[{"publication_status":"published","file_date_updated":"2020-07-14T12:47:59Z","year":"2020","month":"02","related_material":{"record":[{"status":"public","id":"7524","relation":"part_of_dissertation"}]},"author":[{"first_name":"Simon","last_name":"Mayer","full_name":"Mayer, Simon","id":"30C4630A-F248-11E8-B48F-1D18A9856A87"}],"alternative_title":["ISTA Thesis"],"page":"148","ddc":["510"],"date_updated":"2026-04-08T07:25:40Z","OA_place":"publisher","project":[{"_id":"25C6DC12-B435-11E9-9278-68D0E5697425","call_identifier":"H2020","name":"Analysis of quantum many-body systems","grant_number":"694227"}],"has_accepted_license":"1","status":"public","abstract":[{"text":"We study the interacting homogeneous Bose gas in two spatial dimensions in the thermodynamic limit at fixed density. We shall be concerned with some mathematical aspects of this complicated problem in many-body quantum mechanics. More specifically, we consider the dilute limit where the scattering length of the interaction potential, which is a measure for the effective range of the potential, is small compared to the average distance between the particles. We are interested in a setting with positive (i.e., non-zero) temperature. After giving a survey of the relevant literature in the field, we provide some facts and examples to set expectations for the two-dimensional system. The crucial difference to the three-dimensional system is that there is no Bose–Einstein condensate at positive temperature due to the Hohenberg–Mermin–Wagner theorem. However, it turns out that an asymptotic formula for the free energy holds similarly to the three-dimensional case.\r\nWe motivate this formula by considering a toy model with δ interaction potential. By restricting this model Hamiltonian to certain trial states with a quasi-condensate we obtain an upper bound for the free energy that still has the quasi-condensate fraction as a free parameter. When minimizing over the quasi-condensate fraction, we obtain the Berezinskii–Kosterlitz–Thouless critical temperature for superfluidity, which plays an important role in our rigorous contribution. The mathematically rigorous result that we prove concerns the specific free energy in the dilute limit. We give upper and lower bounds on the free energy in terms of the free energy of the non-interacting system and a correction term coming from the interaction. Both bounds match and thus we obtain the leading term of an asymptotic approximation in the dilute limit, provided the thermal wavelength of the particles is of the same order (or larger) than the average distance between the particles. The remarkable feature of this result is its generality: the correction term depends on the interaction potential only through its scattering length and it holds for all nonnegative interaction potentials with finite scattering length that are measurable. In particular, this allows to model an interaction of hard disks.","lang":"eng"}],"type":"dissertation","corr_author":"1","date_created":"2020-02-24T09:17:27Z","oa_version":"Published Version","language":[{"iso":"eng"}],"citation":{"short":"S. Mayer, The Free Energy of a Dilute Two-Dimensional Bose Gas, Institute of Science and Technology Austria, 2020.","mla":"Mayer, Simon. <i>The Free Energy of a Dilute Two-Dimensional Bose Gas</i>. Institute of Science and Technology Austria, 2020, doi:<a href=\"https://doi.org/10.15479/AT:ISTA:7514\">10.15479/AT:ISTA:7514</a>.","ieee":"S. Mayer, “The free energy of a dilute two-dimensional Bose gas,” Institute of Science and Technology Austria, 2020.","ista":"Mayer S. 2020. The free energy of a dilute two-dimensional Bose gas. Institute of Science and Technology Austria.","ama":"Mayer S. The free energy of a dilute two-dimensional Bose gas. 2020. doi:<a href=\"https://doi.org/10.15479/AT:ISTA:7514\">10.15479/AT:ISTA:7514</a>","apa":"Mayer, S. (2020). <i>The free energy of a dilute two-dimensional Bose gas</i>. Institute of Science and Technology Austria. <a href=\"https://doi.org/10.15479/AT:ISTA:7514\">https://doi.org/10.15479/AT:ISTA:7514</a>","chicago":"Mayer, Simon. “The Free Energy of a Dilute Two-Dimensional Bose Gas.” Institute of Science and Technology Austria, 2020. <a href=\"https://doi.org/10.15479/AT:ISTA:7514\">https://doi.org/10.15479/AT:ISTA:7514</a>."},"ec_funded":1,"title":"The free energy of a dilute two-dimensional Bose gas","oa":1,"user_id":"ba8df636-2132-11f1-aed0-ed93e2281fdd","department":[{"_id":"RoSe"},{"_id":"GradSch"}],"day":"24","tmp":{"short":"CC BY (4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","image":"/images/cc_by.png","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)"},"publication_identifier":{"issn":["2663-337X"]},"article_processing_charge":"No","publisher":"Institute of Science and Technology Austria","degree_awarded":"PhD","doi":"10.15479/AT:ISTA:7514","file":[{"file_size":1563429,"checksum":"b4de7579ddc1dbdd44ff3f17c48395f6","date_updated":"2020-07-14T12:47:59Z","file_id":"7515","file_name":"thesis.pdf","relation":"main_file","creator":"dernst","access_level":"open_access","content_type":"application/pdf","date_created":"2020-02-24T09:15:06Z"},{"relation":"source_file","creator":"dernst","access_level":"closed","date_created":"2020-02-24T09:15:16Z","content_type":"application/x-zip-compressed","file_size":2028038,"checksum":"ad7425867b52d7d9e72296e87bc9cb67","date_updated":"2020-07-14T12:47:59Z","file_name":"thesis_source.zip","file_id":"7516"}],"supervisor":[{"first_name":"Robert","orcid":"0000-0002-6781-0521","last_name":"Seiringer","id":"4AFD0470-F248-11E8-B48F-1D18A9856A87","full_name":"Seiringer, Robert"}],"date_published":"2020-02-24T00:00:00Z","_id":"7514"},{"ddc":["536"],"date_updated":"2024-10-15T12:36:24Z","OA_place":"publisher","intvolume":"         3","OA_type":"gold","status":"public","has_accepted_license":"1","abstract":[{"lang":"eng","text":"In developing technologies based on superconducting quantum circuits, the need to control and route heating is a significant challenge in the experimental realisation and operation of these devices. One of the more ubiquitous devices in the current quantum computing toolbox is the transmon-type superconducting quantum bit, embedded in a resonator-based architecture. In the study of heat transport in superconducting circuits, a versatile and sensitive thermometer is based on studying the tunnelling characteristics of superconducting probes weakly coupled to a normal-metal island. Here we show that by integrating superconducting quantum bit coupled to two superconducting resonators at different frequencies, each resonator terminated (and thermally populated) by such a mesoscopic thin film metal island, one can experimentally observe magnetic flux-tunable photonic heat rectification between 0 and 10%."}],"type":"journal_article","publication":"Communications Physics","date_created":"2020-02-26T13:51:14Z","oa_version":"Published Version","language":[{"iso":"eng"}],"DOAJ_listed":"1","article_type":"original","citation":{"chicago":"Senior, Jorden L, Azat Gubaydullin, Bayan Karimi, Joonas T. Peltonen, Joachim Ankerhold, and Jukka P. Pekola. “Heat Rectification via a Superconducting Artificial Atom.” <i>Communications Physics</i>. Springer Nature, 2020. <a href=\"https://doi.org/10.1038/s42005-020-0307-5\">https://doi.org/10.1038/s42005-020-0307-5</a>.","apa":"Senior, J. L., Gubaydullin, A., Karimi, B., Peltonen, J. T., Ankerhold, J., &#38; Pekola, J. P. (2020). Heat rectification via a superconducting artificial atom. <i>Communications Physics</i>. Springer Nature. <a href=\"https://doi.org/10.1038/s42005-020-0307-5\">https://doi.org/10.1038/s42005-020-0307-5</a>","ista":"Senior JL, Gubaydullin A, Karimi B, Peltonen JT, Ankerhold J, Pekola JP. 2020. Heat rectification via a superconducting artificial atom. Communications Physics. 3(1), 40.","ama":"Senior JL, Gubaydullin A, Karimi B, Peltonen JT, Ankerhold J, Pekola JP. Heat rectification via a superconducting artificial atom. <i>Communications Physics</i>. 