocarbon autoxidation in air, were found to be competent reagents for the functionalization of gold surfaces. Intermolecular coupling on the surface in the presence of amines was observed, yielding normal alkylamides. This novel mode of alkyl hydroperoxide activation to generate acylium equivalents was found to be responsive to the magnitude of the bias in the break junction, indicating an electric field influence on this novel reactivity. article_processing_charge: No article_type: original author: - first_name: Xiye full_name: Wang, Xiye last_name: Wang - first_name: Boyuan full_name: Zhang, Boyuan last_name: Zhang - first_name: Brandon full_name: Fowler, Brandon last_name: Fowler - first_name: Latha full_name: Venkataraman, Latha id: 9ebb78a5-cc0d-11ee-8322-fae086a32caf last_name: Venkataraman orcid: 0000-0002-6957-6089 - first_name: Tomislav full_name: Rovis, Tomislav last_name: Rovis citation: ama: Wang X, Zhang B, Fowler B, Venkataraman L, Rovis T. Alkane solvent-derived acylation reaction driven by electric fields. Journal of the American Chemical Society. 2023;145(22):11903-11906. doi:10.1021/jacs.3c02064 apa: Wang, X., Zhang, B., Fowler, B., Venkataraman, L., & Rovis, T. (2023). Alkane solvent-derived acylation reaction driven by electric fields. Journal of the American Chemical Society. American Chemical Society. https://doi.org/10.1021/jacs.3c02064 chicago: Wang, Xiye, Boyuan Zhang, Brandon Fowler, Latha Venkataraman, and Tomislav Rovis. “Alkane Solvent-Derived Acylation Reaction Driven by Electric Fields.” Journal of the American Chemical Society. American Chemical Society, 2023. https://doi.org/10.1021/jacs.3c02064. ieee: X. Wang, B. Zhang, B. Fowler, L. Venkataraman, and T. Rovis, “Alkane solvent-derived acylation reaction driven by electric fields,” Journal of the American Chemical Society, vol. 145, no. 22. American Chemical Society, pp. 11903–11906, 2023. ista: Wang X, Zhang B, Fowler B, Venkataraman L, Rovis T. 2023. Alkane solvent-derived acylation reaction driven by electric fields. Journal of the American Chemical Society. 145(22), 11903–11906. mla: Wang, Xiye, et al. “Alkane Solvent-Derived Acylation Reaction Driven by Electric Fields.” Journal of the American Chemical Society, vol. 145, no. 22, American Chemical Society, 2023, pp. 11903–06, doi:10.1021/jacs.3c02064. short: X. Wang, B. Zhang, B. Fowler, L. Venkataraman, T. Rovis, Journal of the American Chemical Society 145 (2023) 11903–11906. date_created: 2024-09-06T12:55:12Z date_published: 2023-05-25T00:00:00Z date_updated: 2024-11-25T12:29:49Z day: '25' doi: 10.1021/jacs.3c02064 extern: '1' external_id: pmid: - '37227235' intvolume: ' 145' issue: '22' language: - iso: eng month: '05' oa_version: None page: 11903-11906 pmid: 1 publication: Journal of the American Chemical Society publication_identifier: eissn: - 1520-5126 issn: - 0002-7863 publication_status: published publisher: American Chemical Society quality_controlled: '1' scopus_import: '1' status: public title: Alkane solvent-derived acylation reaction driven by electric fields type: journal_article user_id: 68b8ca59-c5b3-11ee-8790-cd641c68093d volume: 145 year: '2023' ... --- OA_place: publisher OA_type: gold _id: '17863' abstract: - lang: eng text: Understanding and tuning charge transport over a single molecule is a fundamental topic in molecular electronics. Single-molecule junctions composed of individual molecules attached to two electrodes are the most common components built for single-molecule charge transport studies. During the past two decades, rapid technical and theoretical advances in single-molecule junctions have increased our understanding of the conductance properties and functions of molecular devices. In this perspective article, we introduce the basic principles of charge transport in single-molecule junctions, then give an overview