2020;3(1). doi:<a href=\"https://doi.org/10.1038/s42005-020-0307-5\">10.1038/s42005-020-0307-5</a>","ieee":"J. L. Senior, A. Gubaydullin, B. Karimi, J. T. Peltonen, J. Ankerhold, and J. P. Pekola, “Heat rectification via a superconducting artificial atom,” <i>Communications Physics</i>, vol. 3, no. 1. Springer Nature, 2020.","mla":"Senior, Jorden L., et al. “Heat Rectification via a Superconducting Artificial Atom.” <i>Communications Physics</i>, vol. 3, no. 1, 40, Springer Nature, 2020, doi:<a href=\"https://doi.org/10.1038/s42005-020-0307-5\">10.1038/s42005-020-0307-5</a>.","short":"J.L. Senior, A. Gubaydullin, B. Karimi, J.T. Peltonen, J. Ankerhold, J.P. Pekola, Communications Physics 3 (2020)."},"publication_status":"published","file_date_updated":"2020-07-14T12:48:00Z","year":"2020","month":"02","volume":3,"issue":"1","author":[{"first_name":"Jorden L","orcid":"0000-0002-0672-9295","last_name":"Senior","id":"5479D234-2D30-11EA-89CC-40953DDC885E","full_name":"Senior, Jorden L"},{"first_name":"Azat","last_name":"Gubaydullin","full_name":"Gubaydullin, Azat"},{"last_name":"Karimi","first_name":"Bayan","full_name":"Karimi, Bayan"},{"first_name":"Joonas T.","last_name":"Peltonen","full_name":"Peltonen, Joonas T."},{"last_name":"Ankerhold","first_name":"Joachim","full_name":"Ankerhold, Joachim"},{"full_name":"Pekola, Jukka P.","first_name":"Jukka P.","last_name":"Pekola"}],"extern":"1","publisher":"Springer Nature","file":[{"date_created":"2020-03-03T10:41:13Z","content_type":"application/pdf","access_level":"open_access","creator":"dernst","relation":"main_file","file_name":"s42005-020-0307-5.pdf","file_id":"7559","date_updated":"2020-07-14T12:48:00Z","checksum":"59255f51d9f113c40e3047e9ac83d367","file_size":1590721},{"file_size":1007249,"checksum":"8325ae7b3c869d9aa6ed84823da4000a","file_id":"7560","file_name":"42005_2020_307_MOESM1_ESM.pdf","date_updated":"2020-07-14T12:48:00Z","creator":"dernst","relation":"main_file","access_level":"open_access","date_created":"2020-03-03T10:41:13Z","content_type":"application/pdf"}],"doi":"10.1038/s42005-020-0307-5","article_number":"40","_id":"7530","quality_controlled":"1","date_published":"2020-02-25T00:00:00Z","title":"Heat rectification via a superconducting artificial atom","oa":1,"user_id":"0043cee0-e5fc-11ee-9736-f83bc23afbf0","day":"25","tmp":{"short":"CC BY (4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","image":"/images/cc_by.png","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)"},"publication_identifier":{"issn":["2399-3650"]},"article_processing_charge":"No"},{"intvolume":"         5","arxiv":1,"date_updated":"2023-08-18T06:44:46Z","type":"journal_article","main_file_link":[{"url":"https://arxiv.org/abs/1912.09270","open_access":"1"}],"oa_version":"Preprint","date_created":"2020-02-27T10:26:57Z","scopus_import":"1","publication":"Physical Review Fluids","status":"public","external_id":{"arxiv":["1912.09270"],"isi":["000515065100001"]},"abstract":[{"lang":"eng","text":"In the past two decades, our understanding of the transition to turbulence in shear flows with linearly stable laminar solutions has greatly improved. Regarding the susceptibility of the laminar flow, two concepts have been particularly useful: the edge states and the minimal seeds. In this nonlinear picture of the transition, the basin boundary of turbulence is set by the edge state's stable manifold and this manifold comes closest in energy to the laminar equilibrium at the minimal seed. We begin this paper by presenting numerical experiments in which three-dimensional perturbations are too energetic to trigger turbulence in pipe flow but they do lead to turbulence when their amplitude is reduced. We show that this seemingly counterintuitive observation is in fact consistent with the fully nonlinear description of the transition mediated by the edge state. In order to understand the physical mechanisms behind this process, we measure the turbulent kinetic energy production and dissipation rates as a function of the radial coordinate. Our main observation is that the transition to turbulence relies on the energy amplification away from the wall, as opposed to the turbulence itself, whose energy is predominantly produced near the wall. This observation is further supported by the similar analyses on the minimal seeds and the edge states. Furthermore, we show that the time evolution of production-over-dissipation curves provides a clear distinction between the different initial amplification stages of the transition to turbulence from the minimal seed."}],"language":[{"iso":"eng"}],"citation":{"chicago":"Budanur, Nazmi B, Elena Marensi, Ashley P. Willis, and Björn Hof. “Upper Edge of Chaos and the Energetics of Transition in Pipe Flow.” <i>Physical Review Fluids</i>. American Physical Society, 2020. <a href=\"https://doi.org/10.1103/physrevfluids.5.023903\">https://doi.org/10.1103/physrevfluids.5.023903</a>.","apa":"Budanur, N. B., Marensi, E., Willis, A. P., &#38; Hof, B. (2020). Upper edge of chaos and the energetics of transition in pipe flow. <i>Physical Review Fluids</i>. American Physical Society. <a href=\"https://doi.org/10.1103/physrevfluids.5.023903\">https://doi.org/10.1103/physrevfluids.5.023903</a>","ama":"Budanur NB, Marensi E, Willis AP, Hof B. Upper edge of chaos and the energetics of transition in pipe flow. <i>Physical Review Fluids</i>. 2020;5(2). doi:<a href=\"https://doi.org/10.1103/physrevfluids.5.023903\">10.1103/physrevfluids.5.023903</a>","ieee":"N. B. Budanur, E. Marensi, A. P. Willis, and B. Hof, “Upper edge of chaos and the energetics of transition in pipe flow,” <i>Physical Review Fluids</i>, vol. 5, no. 2. American Physical Society, 2020.","ista":"Budanur NB, Marensi E, Willis AP, Hof B. 2020. Upper edge of chaos and the energetics of transition in pipe flow. Physical Review Fluids. 5(2), 023903.","mla":"Budanur, Nazmi B., et al. “Upper Edge of Chaos and the Energetics of Transition in Pipe Flow.” <i>Physical Review Fluids</i>, vol. 5, no. 2, 023903, American Physical Society, 2020, doi:<a href=\"https://doi.org/10.1103/physrevfluids.5.023903\">10.1103/physrevfluids.5.023903</a>.","short":"N.B. Budanur, E. Marensi, A.P. Willis, B. Hof, Physical Review Fluids 5 (2020)."},"article_type":"original","year":"2020","publication_status":"published","volume":5,"issue":"2","month":"02","author":[{"id":"3EA1010E-F248-11E8-B48F-1D18A9856A87","full_name":"Budanur, Nazmi B","first_name":"Nazmi B","orcid":"0000-0003-0423-5010","last_name":"Budanur"},{"first_name":"Elena","last_name":"Marensi","full_name":"Marensi, Elena"},{"first_name":"Ashley P.","last_name":"Willis","full_name":"Willis, Ashley P."},{"first_name":"Björn","orcid":"0000-0003-2057-2754","last_name":"Hof","id":"3A374330-F248-11E8-B48F-1D18A9856A87","full_name":"Hof, Björn"}],"doi":"10.1103/physrevfluids.5.023903","isi":1,"publisher":"American Physical Society","_id":"7534","date_published":"2020-02-21T00:00:00Z","quality_controlled":"1","article_number":"023903","user_id":"4359f0d1-fa6c-11eb-b949-802e58b17ae8","title":"Upper edge of chaos and the energetics of transition in pipe flow","oa":1,"day":"21","department":[{"_id":"BjHo"}],"article_processing_charge":"No","publication_identifier":{"issn":["2469-990X"]}},{"type":"journal_article","oa_version":"None","scopus_import":"1","date_created":"2020-02-28T09:18:01Z","publication":"Israel Journal of Plant Sciences","status":"public","external_id":{"isi":["000525343300004"]},"abstract":[{"text":" In vitro propagation of the ornamentally interesting species Wikstroemia gemmata is limited by the recalcitrance to form adventitious roots. In this article, two strategies to improve the rooting capacity of in vitro microcuttings are presented. Firstly, the effect of exogenous auxin was evaluated in both light and dark cultivated stem segments and also the sucrose-content of the medium was varied in order to determine better rooting conditions. Secondly, different spectral lights were evaluated and the effect on shoot growth and root induction demonstrated that the exact spectral composition of light is important for successful in vitro growth and development of Wikstroemia gemmata. We show that exogenous auxin cannot compensate for the poor rooting under unfavorable light conditions. Adapting the culture conditions is therefore paramount for successful industrial propagation of Wikstroemia gemmata. ","lang":"eng"}],"language":[{"iso":"eng"}],"citation":{"short":"I. Verstraeten, H. Buyle, S. Werbrouck, M.C. Van Labeke, D. Geelen, Israel Journal of Plant Sciences 67 (2020) 16–26.","mla":"Verstraeten, Inge, et al. “In Vitro Shoot Growth and Adventitious Rooting of Wikstroemia Gemmata Depends on Light Quality.” <i>Israel Journal of Plant Sciences</i>, vol. 67, no. 1–2, Brill, 2020, pp. 16–26, doi:<a href=\"https://doi.org/10.1163/22238980-20191110\">10.1163/22238980-20191110</a>.","ista":"Verstraeten I, Buyle H, Werbrouck S, Van Labeke MC, Geelen D. 2020. In vitro shoot growth and adventitious rooting of Wikstroemia gemmata depends on light quality. Israel Journal of Plant Sciences. 67(1–2), 16–26.","ama":"Verstraeten I, Buyle H, Werbrouck S, Van Labeke MC, Geelen D. In vitro shoot growth and adventitious rooting of Wikstroemia gemmata depends on light quality. <i>Israel Journal of Plant Sciences</i>. 2020;67(1-2):16-26. doi:<a href=\"https://doi.org/10.1163/22238980-20191110\">10.1163/22238980-20191110</a>","ieee":"I. Verstraeten, H. Buyle, S. Werbrouck, M. C. Van Labeke, and D. Geelen, “In vitro shoot growth and adventitious rooting of Wikstroemia gemmata depends on light quality,” <i>Israel Journal of Plant Sciences</i>, vol. 67, no. 1–2. Brill, pp. 16–26, 2020.","apa":"Verstraeten, I., Buyle, H., Werbrouck, S., Van Labeke, M. C., &#38; Geelen, D. (2020). In vitro shoot growth and adventitious rooting of Wikstroemia gemmata depends on light quality. <i>Israel Journal of Plant Sciences</i>. Brill. <a href=\"https://doi.org/10.1163/22238980-20191110\">https://doi.org/10.1163/22238980-20191110</a>","chicago":"Verstraeten, Inge, H. Buyle, S. Werbrouck, M.C. Van Labeke, and D. Geelen. “In Vitro Shoot Growth and Adventitious Rooting of Wikstroemia Gemmata Depends on Light Quality.” <i>Israel Journal of Plant Sciences</i>. Brill, 2020. <a href=\"https://doi.org/10.1163/22238980-20191110\">https://doi.org/10.1163/22238980-20191110</a>."},"article_type":"original","intvolume":"        67","date_updated":"2023-08-18T06:45:15Z","author":[{"full_name":"Verstraeten, Inge","id":"362BF7FE-F248-11E8-B48F-1D18A9856A87","last_name":"Verstraeten","orcid":"0000-0001-7241-2328","first_name":"Inge"},{"full_name":"Buyle, H.","first_name":"H.","last_name":"Buyle"},{"last_name":"Werbrouck","first_name":"S.","full_name":"Werbrouck, S."},{"last_name":"Van Labeke","first_name":"M.C.","full_name":"Van Labeke, M.C."},{"full_name":"Geelen, D.","first_name":"D.","last_name":"Geelen"}],"page":"16-26","year":"2020","publication_status":"published","volume":67,"issue":"1-2","month":"02","_id":"7540","quality_controlled":"1","date_published":"2020-02-01T00:00:00Z","doi":"10.1163/22238980-20191110","isi":1,"publisher":"Brill","article_processing_charge":"No","publication_identifier":{"issn":["0792-9978"],"eissn":["2223-8980"]},"user_id":"4359f0d1-fa6c-11eb-b949-802e58b17ae8","title":"In vitro shoot growth and adventitious rooting of Wikstroemia gemmata depends on light quality","day":"01","department":[{"_id":"JiFr"}]},{"pmid":1,"acknowledged_ssus":[{"_id":"NanoFab"},{"_id":"M-Shop"}],"author":[{"full_name":"Gao, Fei","last_name":"Gao","first_name":"Fei"},{"last_name":"Wang","first_name":"Jian-Huan","full_name":"Wang, Jian-Huan"},{"first_name":"Hannes","last_name":"Watzinger","id":"35DF8E50-F248-11E8-B48F-1D18A9856A87","full_name":"Watzinger, Hannes"},{"full_name":"Hu, Hao","last_name":"Hu","first_name":"Hao"},{"full_name":"Rančić, Marko J.","last_name":"Rančić","first_name":"Marko J."},{"first_name":"Jie-Yin","last_name":"Zhang","full_name":"Zhang, Jie-Yin"},{"last_name":"Wang","first_name":"Ting","full_name":"Wang, Ting"},{"first_name":"Yuan","last_name":"Yao","full_name":"Yao, Yuan"},{"last_name":"Wang","first_name":"Gui-Lei","full_name":"Wang, Gui-Lei"},{"full_name":"Kukucka, Josip","id":"3F5D8856-F248-11E8-B48F-1D18A9856A87","last_name":"Kukucka","first_name":"Josip"},{"orcid":"0000-0003-2424-8636","first_name":"Lada","last_name":"Vukušić","full_name":"Vukušić, Lada","id":"31E9F056-F248-11E8-B48F-1D18A9856A87"},{"full_name":"Kloeffel, Christoph","last_name":"Kloeffel","first_name":"Christoph"},{"last_name":"Loss","first_name":"Daniel","full_name":"Loss, Daniel"},{"last_name":"Liu","first_name":"Feng","full_name":"Liu, Feng"},{"last_name":"Katsaros","orcid":"0000-0001-8342-202X","first_name":"Georgios","full_name":"Katsaros, Georgios","id":"38DB5788-F248-11E8-B48F-1D18A9856A87"},{"full_name":"Zhang, Jian-Jun","first_name":"Jian-Jun","last_name":"Zhang"}],"month":"04","related_material":{"record":[{"relation":"research_data","status":"public","id":"9222"},{"relation":"dissertation_contains","id":"7996","status":"public"},{"relation":"other","id":"17444","status":"public"}]},"issue":"16","volume":32,"file_date_updated":"2020-11-20T10:11:35Z","publication_status":"published","year":"2020","citation":{"mla":"Gao, Fei, et al. “Site-Controlled Uniform Ge/Si Hut Wires with Electrically Tunable Spin-Orbit Coupling.” <i>Advanced Materials</i>, vol. 32, no. 16, 1906523, Wiley, 2020, doi:<a href=\"https://doi.org/10.1002/adma.201906523\">10.1002/adma.201906523</a>.","short":"F. Gao, J.-H. Wang, H. Watzinger, H. Hu, M.J. Rančić, J.-Y. Zhang, T. Wang, Y. Yao, G.-L. Wang, J. Kukucka, L. Vukušić, C. Kloeffel, D. Loss, F. Liu, G. Katsaros, J.-J. Zhang, Advanced Materials 32 (2020).","apa":"Gao, F., Wang, J.-H., Watzinger, H., Hu, H., Rančić, M. J., Zhang, J.-Y., … Zhang, J.-J. (2020). Site-controlled uniform Ge/Si hut wires with electrically tunable spin-orbit coupling. <i>Advanced Materials</i>. Wiley. <a href=\"https://doi.org/10.1002/adma.201906523\">https://doi.org/10.1002/adma.201906523</a>","ista":"Gao F, Wang J-H, Watzinger H, Hu H, Rančić MJ, Zhang J-Y, Wang T, Yao Y, Wang G-L, Kukucka J, Vukušić L, Kloeffel C, Loss D, Liu F, Katsaros G, Zhang J-J. 2020. Site-controlled uniform Ge/Si hut wires with electrically tunable spin-orbit coupling. Advanced Materials. 32(16), 1906523.","ieee":"F. Gao <i>et al.</i>, “Site-controlled uniform Ge/Si hut wires with electrically tunable spin-orbit coupling,” <i>Advanced Materials</i>, vol. 32, no. 16. Wiley, 2020.","ama":"Gao F, Wang J-H, Watzinger H, et al. Site-controlled uniform Ge/Si hut wires with electrically tunable spin-orbit coupling. <i>Advanced Materials</i>. 2020;32(16). doi:<a href=\"https://doi.org/10.1002/adma.201906523\">10.1002/adma.201906523</a>","chicago":"Gao, Fei, Jian-Huan Wang, Hannes Watzinger, Hao Hu, Marko J. Rančić, Jie-Yin Zhang, Ting Wang, et al. “Site-Controlled Uniform Ge/Si Hut Wires with Electrically Tunable Spin-Orbit Coupling.” <i>Advanced Materials</i>. Wiley, 2020. <a href=\"https://doi.org/10.1002/adma.201906523\">https://doi.org/10.1002/adma.201906523</a>."},"ec_funded":1,"article_type":"original","language":[{"iso":"eng"}],"abstract":[{"text":"Semiconductor nanowires have been playing a crucial role in the development of nanoscale devices for the realization of spin qubits, Majorana fermions, single photon emitters, nanoprocessors, etc. The monolithic growth of site‐controlled nanowires is a prerequisite toward the next generation of devices that will require addressability and scalability. Here, combining top‐down nanofabrication and bottom‐up self‐assembly, the growth of Ge wires on prepatterned Si (001) substrates with controllable position, distance, length, and structure is reported. This is achieved by a novel growth process that uses a SiGe strain‐relaxation template and can be potentially generalized to other material combinations. Transport measurements show an electrically tunable spin–orbit coupling, with a spin–orbit length similar to that of III–V materials. Also, charge sensing between quantum dots in closely spaced wires is observed, which underlines their potential for the realization of advanced quantum devices. The reported results open a path toward scalable qubit devices using nanowires on silicon.","lang":"eng"}],"status":"public","external_id":{"pmid":["32105375"],"isi":["000516660900001"]},"has_accepted_license":"1","scopus_import":"1","publication":"Advanced Materials","oa_version":"Published Version","date_created":"2020-02-28T09:47:00Z","corr_author":"1","type":"journal_article","project":[{"grant_number":"335497","call_identifier":"FP7","name":"Towards Spin qubits and Majorana fermions in Germanium self assembled hut-wires","_id":"25517E86-B435-11E9-9278-68D0E5697425"},{"grant_number":"P32235","name":"Towards scalable hut wire quantum