of recent progress in modulating single-molecule transport through external stimuli such as electric field and potential, light, mechanical force, heat, and chemical environment. Lastly, we discuss challenges and offer views on future developments in molecular electronics. article_number: '100115' article_processing_charge: No article_type: original author: - first_name: Qi full_name: Zou, Qi last_name: Zou - first_name: Jin full_name: Qiu, Jin last_name: Qiu - first_name: Yaping full_name: Zang, Yaping last_name: Zang - first_name: He full_name: Tian, He last_name: Tian - first_name: Latha full_name: Venkataraman, Latha id: 9ebb78a5-cc0d-11ee-8322-fae086a32caf last_name: Venkataraman orcid: 0000-0002-6957-6089 citation: ama: Zou Q, Qiu J, Zang Y, Tian H, Venkataraman L. Modulating single-molecule charge transport through external stimulus. eScience. 2023;3(3). doi:10.1016/j.esci.2023.100115 apa: Zou, Q., Qiu, J., Zang, Y., Tian, H., & Venkataraman, L. (2023). Modulating single-molecule charge transport through external stimulus. EScience. Elsevier BV. https://doi.org/10.1016/j.esci.2023.100115 chicago: Zou, Qi, Jin Qiu, Yaping Zang, He Tian, and Latha Venkataraman. “Modulating Single-Molecule Charge Transport through External Stimulus.” EScience. Elsevier BV, 2023. https://doi.org/10.1016/j.esci.2023.100115. ieee: Q. Zou, J. Qiu, Y. Zang, H. Tian, and L. Venkataraman, “Modulating single-molecule charge transport through external stimulus,” eScience, vol. 3, no. 3. Elsevier BV, 2023. ista: Zou Q, Qiu J, Zang Y, Tian H, Venkataraman L. 2023. Modulating single-molecule charge transport through external stimulus. eScience. 3(3), 100115. mla: Zou, Qi, et al. “Modulating Single-Molecule Charge Transport through External Stimulus.” EScience, vol. 3, no. 3, 100115, Elsevier BV, 2023, doi:10.1016/j.esci.2023.100115. short: Q. Zou, J. Qiu, Y. Zang, H. Tian, L. Venkataraman, EScience 3 (2023). date_created: 2024-09-06T12:56:54Z date_published: 2023-05-01T00:00:00Z date_updated: 2024-11-25T12:41:14Z doi: 10.1016/j.esci.2023.100115 extern: '1' intvolume: ' 3' issue: '3' language: - iso: eng main_file_link: - open_access: '1' url: https://www.sciencedirect.com/science/article/pii/S2667141723000332?via%3Dihub month: '05' oa: 1 oa_version: Published Version publication: eScience publication_identifier: eissn: - 2667-1417 publication_status: published publisher: Elsevier BV quality_controlled: '1' scopus_import: '1' status: public title: Modulating single-molecule charge transport through external stimulus type: journal_article user_id: 68b8ca59-c5b3-11ee-8790-cd641c68093d volume: 3 year: '2023' ... --- OA_type: closed access _id: '17864' abstract: - lang: eng text: 'Molecular one-dimensional topological insulators (1D TIs), which conduct through energetically low-lying topological edge states, can be extremely highly conducting and exhibit a reversed conductance decay, affording them great potential as building blocks for nanoelectronic devices. However, these properties can only be observed at the short length limit. To extend the length at which these anomalous effects can be observed, we design topological oligo[n]emeraldine wires using short 1D TIs as building blocks. As the wire length increases, the number of topological states increases, enabling an increased electronic transmission along the wire; specifically, we show that we can drive over a microampere current through a single ∼5 nm molecular wire, appreciably more than what has been observed in other long wires reported to date. Calculations and experiments show that the longest oligo[7]emeraldine with doped topological states has over 106 enhancements in the transmission compared to its pristine form. The discovery of these highly conductive, long organic wires helps overcome a fundamental hurdle to implementing molecules in complex, nanoscale circuitry: their structures become too insulating at lengths that are useful in designing nanoscale circuits.' article_processing_charge: No author: - first_name: Liang full_name: Li, Liang last_name: Li - first_name: Shayan full_name: Louie, Shayan last_name: Louie - first_name: Austin M. full_name: Evans, Austin M. last_name: Evans - first_name: Elena full_name: Meirzadeh, Elena last_name: Meirzadeh - first_name: Colin full_name: Nuckolls, Colin last_name: Nuckolls - first_name: Latha full_name: Venkataraman, Latha id: 9ebb78a5-cc0d-11ee-8322-fae086a32caf last_name: Venkataraman orcid: 0000-0002-6957-6089 citation: ama: Li L, Louie S, Evans AM, Meirzadeh E, Nuckolls C, Venkataraman L. Topological radical pairs produce ultrahigh conductance in long molecular wires. Journal of the American Chemical Society. 2023;145(4):2492-2498. doi:10.1021/jacs.2c12059 apa: Li, L., Louie, S., Evans, A. M., Meirzadeh, E., Nuckolls, C., & Venkataraman, L. (2023). Topological radical pairs produce ultrahigh conductance in long molecular wires. Journal of the American Chemical Society. American Chemical Society. https://doi.org/10.1021/jacs.2c12059 chicago: Li, Liang, Shayan Louie, Austin M. Evans, Elena Meirzadeh, Colin Nuckolls, and Latha Venkataraman. “Topological Radical Pairs Produce Ultrahigh Conductance in Long Molecular Wires.” Journal of the American Chemical Society. American Chemical Society, 2023. https://doi.org/10.1021/jacs.2c12059. ieee: L. Li, S. Louie, A. M. Evans, E. Meirzadeh, C. Nuckolls, and L. Venkataraman, “Topological radical pairs produce ultrahigh conductance in long molecular wires,” Journal of the American Chemical Society, vol. 145, no. 4. American Chemical Society, pp. 2492–2498, 2023. ista: Li L, Louie S, Evans AM, Meirzadeh E, Nuckolls C, Venkataraman L. 2023. Topological radical pairs produce ultrahigh conductance in long molecular wires. Journal of the American Chemical Society. 145(4), 2492–2498. mla: Li, Liang, et al. “Topological Radical Pairs Produce Ultrahigh Conductance in Long Molecular Wires.” Journal of the American Chemical Society, vol. 145, no. 4, American Chemical Society, 2023, pp. 2492–98, doi:10.1021/jacs.2c12059. short: L. Li, S. Louie, A.M. Evans, E. Meirzadeh, C. Nuckolls, L. Venkataraman, Journal of the American Chemical Society 145 (2023) 2492–2498. date_created: 2024-09-06T12:57:45Z date_published: 2023-01-23T00:00:00Z date_updated: 2024-11-25T14:21:10Z day: '23' doi: 10.1021/jacs.2c12059 extern: '1' external_id: pmid: - '36689781' intvolume: ' 145' issue: '4' language: - iso: eng month: '01' oa_version: None page: 2492-2498 pmid: 1 publication: Journal of the American Chemical Society publication_identifier: eissn: - 1520-5126 issn: - 0002-7863 publication_status: published publisher: American Chemical Society quality_controlled: '1' scopus_import: '1' status: public title: Topological radical pairs produce ultrahigh conductance in long molecular wires type: journal_article user_id: 68b8ca59-c5b3-11ee-8790-cd641c68093d volume: 145 year: '2023' ... --- OA_type: closed access _id: '17865' abstract: - lang: eng text: Understanding how molecular geometry affects the electronic properties of single-molecule junctions experimentally has been challenging. Typically, metal–molecule–metal junctions are measured using a break-junction method where electrode separation is mechanically evolving during measurement. Here, to probe the impact of the junction geometry on conductance, we apply a sinusoidal modulation to the molecular junction electrode position. Simultaneously, we probe the nonlinearity of the current–voltage characteristics of each junction through a modulation in the applied bias at a different frequency. In turn, we show that junctions formed with molecules that have different molecule–electrode interfaces exhibit statistically distinguishable