devices","_id":"237B3DA4-32DE-11EA-91FC-C7463DDC885E","call_identifier":"FWF"},{"_id":"237E5020-32DE-11EA-91FC-C7463DDC885E","name":"TOPOLOGICALLY PROTECTED AND SCALABLE QUANTUM BITS","call_identifier":"H2020","grant_number":"862046"}],"date_updated":"2026-06-18T17:54:46Z","ddc":["530"],"intvolume":"        32","publication_identifier":{"issn":["0935-9648"]},"tmp":{"short":"CC BY (4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","image":"/images/cc_by.png","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)"},"article_processing_charge":"Yes (via OA deal)","department":[{"_id":"GeKa"}],"day":"23","oa":1,"title":"Site-controlled uniform Ge/Si hut wires with electrically tunable spin-orbit coupling","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","article_number":"1906523","date_published":"2020-04-23T00:00:00Z","_id":"7541","quality_controlled":"1","publisher":"Wiley","doi":"10.1002/adma.201906523","file":[{"success":1,"checksum":"c622737dc295972065782558337124a2","file_id":"8782","file_name":"2020_AdvancedMaterials_Gao.pdf","date_updated":"2020-11-20T10:11:35Z","file_size":5242880,"date_created":"2020-11-20T10:11:35Z","content_type":"application/pdf","creator":"dernst","relation":"main_file","access_level":"open_access"}],"acknowledgement":"This work was supported by the National Key R&D Program of China (Grant Nos. 2016YFA0301701 and 2016YFA0300600), the NSFC (Grant Nos. 11574356, 11434010, and 11404252), the Strategic Priority Research Program of CAS (Grant No. XDB30000000), the ERC Starting Grant No. 335497, the FWF P32235 project, and the European Union's Horizon 2020 research and innovation program under Grant Agreement #862046. This research was supported by the Scientific Service Units of IST Austria through resources provided by the MIBA Machine Shop and the nanofabrication facility. F.L. thanks support from DOE (Grant No. DE‐FG02‐04ER46148). H.H. thanks the Startup Funding from Xi'an Jiaotong University.","isi":1},{"article_processing_charge":"No","publication_identifier":{"issn":["0012-1606"]},"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","oa":1,"title":"Long-term activity drives dendritic branch elaboration of a C. elegans sensory neuron","day":"01","_id":"7545","quality_controlled":"1","date_published":"2020-05-01T00:00:00Z","extern":"1","doi":"10.1016/j.ydbio.2020.01.005","publisher":"Elsevier","author":[{"last_name":"Cohn","first_name":"Jesse A.","full_name":"Cohn, Jesse A."},{"first_name":"Elizabeth R.","last_name":"Cebul","full_name":"Cebul, Elizabeth R."},{"full_name":"Valperga, Giulio","last_name":"Valperga","first_name":"Giulio"},{"last_name":"Brose","first_name":"Lotti","full_name":"Brose, Lotti"},{"id":"4E3FF80E-F248-11E8-B48F-1D18A9856A87","full_name":"de Bono, Mario","last_name":"de Bono","first_name":"Mario","orcid":"0000-0001-8347-0443"},{"full_name":"Heiman, Maxwell G.","last_name":"Heiman","first_name":"Maxwell G."},{"last_name":"Pierce","first_name":"Jonathan T.","full_name":"Pierce, Jonathan T."}],"page":"66-74","year":"2020","publication_status":"published","issue":"1","volume":461,"month":"05","oa_version":"Preprint","publication":"Developmental Biology","date_created":"2020-02-28T10:38:32Z","main_file_link":[{"url":"https://doi.org/10.1101/685339","open_access":"1"}],"type":"journal_article","abstract":[{"lang":"eng","text":"Neuronal activity often leads to alterations in gene expression and cellular architecture. The nematode Caenorhabditis elegans, owing to its compact translucent nervous system, is a powerful system in which to study conserved aspects of the development and plasticity of neuronal morphology. Here we focus on one pair of sensory neurons, termed URX, which the worm uses to sense and avoid high levels of environmental oxygen. Previous studies have reported that the URX neuron pair has variable branched endings at its dendritic sensory tip. By controlling oxygen levels and analyzing mutants, we found that these microtubule-rich branched endings grow over time as a consequence of neuronal activity in adulthood. We also find that the growth of these branches correlates with an increase in cellular sensitivity to particular ranges of oxygen that is observable in the behavior of older worms. Given the strengths of C. elegans as a model organism, URX may serve as a potent system for uncovering genes and mechanisms involved in activity-dependent morphological changes in neurons and possible adaptive changes in the aging nervous system."}],"status":"public","citation":{"ieee":"J. A. Cohn <i>et al.</i>, “Long-term activity drives dendritic branch elaboration of a C. elegans sensory neuron,” <i>Developmental Biology</i>, vol. 461, no. 1. Elsevier, pp. 66–74, 2020.","ista":"Cohn JA, Cebul ER, Valperga G, Brose L, de Bono M, Heiman MG, Pierce JT. 2020. Long-term activity drives dendritic branch elaboration of a C. elegans sensory neuron. Developmental Biology. 461(1), 66–74.","ama":"Cohn JA, Cebul ER, Valperga G, et al. Long-term activity drives dendritic branch elaboration of a C. elegans sensory neuron. <i>Developmental Biology</i>. 2020;461(1):66-74. doi:<a href=\"https://doi.org/10.1016/j.ydbio.2020.01.005\">10.1016/j.ydbio.2020.01.005</a>","apa":"Cohn, J. A., Cebul, E. R., Valperga, G., Brose, L., de Bono, M., Heiman, M. G., &#38; Pierce, J. T. (2020). Long-term activity drives dendritic branch elaboration of a C. elegans sensory neuron. <i>Developmental Biology</i>. Elsevier. <a href=\"https://doi.org/10.1016/j.ydbio.2020.01.005\">https://doi.org/10.1016/j.ydbio.2020.01.005</a>","short":"J.A. Cohn, E.R. Cebul, G. Valperga, L. Brose, M. de Bono, M.G. Heiman, J.T. Pierce, Developmental Biology 461 (2020) 66–74.","mla":"Cohn, Jesse A., et al. “Long-Term Activity Drives Dendritic Branch Elaboration of a C. Elegans Sensory Neuron.” <i>Developmental Biology</i>, vol. 461, no. 1, Elsevier, 2020, pp. 66–74, doi:<a href=\"https://doi.org/10.1016/j.ydbio.2020.01.005\">10.1016/j.ydbio.2020.01.005</a>.","chicago":"Cohn, Jesse A., Elizabeth R. Cebul, Giulio Valperga, Lotti Brose, Mario de Bono, Maxwell G. Heiman, and Jonathan T. Pierce. “Long-Term Activity Drives Dendritic Branch Elaboration of a C. Elegans Sensory Neuron.” <i>Developmental Biology</i>. Elsevier, 2020. <a href=\"https://doi.org/10.1016/j.ydbio.2020.01.005\">https://doi.org/10.1016/j.ydbio.2020.01.005</a>."},"article_type":"original","language":[{"iso":"eng"}],"intvolume":"       461","date_updated":"2021-01-12T08:14:06Z"},{"date_updated":"2024-10-09T20:59:20Z","ddc":["570"],"intvolume":"       105","abstract":[{"lang":"eng","text":"The extent to which behavior is shaped by experience varies between individuals. Genetic differences contribute to this variation, but the neural mechanisms are not understood. Here, we dissect natural variation in the behavioral flexibility of two Caenorhabditis elegans wild strains. In one strain, a memory of exposure to 21% O2 suppresses CO2-evoked locomotory arousal; in the other, CO2 evokes arousal regardless of previous O2 experience. We map that variation to a polymorphic dendritic scaffold protein, ARCP-1, expressed in sensory neurons. ARCP-1 binds the Ca2+-dependent phosphodiesterase PDE-1 and co-localizes PDE-1 with molecular sensors for CO2 at dendritic ends. Reducing ARCP-1 or PDE-1 activity promotes CO2 escape by altering neuropeptide expression in the BAG CO2 sensors. Variation in ARCP-1 alters behavioral plasticity in multiple paradigms. Our findings are reminiscent of genetic accommodation, an evolutionary process by which phenotypic flexibility in response to environmental variation is reset by genetic change."}],"has_accepted_license":"1","status":"public","external_id":{"isi":["000507341300012"],"pmid":["31757604"]},"publication":"Neuron","date_created":"2020-02-28T10:43:39Z","oa_version":"Published Version","type":"journal_article","corr_author":"1","article_type":"original","citation":{"chicago":"Beets, Isabel, Gaotian Zhang, Lorenz A. Fenk, Changchun Chen, Geoffrey M. Nelson, Marie-Anne Félix, and Mario de Bono. “Natural Variation in a Dendritic Scaffold Protein Remodels Experience-Dependent Plasticity by Altering Neuropeptide Expression.” <i>Neuron</i>. Cell Press, 2020. <a href=\"https://doi.org/10.1016/j.neuron.2019.10.001\">https://doi.org/10.1016/j.neuron.2019.10.001</a>.","short":"I. Beets, G. Zhang, L.A. Fenk, C. Chen, G.M. Nelson, M.