Fourier-transformed conductances. In particular, we find a marked bias dependence for the modulation of junctions where transmission is mediated thorough the van der Waals (vdW) interaction. We attribute our findings to voltage-modulated vdW interactions at the single-molecule level. article_processing_charge: No article_type: original author: - first_name: Yujing full_name: Wei, Yujing last_name: Wei - first_name: Liang full_name: Li, Liang last_name: Li - first_name: Julia E. full_name: Greenwald, Julia E. last_name: Greenwald - first_name: Latha full_name: Venkataraman, Latha id: 9ebb78a5-cc0d-11ee-8322-fae086a32caf last_name: Venkataraman orcid: 0000-0002-6957-6089 citation: ama: Wei Y, Li L, Greenwald JE, Venkataraman L. Voltage-modulated van der waals interaction in single-molecule junctions. Nano Letters. 2023;23(2):567-572. doi:10.1021/acs.nanolett.2c04098 apa: Wei, Y., Li, L., Greenwald, J. E., & Venkataraman, L. (2023). Voltage-modulated van der waals interaction in single-molecule junctions. Nano Letters. American Chemical Society. https://doi.org/10.1021/acs.nanolett.2c04098 chicago: Wei, Yujing, Liang Li, Julia E. Greenwald, and Latha Venkataraman. “Voltage-Modulated van Der Waals Interaction in Single-Molecule Junctions.” Nano Letters. American Chemical Society, 2023. https://doi.org/10.1021/acs.nanolett.2c04098. ieee: Y. Wei, L. Li, J. E. Greenwald, and L. Venkataraman, “Voltage-modulated van der waals interaction in single-molecule junctions,” Nano Letters, vol. 23, no. 2. American Chemical Society, pp. 567–572, 2023. ista: Wei Y, Li L, Greenwald JE, Venkataraman L. 2023. Voltage-modulated van der waals interaction in single-molecule junctions. Nano Letters. 23(2), 567–572. mla: Wei, Yujing, et al. “Voltage-Modulated van Der Waals Interaction in Single-Molecule Junctions.” Nano Letters, vol. 23, no. 2, American Chemical Society, 2023, pp. 567–72, doi:10.1021/acs.nanolett.2c04098. short: Y. Wei, L. Li, J.E. Greenwald, L. Venkataraman, Nano Letters 23 (2023) 567–572. date_created: 2024-09-06T12:58:41Z date_published: 2023-01-05T00:00:00Z date_updated: 2024-11-25T14:49:19Z day: '05' doi: 10.1021/acs.nanolett.2c04098 extern: '1' external_id: pmid: - '36602221' intvolume: ' 23' issue: '2' language: - iso: eng month: '01' oa_version: None page: 567-572 pmid: 1 publication: Nano Letters publication_identifier: eissn: - 1530-6992 issn: - 1530-6984 publication_status: published publisher: American Chemical Society quality_controlled: '1' status: public title: Voltage-modulated van der waals interaction in single-molecule junctions type: journal_article user_id: 68b8ca59-c5b3-11ee-8790-cd641c68093d volume: 23 year: '2023' ... --- OA_place: publisher OA_type: gold _id: '17866' abstract: - lang: eng text: Electric fields have been used to control and direct chemical reactions in biochemistry and enzymatic catalysis, yet directly applying external electric fields to activate reactions in bulk solution and to characterize them ex situ remains a challenge. Here we utilize the scanning tunneling microscope-based break-junction technique to investigate the electric field driven homolytic cleavage of the radical initiator 4-(methylthio)benzoic peroxyanhydride at ambient temperatures in bulk solution, without the use of co-initiators or photochemical activators. Through time-dependent ex situ quantification by high performance liquid chromatography using a UV-vis detector, we find that the electric field catalyzes the reaction. Importantly, we demonstrate that the reaction rate in a field increases linearly with the solvent dielectric constant. Using density functional theory calculations, we show that the applied electric field decreases the dissociation energy of the O–O bond and stabilizes the product relative to the reactant due to their different dipole moments. article_processing_charge: Yes article_type: original author: - first_name: Boyuan full_name: Zhang, Boyuan last_name: Zhang - first_name: Cedric full_name: Schaack, Cedric last_name: Schaack - first_name: Claudia R. full_name: Prindle, Claudia R. last_name: Prindle - first_name: Ethan A. full_name: Vo, Ethan A. last_name: Vo - first_name: Miriam full_name: Aziz, Miriam last_name: Aziz - first_name: Michael L. full_name: Steigerwald, Michael L. last_name: Steigerwald - first_name: Timothy C. full_name: Berkelbach, Timothy C. last_name: Berkelbach - first_name: Colin full_name: Nuckolls, Colin last_name: Nuckolls - first_name: Latha full_name: Venkataraman, Latha id: 9ebb78a5-cc0d-11ee-8322-fae086a32caf last_name: Venkataraman orcid: 0000-0002-6957-6089 citation: ama: Zhang B, Schaack C, Prindle CR, et al. Electric fields drive bond homolysis. Chemical Science. 2023;14(7):1769-1774. doi:10.1039/d2sc06411a apa: Zhang, B., Schaack, C., Prindle, C. R., Vo, E. A., Aziz, M., Steigerwald, M. L., … Venkataraman, L. (2023). Electric fields drive bond homolysis. Chemical Science. Royal Society of Chemistry. https://doi.org/10.1039/d2sc06411a chicago: Zhang, Boyuan, Cedric Schaack, Claudia R. Prindle, Ethan A. Vo, Miriam Aziz, Michael L. Steigerwald, Timothy C. Berkelbach, Colin Nuckolls, and Latha Venkataraman. “Electric Fields Drive Bond Homolysis.” Chemical Science. Royal Society of Chemistry, 2023. https://doi.org/10.1039/d2sc06411a. ieee: B. Zhang et al., “Electric fields drive bond homolysis,” Chemical Science, vol. 14, no. 7. Royal Society of Chemistry, pp. 1769–1774, 2023. ista: Zhang B, Schaack C, Prindle CR, Vo EA, Aziz M, Steigerwald ML, Berkelbach TC, Nuckolls C, Venkataraman L. 2023. Electric fields drive bond homolysis. Chemical Science. 14(7), 1769–1774. mla: Zhang, Boyuan, et al. “Electric Fields Drive Bond Homolysis.” Chemical Science, vol. 14, no. 7, Royal Society of Chemistry, 2023, pp. 1769–74, doi:10.1039/d2sc06411a. short: B. Zhang, C. Schaack, C.R. Prindle, E.A. Vo, M. Aziz, M.L. Steigerwald, T.C. Berkelbach, C. Nuckolls, L. Venkataraman, Chemical Science 14 (2023) 1769–1774. date_created: 2024-09-06T12:59:45Z date_published: 2023-01-16T00:00:00Z date_updated: 2024-11-25T15:01:40Z day: '16' doi: 10.1039/d2sc06411a extern: '1' external_id: pmid: - '36819847' intvolume: ' 14' issue: '7' language: - iso: eng main_file_link: - open_access: '1' url: https://europepmc.org/article/pmc/pmc9931054 month: '01' oa: 1 oa_version: Published Version page: 1769-1774 pmid: 1 publication: Chemical Science publication_identifier: eissn: - 2041-6539 issn: - 2041-6520 publication_status: published publisher: Royal Society of Chemistry quality_controlled: '1' status: public title: Electric fields drive bond homolysis type: journal_article user_id: 68b8ca59-c5b3-11ee-8790-cd641c68093d volume: 14 year: '2023' ... --- _id: '18179' abstract: - lang: eng text: 'Linnik type problems concern the distribution of projections of integral points on the unit sphere as their norm increases, and different generalizations of this phenomenon. Our work addresses a question of this type: we prove the uniform distribution of the projections of primitive Z2 points in the p-adic unit sphere, as their (real) norm tends to infinity. The proof is via counting lattice points in semi-simple S-arithmetic groups.' - lang: fre text: 'Les problèmes de type Linnik concernent la distribution des projections des points entiers sur la sphère unitaire lorsque leur norme augmente et différentes généralisations de ce phénomène. Notre travail s’intéresse à une question de ce type : nous prouvons la distribution uniforme des projections des points primitifs de Z2 sur la sphère unitaire p-adique lorsque leur norme (réelle) tend vers l’infini. La preuve se fait en comptant les points d’un réseau dans des S-groupes arithmétiques semi-simples.' acknowledgement: The second author is supported by EPRSC grant EP/P026710/1. article_processing_charge: Yes (in subscription journal) article_type: original arxiv: 1 author: - first_name: Antonin full_name: Guilloux, Antonin last_name: Guilloux - first_name: Tal full_name: Horesh, Tal id: C8B7BF48-8D81-11E9-BCA9-F536E6697425 last_name: Horesh citation: ama: Guilloux A, Horesh T. p-adic directions of primitive vectors. Publications mathématiques de Besançon - Algèbre et Théorie des nombres. 2023;2023:85-107. doi:10.5802/pmb.50 apa: Guilloux, A., & Horesh, T. (2023). p-adic directions of primitive vectors. Publications Mathématiques de Besançon - Algèbre et Théorie Des Nombres. Presses Universitaires de Franche-Comté. https://doi.org/10.5802/pmb.50 chicago: Guilloux, Antonin, and Tal Horesh. “P-Adic Directions of Primitive Vectors.” Publications Mathématiques de Besançon - Algèbre et Théorie Des Nombres. Presses Universitaires de Franche-Comté, 2023. https://doi.org/10.5802/pmb.50. ieee: A. Guilloux and T. Horesh, “p-adic directions of primitive vectors,” Publications mathématiques de Besançon - Algèbre et Théorie des nombres, vol. 2023. Presses Universitaires de Franche-Comté, pp. 85–107, 2023. ista: Guilloux A, Horesh T. 2023. p-adic directions of primitive vectors. Publications mathématiques de Besançon - Algèbre et Théorie des nombres. 2023, 85–107. mla: Guilloux, Antonin, and Tal Horesh. “P-Adic Directions of Primitive Vectors.” Publications Mathématiques de Besançon - Algèbre et Théorie Des Nombres, vol. 2023, Presses Universitaires de Franche-Comté, 2023, pp. 85–107, doi:10.5802/pmb.50. short: A. Guilloux, T. Horesh, Publications Mathématiques de Besançon - Algèbre et Théorie Des Nombres 2023 (2023) 85–107. corr_author: '1' date_created: 2024-10-06T22:01:13Z date_published: 2023-06-15T00:00:00Z date_updated: 2025-04-14T09:25:44Z day: '15' ddc: - '510' department: - _id: TiBr doi: 10.5802/pmb.50 external_id: arxiv: - '2103.10889' file: - access_level: open_access checksum: cefc47a2cf55a87f8e4960197f73353b content_type: application/pdf creator: dernst date_created: 2024-10-07T11:32:32Z date_updated: 2024-10-07T11:32:32Z file_id: '18186' file_name: 2023_MathBesancon_Guilloux.pdf file_size: 1399390 relation: main_file success: 1 file_date_updated: 2024-10-07T11:32:32Z has_accepted_license: '1' intvolume: ' 2023' language: - iso: eng month: '06' oa: 1 oa_version: Published Version page: 85-107 project: - _id: 26A8D266-B435-11E9-9278-68D0E5697425 grant_number: EP-P026710-2 name: Between rational and integral points publication: Publications mathématiques de Besançon - Algèbre et Théorie des nombres publication_identifier: eissn: - 2592-6616 issn: - 2804-8504 publication_status: published publisher: Presses Universitaires de Franche-Comté quality_controlled: '1' scopus_import: '1' status: public title: p-adic directions of primitive vectors tmp: image: /image/cc_by_nd.png legal_code_url: https://creativecommons.org/licenses/by-nd/4.0/legalcode name: Creative Commons Attribution-NoDerivatives 4.0 International (CC BY-ND 4.0) short: CC BY-ND (4.0) type: journal_article user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 volume: 2023 year: '2023' ... --- _id: '18189' abstract: - lang: eng text: 'Strongly interacting topological matter1 exhibits fundamentally new phenomena with potential applications in quantum information technology2,3. Emblematic instances are fractional quantum Hall (FQH) states4, in which the interplay of a magnetic field and strong interactions gives rise to fractionally charged quasi-particles, long-ranged entanglement and anyonic exchange statistics. Progress in engineering synthetic magnetic fields5,6,7,8,9,10,11,12,13,14,15,16,17,18,19,20,21 has raised the hope to create these exotic states in controlled quantum systems. However, except for a recent Laughlin state of light22, preparing