-A. Félix, M. de Bono, Neuron 105 (2020) 106–121.e10.","mla":"Beets, Isabel, et al. “Natural Variation in a Dendritic Scaffold Protein Remodels Experience-Dependent Plasticity by Altering Neuropeptide Expression.” <i>Neuron</i>, vol. 105, no. 1, Cell Press, 2020, p. 106–121.e10, doi:<a href=\"https://doi.org/10.1016/j.neuron.2019.10.001\">10.1016/j.neuron.2019.10.001</a>.","ista":"Beets I, Zhang G, Fenk LA, Chen C, Nelson GM, Félix M-A, de Bono M. 2020. Natural variation in a dendritic scaffold protein remodels experience-dependent plasticity by altering neuropeptide expression. Neuron. 105(1), 106–121.e10.","ieee":"I. Beets <i>et al.</i>, “Natural variation in a dendritic scaffold protein remodels experience-dependent plasticity by altering neuropeptide expression,” <i>Neuron</i>, vol. 105, no. 1. Cell Press, p. 106–121.e10, 2020.","ama":"Beets I, Zhang G, Fenk LA, et al. Natural variation in a dendritic scaffold protein remodels experience-dependent plasticity by altering neuropeptide expression. <i>Neuron</i>. 2020;105(1):106-121.e10. doi:<a href=\"https://doi.org/10.1016/j.neuron.2019.10.001\">10.1016/j.neuron.2019.10.001</a>","apa":"Beets, I., Zhang, G., Fenk, L. A., Chen, C., Nelson, G. M., Félix, M.-A., &#38; de Bono, M. (2020). Natural variation in a dendritic scaffold protein remodels experience-dependent plasticity by altering neuropeptide expression. <i>Neuron</i>. Cell Press. <a href=\"https://doi.org/10.1016/j.neuron.2019.10.001\">https://doi.org/10.1016/j.neuron.2019.10.001</a>"},"language":[{"iso":"eng"}],"file_date_updated":"2020-07-14T12:48:00Z","publication_status":"published","year":"2020","month":"01","issue":"1","volume":105,"author":[{"last_name":"Beets","first_name":"Isabel","full_name":"Beets, Isabel"},{"last_name":"Zhang","first_name":"Gaotian","full_name":"Zhang, Gaotian"},{"first_name":"Lorenz A.","last_name":"Fenk","full_name":"Fenk, Lorenz A."},{"last_name":"Chen","first_name":"Changchun","full_name":"Chen, Changchun"},{"first_name":"Geoffrey M.","last_name":"Nelson","full_name":"Nelson, Geoffrey M."},{"first_name":"Marie-Anne","last_name":"Félix","full_name":"Félix, Marie-Anne"},{"last_name":"de Bono","orcid":"0000-0001-8347-0443","first_name":"Mario","full_name":"de Bono, Mario","id":"4E3FF80E-F248-11E8-B48F-1D18A9856A87"}],"page":"106-121.e10","pmid":1,"publisher":"Cell Press","doi":"10.1016/j.neuron.2019.10.001","isi":1,"file":[{"access_level":"open_access","relation":"main_file","creator":"dernst","date_created":"2020-03-02T15:43:57Z","content_type":"application/pdf","file_size":3294066,"date_updated":"2020-07-14T12:48:00Z","file_name":"2020_Neuron_Beets.pdf","file_id":"7558","checksum":"799bfd297a008753a688b30d3958fa48"}],"quality_controlled":"1","_id":"7546","date_published":"2020-01-08T00:00:00Z","oa":1,"title":"Natural variation in a dendritic scaffold protein remodels experience-dependent plasticity by altering neuropeptide expression","user_id":"4359f0d1-fa6c-11eb-b949-802e58b17ae8","department":[{"_id":"MaDe"}],"day":"08","publication_identifier":{"issn":["0896-6273"]},"tmp":{"short":"CC BY (4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","image":"/images/cc_by.png","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)"},"article_processing_charge":"No"},{"abstract":[{"lang":"eng","text":"Slicing a Voronoi tessellation in ${R}^n$ with a $k$-plane gives a $k$-dimensional weighted Voronoi tessellation, also known as a power diagram or Laguerre tessellation. Mapping every simplex of the dual weighted Delaunay mosaic to the radius of the smallest empty circumscribed sphere whose center lies in the $k$-plane gives a generalized discrete Morse function. Assuming the Voronoi tessellation is generated by a Poisson point process in ${R}^n$, we study the expected number of simplices in the $k$-dimensional weighted Delaunay mosaic as well as the expected number of intervals of the Morse function, both as functions of a radius threshold. As a by-product, we obtain a new proof for the expected number of connected components (clumps) in a line section of a circular Boolean model in ${R}^n$."}],"external_id":{"isi":["000551393100007"],"arxiv":["1705.08735"]},"status":"public","scopus_import":"1","date_created":"2020-03-01T23:00:39Z","oa_version":"Preprint","publication":"Theory of Probability and its Applications","main_file_link":[{"open_access":"1","url":"https://arxiv.org/abs/1705.08735"}],"type":"journal_article","ec_funded":1,"article_type":"original","citation":{"short":"H. Edelsbrunner, A. Nikitenko, Theory of Probability and Its Applications 64 (2020) 595–614.","mla":"Edelsbrunner, Herbert, and Anton Nikitenko. “Weighted Poisson–Delaunay Mosaics.” <i>Theory of Probability and Its Applications</i>, vol. 64, no. 4, SIAM, 2020, pp. 595–614, doi:<a href=\"https://doi.org/10.1137/S0040585X97T989726\">10.1137/S0040585X97T989726</a>.","ista":"Edelsbrunner H, Nikitenko A. 2020. Weighted Poisson–Delaunay mosaics. Theory of Probability and its Applications. 64(4), 595–614.","ama":"Edelsbrunner H, Nikitenko A. Weighted Poisson–Delaunay mosaics. <i>Theory of Probability and its Applications</i>. 2020;64(4):595-614. doi:<a href=\"https://doi.org/10.1137/S0040585X97T989726\">10.1137/S0040585X97T989726</a>","ieee":"H. Edelsbrunner and A. Nikitenko, “Weighted Poisson–Delaunay mosaics,” <i>Theory of Probability and its Applications</i>, vol. 64, no. 4. SIAM, pp. 595–614, 2020.","apa":"Edelsbrunner, H., &#38; Nikitenko, A. (2020). Weighted Poisson–Delaunay mosaics. <i>Theory of Probability and Its Applications</i>. SIAM. <a href=\"https://doi.org/10.1137/S0040585X97T989726\">https://doi.org/10.1137/S0040585X97T989726</a>","chicago":"Edelsbrunner, Herbert, and Anton Nikitenko. “Weighted Poisson–Delaunay Mosaics.” <i>Theory of Probability and Its Applications</i>. SIAM, 2020. <a href=\"https://doi.org/10.1137/S0040585X97T989726\">https://doi.org/10.1137/S0040585X97T989726</a>."},"language":[{"iso":"eng"}],"date_updated":"2025-07-10T11:54:44Z","arxiv":1,"intvolume":"        64","project":[{"name":"Alpha Shape Theory Extended","call_identifier":"H2020","_id":"266A2E9E-B435-11E9-9278-68D0E5697425","grant_number":"788183"},{"_id":"2561EBF4-B435-11E9-9278-68D0E5697425","call_identifier":"FWF","name":"Persistence and stability of geometric complexes","grant_number":"I02979-N35"}],"author":[{"first_name":"Herbert","orcid":"0000-0002-9823-6833","last_name":"Edelsbrunner","id":"3FB178DA-F248-11E8-B48F-1D18A9856A87","full_name":"Edelsbrunner, Herbert"},{"last_name":"Nikitenko","first_name":"Anton","orcid":"0000-0002-0659-3201","id":"3E4FF1BA-F248-11E8-B48F-1D18A9856A87","full_name":"Nikitenko, Anton"}],"page":"595-614","publication_status":"published","year":"2020","month":"02","issue":"4","volume":64,"quality_controlled":"1","_id":"7554","date_published":"2020-02-13T00:00:00Z","publisher":"SIAM","isi":1,"doi":"10.1137/S0040585X97T989726","publication_identifier":{"eissn":["1095-7219"],"issn":["0040-585X"]},"article_processing_charge":"No","oa":1,"title":"Weighted Poisson–Delaunay mosaics","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","department":[{"_id":"HeEd"}],"day":"13"},{"publisher":"American Chemical Society","doi":"10.1021/jacs.9b13450.s002","date_updated":"2025-07-10T11:55:01Z","citation":{"chicago":"Gupta, Chitrak, Umesh Khaniya, Chun Kit Chan, Francois Dehez, Mrinal Shekhar, M.R. Gunner, Leonid A Sazanov, Christophe Chipot, and Abhishek Singharoy. “Movies.” American Chemical Society, 2020. <a href=\"https://doi.org/10.1021/jacs.9b13450.s002\">https://doi.org/10.1021/jacs.9b13450.s002</a>.","ieee":"C. Gupta <i>et al.</i>, “Movies.” American Chemical Society, 2020.","ista":"Gupta C, Khaniya U, Chan CK, Dehez F, Shekhar M, Gunner MR, Sazanov LA, Chipot C, Singharoy A. 2020. Movies, American Chemical Society, <a href=\"https://doi.org/10.1021/jacs.9b13450.s002\">10.1021/jacs.9b13450.s002</a>.","ama":"Gupta C, Khaniya U, Chan CK, et al. Movies. 2020. doi:<a href=\"https://doi.org/10.1021/jacs.9b13450.s002\">10.1021/jacs.9b13450.s002</a>","apa":"Gupta, C., Khaniya, U., Chan, C. K., Dehez, F., Shekhar, M., Gunner, M. R., … Singharoy, A. (2020). Movies. American Chemical Society. <a href=\"https://doi.org/10.1021/jacs.9b13450.s002\">https://doi.org/10.1021/jacs.9b13450.s002</a>","short":"C. Gupta, U. Khaniya, C.K. Chan, F. Dehez, M. Shekhar, M.R. Gunner, L.A. Sazanov, C. Chipot, A. Singharoy, (2020).","mla":"Gupta, Chitrak, et al. <i>Movies</i>. American Chemical Society, 2020, doi:<a href=\"https://doi.org/10.1021/jacs.9b13450.s002\">10.1021/jacs.9b13450.s002</a>."