FQH states in engineered systems remains elusive. Here we realize a FQH state with ultracold atoms in an optical lattice. The state is a lattice version of a bosonic ν = 1/2 Laughlin state4,23 with two particles on 16 sites. This minimal system already captures many hallmark features of Laughlin-type FQH states24,25,26,27,28: we observe a suppression of two-body interactions, we find a distinctive vortex structure in the density correlations and we measure a fractional Hall conductivity of σH/σ0 = 0.6(2) by means of the bulk response to a magnetic perturbation. Furthermore, by tuning the magnetic field, we map out the transition point between the normal and the FQH regime through a spectroscopic investigation of the many-body gap. Our work provides a starting point for exploring highly entangled topological matter with ultracold atoms29,30,31,32,33.' article_processing_charge: No article_type: original arxiv: 1 author: - first_name: Julian full_name: Leonard, Julian id: b75b3f45-7995-11ef-9bfd-9a9cd02c3577 last_name: Leonard - first_name: Sooshin full_name: Kim, Sooshin last_name: Kim - first_name: Joyce full_name: Kwan, Joyce last_name: Kwan - first_name: Perrin full_name: Segura, Perrin last_name: Segura - first_name: Fabian full_name: Grusdt, Fabian last_name: Grusdt - first_name: Cécile full_name: Repellin, Cécile last_name: Repellin - first_name: Nathan full_name: Goldman, Nathan last_name: Goldman - first_name: Markus full_name: Greiner, Markus last_name: Greiner citation: ama: Leonard J, Kim S, Kwan J, et al. Realization of a fractional quantum Hall state with ultracold atoms. Nature. 2023;619(7970):495-499. doi:10.1038/s41586-023-06122-4 apa: Leonard, J., Kim, S., Kwan, J., Segura, P., Grusdt, F., Repellin, C., … Greiner, M. (2023). Realization of a fractional quantum Hall state with ultracold atoms. Nature. Springer Nature. https://doi.org/10.1038/s41586-023-06122-4 chicago: Leonard, Julian, Sooshin Kim, Joyce Kwan, Perrin Segura, Fabian Grusdt, Cécile Repellin, Nathan Goldman, and Markus Greiner. “Realization of a Fractional Quantum Hall State with Ultracold Atoms.” Nature. Springer Nature, 2023. https://doi.org/10.1038/s41586-023-06122-4. ieee: J. Leonard et al., “Realization of a fractional quantum Hall state with ultracold atoms,” Nature, vol. 619, no. 7970. Springer Nature, pp. 495–499, 2023. ista: Leonard J, Kim S, Kwan J, Segura P, Grusdt F, Repellin C, Goldman N, Greiner M. 2023. Realization of a fractional quantum Hall state with ultracold atoms. Nature. 619(7970), 495–499. mla: Leonard, Julian, et al. “Realization of a Fractional Quantum Hall State with Ultracold Atoms.” Nature, vol. 619, no. 7970, Springer Nature, 2023, pp. 495–99, doi:10.1038/s41586-023-06122-4. short: J. Leonard, S. Kim, J. Kwan, P. Segura, F. Grusdt, C. Repellin, N. Goldman, M. Greiner, Nature 619 (2023) 495–499. date_created: 2024-10-07T11:46:13Z date_published: 2023-06-21T00:00:00Z date_updated: 2024-10-08T11:09:24Z day: '21' doi: 10.1038/s41586-023-06122-4 extern: '1' external_id: arxiv: - '2210.10919' pmid: - '37344594 ' intvolume: ' 619' issue: '7970' language: - iso: eng main_file_link: - open_access: '1' url: https://doi.org/10.48550/arXiv.2210.10919 month: '06' oa: 1 oa_version: Preprint page: 495-499 pmid: 1 publication: Nature publication_identifier: eissn: - 1476-4687 issn: - 0028-0836 publication_status: published publisher: Springer Nature quality_controlled: '1' scopus_import: '1' status: public title: Realization of a fractional quantum Hall state with ultracold atoms type: journal_article user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 volume: 619 year: '2023' ... --- _id: '18190' abstract: - lang: eng text: Strongly correlated systems can exhibit unexpected phenomena when brought in a state far from equilibrium. An example is many-body localization, which prevents