},"date_published":"2020-05-20T00:00:00Z","_id":"9878","status":"public","type":"research_data_reference","oa_version":"Published Version","date_created":"2021-08-11T09:18:54Z","department":[{"_id":"LeSa"}],"month":"05","related_material":{"record":[{"relation":"used_in_publication","status":"public","id":"8040"}]},"day":"20","title":"Movies","user_id":"6785fbc1-c503-11eb-8a32-93094b40e1cf","year":"2020","article_processing_charge":"No","author":[{"first_name":"Chitrak","last_name":"Gupta","full_name":"Gupta, Chitrak"},{"first_name":"Umesh","last_name":"Khaniya","full_name":"Khaniya, Umesh"},{"first_name":"Chun Kit","last_name":"Chan","full_name":"Chan, Chun Kit"},{"last_name":"Dehez","first_name":"Francois","full_name":"Dehez, Francois"},{"full_name":"Shekhar, Mrinal","last_name":"Shekhar","first_name":"Mrinal"},{"last_name":"Gunner","first_name":"M.R.","full_name":"Gunner, M.R."},{"last_name":"Sazanov","orcid":"0000-0002-0977-7989","first_name":"Leonid A","full_name":"Sazanov, Leonid A","id":"338D39FE-F248-11E8-B48F-1D18A9856A87"},{"full_name":"Chipot, Christophe","last_name":"Chipot","first_name":"Christophe"},{"first_name":"Abhishek","last_name":"Singharoy","full_name":"Singharoy, Abhishek"}]},{"article_number":"2070122","_id":"17444","date_published":"2020-04-23T00:00:00Z","quality_controlled":"1","publisher":"Wiley","doi":"10.1002/adma.202070122","publication_identifier":{"issn":["0935-9648"],"eissn":["1521-4095"]},"article_processing_charge":"No","department":[{"_id":"GeKa"}],"day":"23","oa":1,"title":"Nanowires: Site‐controlled uniform Ge/Si Hut wires with electrically tunable spin–orbit coupling (Adv. Mater. 16/2020)","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","citation":{"chicago":"Gao, Fei, Jian‐Huan Wang, Hannes Watzinger, Hao Hu, Marko J. Rančić, Jie‐Yin Zhang, Ting Wang, et al. <i>Nanowires: Site‐controlled Uniform Ge/Si Hut Wires with Electrically Tunable Spin–Orbit Coupling (Adv. Mater. 16/2020)</i>. <i>Advanced Materials</i>. Vol. 32. Wiley, 2020. <a href=\"https://doi.org/10.1002/adma.202070122\">https://doi.org/10.1002/adma.202070122</a>.","ama":"Gao F, Wang J, Watzinger H, et al. <i>Nanowires: Site‐controlled Uniform Ge/Si Hut Wires with Electrically Tunable Spin–Orbit Coupling (Adv. Mater. 16/2020)</i>. Vol 32. Wiley; 2020. doi:<a href=\"https://doi.org/10.1002/adma.202070122\">10.1002/adma.202070122</a>","ista":"Gao F, Wang J, Watzinger H, Hu H, Rančić MJ, Zhang J, Wang T, Yao Y, Wang G, Kukucka J, Vukušić L, Kloeffel C, Loss D, Liu F, Katsaros G, Zhang J. 2020. Nanowires: Site‐controlled uniform Ge/Si Hut wires with electrically tunable spin–orbit coupling (Adv. Mater. 16/2020), Wiley,p.","ieee":"F. Gao <i>et al.</i>, <i>Nanowires: Site‐controlled uniform Ge/Si Hut wires with electrically tunable spin–orbit coupling (Adv. Mater. 16/2020)</i>, vol. 32, no. 16. Wiley, 2020.","apa":"Gao, F., Wang, J., Watzinger, H., Hu, H., Rančić, M. J., Zhang, J., … Zhang, J. (2020). <i>Nanowires: Site‐controlled uniform Ge/Si Hut wires with electrically tunable spin–orbit coupling (Adv. Mater. 16/2020)</i>. <i>Advanced Materials</i> (Vol. 32). Wiley. <a href=\"https://doi.org/10.1002/adma.202070122\">https://doi.org/10.1002/adma.202070122</a>","short":"F. Gao, J. Wang, H. Watzinger, H. Hu, M.J. Rančić, J. Zhang, T. Wang, Y. Yao, G. Wang, J. Kukucka, L. Vukušić, C. Kloeffel, D. Loss, F. Liu, G. Katsaros, J. Zhang, Nanowires: Site‐controlled Uniform Ge/Si Hut Wires with Electrically Tunable Spin–Orbit Coupling (Adv. Mater. 16/2020), Wiley, 2020.","mla":"Gao, Fei, et al. “Nanowires: Site‐controlled Uniform Ge/Si Hut Wires with Electrically Tunable Spin–Orbit Coupling (Adv. Mater. 16/2020).” <i>Advanced Materials</i>, vol. 32, no. 16, 2070122, Wiley, 2020, doi:<a href=\"https://doi.org/10.1002/adma.202070122\">10.1002/adma.202070122</a>."},"language":[{"iso":"eng"}],"abstract":[{"text":"The first wafer-scale growth of site-controlled Ge/Si nanowires is reported by Georgios Katsaros, Jian-Jun Zhang, and co-workers in article number 1906523. They are highly uniform and their position, distance, length, and even square- or L-shaped structures can all be precisely controlled. The electrically tunable spin-orbit coupling demonstrated by transport measurements and the charge sensing between quantum dots in closely spaced wires open a path toward scalable qubit devices using nanowires on silicon.","lang":"eng"}],"status":"public","date_created":"2024-08-20T08:22:42Z","publication":"Advanced Materials","oa_version":"Published Version","type":"other_academic_publication","main_file_link":[{"url":"https://doi.org/10.1002/adma.202070122","open_access":"1"}],"date_updated":"2026-06-18T17:54:47Z","ddc":["530"],"intvolume":"        32","author":[{"first_name":"Fei","last_name":"Gao","full_name":"Gao, Fei"},{"first_name":"Jian‐Huan","last_name":"Wang","full_name":"Wang, Jian‐Huan"},{"last_name":"Watzinger","first_name":"Hannes","full_name":"Watzinger, Hannes","id":"35DF8E50-F248-11E8-B48F-1D18A9856A87"},{"full_name":"Hu, Hao","first_name":"Hao","last_name":"Hu"},{"full_name":"Rančić, Marko J.","first_name":"Marko J.","last_name":"Rančić"},{"full_name":"Zhang, Jie‐Yin","first_name":"Jie‐Yin","last_name":"Zhang"},{"first_name":"Ting","last_name":"Wang","full_name":"Wang, Ting"},{"full_name":"Yao, Yuan","first_name":"Yuan","last_name":"Yao"},{"last_name":"Wang","first_name":"Gui‐Lei","full_name":"Wang, Gui‐Lei"},{"first_name":"Josip","last_name":"Kukucka","id":"3F5D8856-F248-11E8-B48F-1D18A9856A87","full_name":"Kukucka, Josip"},{"id":"31E9F056-F248-11E8-B48F-1D18A9856A87","full_name":"Vukušić, Lada","first_name":"Lada","orcid":"0000-0003-2424-8636","last_name":"Vukušić"},{"full_name":"Kloeffel, Christoph","last_name":"Kloeffel","first_name":"Christoph"},{"full_name":"Loss, Daniel","first_name":"Daniel","last_name":"Loss"},{"last_name":"Liu","first_name":"Feng","full_name":"Liu, Feng"},{"last_name":"Katsaros","orcid":"0000-0001-8342-202X","first_name":"Georgios","full_name":"Katsaros, Georgios","id":"38DB5788-F248-11E8-B48F-1D18A9856A87"},{"first_name":"Jian‐Jun","last_name":"Zhang","full_name":"Zhang, Jian‐Jun"}],"month":"04","issue":"16","related_material":{"record":[{"id":"7541","status":"public","relation":"other"}]},"volume":32,"publication_status":"published","year":"2020"},{"date_updated":"2024-09-11T08:08:21Z","intvolume":"       495","citation":{"chicago":"Xin, Chengcheng, Maria Charisi, Zoltán Haiman, and David Schiminovich. “Correlation between Optical and UV Variability of a Large Sample of Quasars.” <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press, 2020. <a href=\"https://doi.org/10.1093/mnras/staa1258\">https://doi.org/10.1093/mnras/staa1258</a>.","ista":"Xin C, Charisi M, Haiman Z, Schiminovich D. 2020. Correlation between optical and UV variability of a large sample of quasars. Monthly Notices of the Royal Astronomical Society. 495(1), 1403–1413.","ieee":"C. Xin, M. Charisi, Z. Haiman, and D. Schiminovich, “Correlation between optical and UV variability of a large sample of quasars,” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 495, no. 1. Oxford University Press, pp. 1403–1413, 2020.","ama":"Xin C, Charisi M, Haiman Z, Schiminovich D. Correlation between optical and UV variability of a large sample of quasars. <i>Monthly Notices of the Royal Astronomical Society</i>. 2020;495(1):1403-1413. doi:<a href=\"https://doi.org/10.1093/mnras/staa1258\">10.1093/mnras/staa1258</a>","apa":"Xin, C., Charisi, M., Haiman, Z., &#38; Schiminovich, D. (2020). Correlation between optical and UV variability of a large sample of quasars. <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press. <a href=\"https://doi.org/10.1093/mnras/staa1258\">https://doi.org/10.1093/mnras/staa1258</a>","short":"C. Xin, M. Charisi, Z. Haiman, D. Schiminovich, Monthly Notices of the Royal Astronomical Society 495 (2020) 1403–1413.","mla":"Xin, Chengcheng, et al. “Correlation between Optical and UV Variability of a Large Sample of Quasars.” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 495, no. 1, Oxford University Press, 2020, pp. 1403–13, doi:<a href=\"https://doi.org/10.1093/mnras/staa1258\">10.1093/mnras/staa1258</a>."},"article_type":"original","language":[{"iso":"eng"}],"abstract":[{"lang":"eng","text":"The variability of quasars across multiple wavelengths is a useful probe of physical conditions in active galactic nuclei. In particular, variable accretion rates, instabilities, and reverberation effects in the accretion disc of a supermassive black hole are expected to produce correlated flux variations in ultraviolet (UV) and optical bands. Recent work has further argued that binary quasars should exhibit strongly correlated UV and optical periodicities. Strong UV–optical correlations have indeed been established in small samples of (N ≲ 30) quasars with well-sampled light curves, and have extended the ‘bluer-when-brighter’ trend previously found within the optical bands. Here, we further test the nature of quasar variability by examining the observed-frame UV–optical correlations among bright quasars extracted from the Half Million Quasars (HMQ) catalogue. We identified a large sample of 1315 quasars in HMQ with overlapping UV and optical light curves from the Galaxy Evolution Explorer and the Catalina Real-time Transient Survey, respectively. We find that strong correlations exist in this much larger sample, but we rule out, at ∼95 per cent confidence, the simple hypothesis that the intrinsic UV and optical variations of all quasars are fully correlated. Our results therefore imply the existence of physical mechanism(s) that can generate uncorrelated optical and UV flux variations."}],"status":"public","scopus_import":"1","publication":"Monthly Notices of the Royal Astronomical Society","date_created":"2024-09-05T09:27:32Z","oa_version":"Published Version","type":"journal_article","main_file_link":[{"url":"https://doi.org/10.1093/mnras/staa1258","open_access":"1"}],"month":"05","issue":"1","volume":495,"publication_status":"published","year":"2020","page":"1403-1413","author":[{"last_name":"Xin","first_name":"Chengcheng","full_name":"Xin, Chengcheng"},{"full_name":"Charisi, Maria","first_name":"Maria","last_name":"Charisi"},{"last_name":"Haiman","first_name":"Zoltán","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","full_name":"Haiman, Zoltán"},{"full_name":"Schiminovich, David","first_name":"David","last_name":"Schiminovich"}],"publisher":"Oxford University Press","doi":"10.1093/mnras/staa1258","extern":"1","date_published":"2020-05-07T00:00:00Z","_id":"17524","quality_controlled":"1","day":"07","oa":1,"title":"Correlation between optical and UV variability of a large sample of quasars","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","publication_identifier":{"issn":["0035-8711","1365-2966"]},"article_processing_charge":"No"},{"author":[{"full_name":"Matilla, José Manuel Zorrilla","last_name":"Matilla","first_name":"José Manuel Zorrilla"},{"last_name":"Waterval","first_name":"Stefan","full_name":"Waterval, Stefan"},{"first_name":"Zoltán","last_name":"Haiman","full_name":"Haiman, Zoltán","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36"}],"month":"05","issue":"6","volume":159,"publication_status":"published","year":"2020","article_type":"original","citation":{"chicago":"Matilla, José Manuel Zorrilla, Stefan Waterval, and Zoltán Haiman. “Optimizing Simulation Parameters for Weak Lensing Analyses Involving Non-Gaussian Observables.” <i>The Astronomical Journal</i>. American Astronomical Society, 2020. <a href=\"https://doi.org/10.3847/1538-3881/ab8f8c\">https://doi.org/10.3847/1538-3881/ab8f8c</a>.","mla":"Matilla, José Manuel Zorrilla, et al. “Optimizing Simulation Parameters for Weak Lensing Analyses Involving Non-Gaussian Observables.” <i>The Astronomical Journal</i>, vol. 159, no. 6, 284, American Astronomical Society, 2020, doi:<a href=\"https://doi.org/10.3847/1538-3881/ab8f8c\">10.3847/1538-3881/ab8f8c</a>.","short":"J.M.Z. Matilla, S. Waterval, Z. Haiman, The Astronomical Journal 159 (2020).","apa":"Matilla, J. M. Z., Waterval, S., &#38; Haiman, Z. (2020). Optimizing simulation parameters for weak lensing analyses involving non-Gaussian observables. <i>The Astronomical Journal</i>. American Astronomical Society. <a href=\"https://doi.org/10.3847/1538-3881/ab8f8c\">https://doi.org/10.3847/1538-3881/ab8f8c</a>","ama":"Matilla JMZ, Waterval S, Haiman Z. Optimizing simulation parameters for weak lensing analyses involving non-Gaussian observables. <i>The Astronomical Journal</i>. 2020;159(6). doi:<a href=\"https://doi.org/10.3847/1538-3881/ab8f8c\">10.3847/1538-3881/ab8f8c</a>","ista":"Matilla JMZ, Waterval S, Haiman Z. 2020. Optimizing simulation parameters for weak lensing analyses involving non-Gaussian observables. The Astronomical Journal. 159(6), 284.","ieee":"J. M. Z. Matilla, S. Waterval, and Z. Haiman, “Optimizing simulation parameters for weak lensing analyses involving non-Gaussian observables,” <i>The Astronomical Journal</i>, vol. 159, no. 6. American Astronomical Society, 2020."},"language":[{"iso":"eng"}],"abstract":[{"lang":"eng","text":"We performed a series of numerical experiments to quantify the sensitivity of the predictions for weak lensing statistics obtained in ray-tracing dark matter (DM)-only simulations, to two hyper-parameters that influence the accuracy as well as the computational cost of the predictions: the thickness of the lens planes used to build past light cones and the mass resolution of the underlying DM simulation. The statistics considered are the power spectrum (PS) and a series of non-Gaussian observables, including the one-point probability density function, lensing peaks, and Minkowski functionals. Counterintuitively, we find that using thin lens planes (< 60 h−1 Mpc on a 240 h−1 Mpc simulation box) suppresses the PS over a broad range of scales beyond what would be acceptable for a survey comparable to the Large Synoptic Survey Telescope (LSST). A mass resolution of 7.2 × 1011 h−1 M⊙ per DM particle (or 2563 particles in a (240 h−1 Mpc)3 box) is sufficient to extract information using the PS and non-Gaussian statistics from weak lensing data at angular scales down to 1' with LSST-like levels of shape noise."}],"status":"public","date_created":"2024-09-05T09:35:49Z","scopus_import":"1","oa_version":"Published Version","publication":"The Astronomical Journal","type":"journal_article","main_file_link":[{"open_access":"1","url":"https://doi.org/10.3847/1538-3881/ab8f8c"}],"date_updated":"2024-09-11T09:03:15Z","intvolume":"       159","publication_identifier":{"issn":["0004-6256","1538-3881"]},"article_processing_charge":"No","day":"29","oa":1,"title":"Optimizing simulation parameters for weak lensing analyses involving non-Gaussian observables","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","article_number":"284","_id":"17528","date_published":"2020-05-29T00:00:00Z","quality_controlled":"1","publisher":"American Astronomical Society","doi":"10.3847/1538-3881/ab8f8c","extern":"1"},{"extern":"1","doi":"10.3847/1538-4357/aba2cc","publisher":"American Astronomical Society","_id":"17529","quality_controlled":"1","date_published":"2020-08-10T00:00:00Z","article_number":"26","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","oa":1,"title":"Spin evolution of stellar-mass black hole binaries in active galactic nuclei","day":"10","article_processing_charge":"No","publication_identifier":{"issn":["0004-637X","1538-4357"]},"intvolume":"       899","date_updated":"2024-09-11T09:11:55Z","date_created":"2024-09-05T09:36:37Z","publication":"The Astrophysical Journal","scopus_import":"1","oa_version":"Published Version","main_file_link":[{"url":"https://doi.org/10.3847/1538-4357/aba2cc","open_access":"1"}],"type":"journal_article","abstract":[{"text":"The astrophysical origin of gravitational wave (GW) events is one of the most timely problems in the wake of the LIGO/Virgo discoveries. In active galactic nuclei (AGN), binaries form and evolve efficiently by dynamical interactions and gaseous dissipation. Previous studies have suggested that binary black hole (BBH) mergers in AGN disks can contribute significantly to BBH mergers observed by GW interferometers. Here we examine the distribution of the effective spin