generic interacting systems from reaching thermal equilibrium even at long times1,2. The stability of the many-body localized phase has been predicted to be hindered by the presence of small thermal inclusions that act as a bath, leading to the delocalization of the entire system through an avalanche propagation mechanism3,4,5,6,7,8. Here we study the dynamics of a thermal inclusion of variable size when it is coupled to a many-body localized system. We find evidence for accelerated transport of thermal inclusion into the localized region. We monitor how the avalanche spreads through the localized system and thermalizes it site by site by measuring the site-resolved entropy over time. Furthermore, we isolate the strongly correlated bath-induced dynamics with multipoint correlations between the bath and the system. Our results have implications on the robustness of many-body localized systems and their critical behaviour. article_processing_charge: No article_type: letter_note arxiv: 1 author: - first_name: Julian full_name: Leonard, Julian id: b75b3f45-7995-11ef-9bfd-9a9cd02c3577 last_name: Leonard - first_name: Sooshin full_name: Kim, Sooshin last_name: Kim - first_name: Matthew full_name: Rispoli, Matthew last_name: Rispoli - first_name: Alexander full_name: Lukin, Alexander last_name: Lukin - first_name: Robert full_name: Schittko, Robert last_name: Schittko - first_name: Joyce full_name: Kwan, Joyce last_name: Kwan - first_name: Eugene full_name: Demler, Eugene last_name: Demler - first_name: Dries full_name: Sels, Dries last_name: Sels - first_name: Markus full_name: Greiner, Markus last_name: Greiner citation: ama: Leonard J, Kim S, Rispoli M, et al. Probing the onset of quantum avalanches in a many-body localized system. Nature Physics. 2023;19(4):481-485. doi:10.1038/s41567-022-01887-3 apa: Leonard, J., Kim, S., Rispoli, M., Lukin, A., Schittko, R., Kwan, J., … Greiner, M. (2023). Probing the onset of quantum avalanches in a many-body localized system. Nature Physics. Springer Nature. https://doi.org/10.1038/s41567-022-01887-3 chicago: Leonard, Julian, Sooshin Kim, Matthew Rispoli, Alexander Lukin, Robert Schittko, Joyce Kwan, Eugene Demler, Dries Sels, and Markus Greiner. “Probing the Onset of Quantum Avalanches in a Many-Body Localized System.” Nature Physics. Springer Nature, 2023. https://doi.org/10.1038/s41567-022-01887-3. ieee: J. Leonard et al., “Probing the onset of quantum avalanches in a many-body localized system,” Nature Physics, vol. 19, no. 4. Springer Nature, pp. 481–485, 2023. ista: Leonard J, Kim S, Rispoli M, Lukin A, Schittko R, Kwan J, Demler E, Sels D, Greiner M. 2023. Probing the onset of quantum avalanches in a many-body localized system. Nature Physics. 19(4), 481–485. mla: Leonard, Julian, et al. “Probing the Onset of Quantum Avalanches in a Many-Body Localized System.” Nature Physics, vol. 19, no. 4, Springer Nature, 2023, pp. 481–85, doi:10.1038/s41567-022-01887-3. short: J. Leonard, S. Kim, M. Rispoli, A. Lukin, R. Schittko, J. Kwan, E. Demler, D. Sels, M. Greiner, Nature Physics 19 (2023) 481–485. date_created: 2024-10-07T11:46:33Z date_published: 2023-01-26T00:00:00Z date_updated: 2024-10-08T10:52:08Z day: '26' doi: 10.1038/s41567-022-01887-3 extern: '1' external_id: arxiv: - '2012.15270' intvolume: ' 19' issue: '4' language: - iso: eng main_file_link: - open_access: '1' url: https://doi.org/10.48550/arXiv.2012.15270 month: '01' oa: 1 oa_version: Preprint page: 481-485 publication: Nature Physics publication_identifier: eissn: - 1745-2481 issn: - 1745-2473 publication_status: published publisher: Springer Nature quality_controlled: '1' scopus_import: '1' status: public title: Probing the onset of quantum avalanches in a many-body localized system type: journal_article user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 volume: 19 year: '2023' ...