parameter χeff of this GW source population. We extend our semi-analytical model of binary formation and evolution in AGN disks by following the evolution of the binary orbital angular momenta and black hole (BH) spins. BH spins change due to gas accretion and BH mergers, while the binary orbital angular momenta evolve due to gas accretion and binary-single interactions. We find that the distribution of χeff predicted by our AGN model is similar to the distribution observed during LIGO/Virgo O1 and O2. On the other hand, if radial migration of BHs is inefficient, χeff is skewed toward higher values compared with the observed distribution, because of the paucity of scattering events that would randomize spin directions relative to the orbital plane. We suggest that high binary masses and the positive correlation between binary mass and the standard deviation of χeff for chirp masses up to ≈20 M⊙, can be possible signatures for mergers originating in AGN disks. Finally, hierarchical mergers in AGN disks naturally produce properties of the recent GW event GW190412, including a low mass ratio, a high primary BH spin, and a significant spin component in the orbital plane.","lang":"eng"}],"status":"public","citation":{"mla":"Tagawa, Hiromichi, et al. “Spin Evolution of Stellar-Mass Black Hole Binaries in Active Galactic Nuclei.” <i>The Astrophysical Journal</i>, vol. 899, no. 1, 26, American Astronomical Society, 2020, doi:<a href=\"https://doi.org/10.3847/1538-4357/aba2cc\">10.3847/1538-4357/aba2cc</a>.","short":"H. Tagawa, Z. Haiman, I. Bartos, B. Kocsis, The Astrophysical Journal 899 (2020).","apa":"Tagawa, H., Haiman, Z., Bartos, I., &#38; Kocsis, B. (2020). Spin evolution of stellar-mass black hole binaries in active galactic nuclei. <i>The Astrophysical Journal</i>. American Astronomical Society. <a href=\"https://doi.org/10.3847/1538-4357/aba2cc\">https://doi.org/10.3847/1538-4357/aba2cc</a>","ista":"Tagawa H, Haiman Z, Bartos I, Kocsis B. 2020. Spin evolution of stellar-mass black hole binaries in active galactic nuclei. The Astrophysical Journal. 899(1), 26.","ama":"Tagawa H, Haiman Z, Bartos I, Kocsis B. Spin evolution of stellar-mass black hole binaries in active galactic nuclei. <i>The Astrophysical Journal</i>. 2020;899(1). doi:<a href=\"https://doi.org/10.3847/1538-4357/aba2cc\">10.3847/1538-4357/aba2cc</a>","ieee":"H. Tagawa, Z. Haiman, I. Bartos, and B. Kocsis, “Spin evolution of stellar-mass black hole binaries in active galactic nuclei,” <i>The Astrophysical Journal</i>, vol. 899, no. 1. American Astronomical Society, 2020.","chicago":"Tagawa, Hiromichi, Zoltán Haiman, Imre Bartos, and Bence Kocsis. “Spin Evolution of Stellar-Mass Black Hole Binaries in Active Galactic Nuclei.” <i>The Astrophysical Journal</i>. American Astronomical Society, 2020. <a href=\"https://doi.org/10.3847/1538-4357/aba2cc\">https://doi.org/10.3847/1538-4357/aba2cc</a>."},"article_type":"original","language":[{"iso":"eng"}],"year":"2020","publication_status":"published","issue":"1","volume":899,"month":"08","author":[{"full_name":"Tagawa, Hiromichi","last_name":"Tagawa","first_name":"Hiromichi"},{"full_name":"Haiman, Zoltán","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","last_name":"Haiman","first_name":"Zoltán"},{"last_name":"Bartos","first_name":"Imre","full_name":"Bartos, Imre"},{"last_name":"Kocsis","first_name":"Bence","full_name":"Kocsis, Bence"}]},{"publication_identifier":{"issn":["2041-8205","2041-8213"]},"article_processing_charge":"No","day":"02","title":"Formation of GW190521 via gas accretion onto population III stellar black hole remnants born in high-redshift minihalos","oa":1,"user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","article_number":"L21","quality_controlled":"1","_id":"17537","date_published":"2020-11-02T00:00:00Z","publisher":"American Astronomical Society","doi":"10.3847/2041-8213/abc253","extern":"1","author":[{"last_name":"Safarzadeh","first_name":"Mohammadtaher","full_name":"Safarzadeh, Mohammadtaher"},{"id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","full_name":"Haiman, Zoltán","first_name":"Zoltán","last_name":"Haiman"}],"month":"11","volume":903,"issue":"1","publication_status":"published","year":"2020","language":[{"iso":"eng"}],"article_type":"original","citation":{"apa":"Safarzadeh, M., &#38; Haiman, Z. (2020). Formation of GW190521 via gas accretion onto population III stellar black hole remnants born in high-redshift minihalos. <i>The Astrophysical Journal Letters</i>. American Astronomical Society. <a href=\"https://doi.org/10.3847/2041-8213/abc253\">https://doi.org/10.3847/2041-8213/abc253</a>","ieee":"M. Safarzadeh and Z. Haiman, “Formation of GW190521 via gas accretion onto population III stellar black hole remnants born in high-redshift minihalos,” <i>The Astrophysical Journal Letters</i>, vol. 903, no. 1. American Astronomical Society, 2020.","ama":"Safarzadeh M, Haiman Z. Formation of GW190521 via gas accretion onto population III stellar black hole remnants born in high-redshift minihalos. <i>The Astrophysical Journal Letters</i>. 2020;903(1). doi:<a href=\"https://doi.org/10.3847/2041-8213/abc253\">10.3847/2041-8213/abc253</a>","ista":"Safarzadeh M, Haiman Z. 2020. Formation of GW190521 via gas accretion onto population III stellar black hole remnants born in high-redshift minihalos. The Astrophysical Journal Letters. 903(1), L21.","mla":"Safarzadeh, Mohammadtaher, and Zoltán Haiman. “Formation of GW190521 via Gas Accretion onto Population III Stellar Black Hole Remnants Born in High-Redshift Minihalos.” <i>The Astrophysical Journal Letters</i>, vol. 903, no. 1, L21, American Astronomical Society, 2020, doi:<a href=\"https://doi.org/10.3847/2041-8213/abc253\">10.3847/2041-8213/abc253</a>.","short":"M. Safarzadeh, Z. Haiman, The Astrophysical Journal Letters 903 (2020).","chicago":"Safarzadeh, Mohammadtaher, and Zoltán Haiman. “Formation of GW190521 via Gas Accretion onto Population III Stellar Black Hole Remnants Born in High-Redshift Minihalos.” <i>The Astrophysical Journal Letters</i>. American Astronomical Society, 2020. <a href=\"https://doi.org/10.3847/2041-8213/abc253\">https://doi.org/10.3847/2041-8213/abc253</a>."},"status":"public","abstract":[{"text":"The recent gravitational wave merger event, GW190521, has challenged our understanding of the stellar-mass black hole (BH) formation. The primary and secondary BH are both inferred to fall inside the pair-instability (PI) mass gap. Here we propose that the formation of such binaries is possible through gas accretion onto the BH remnants of Population III (Pop~III) stars born in high-redshift (z>10) minihalos. Once the parent halo has grown to the atomic-cooling limit, even brief episodes of gas accretion in the dense central regions of the halo can increase the masses of Pop~III remnant BHs above the PI limit. Starting with a BBH with an initial mass of O(100) M⊙ we find that it would only need to spend about 100~Myr in the inner few pc of an atomic-cooling halo to accrete about 50~M⊙ of material and resemble a system similar to GW190521. The dynamical friction timescale for the binary to sink to the dense inner region of its parent halo is comparable or shorter than the accretion timescale required to increase their mass above the PI limit. Once in the core of the halo, the binary can enter a phase of hyper-Eddington accretion, where it would only take a few thousand years to exceed the PI limit through accretion. Even more massive BBHs could form through this channel, and be detectable by detectors with improved low-frequency sensitivity. Single Pop~III BH remnants would also grow through accretion and could later form binaries dynamically. As little as a few percent of Pop~III BH remnants may be sufficient to match the rate of massive BBH mergers inferred from GW190521 of 0.13+0.3−0.11Gpc−3yr−1.","lang":"eng"}],"type":"journal_article","main_file_link":[{"open_access":"1","url":"https://doi.org/10.3847/2041-8213/abc253"}],"scopus_import":"1","oa_version":"Published Version","date_created":"2024-09-05T09:50:29Z","publication":"The Astrophysical Journal Letters","date_updated":"2024-09-12T09:33:05Z","intvolume":"       903"},{"intvolume":"       499","date_updated":"2024-09-12T09:39:27Z","citation":{"chicago":"Sakurai, Yuya, Zoltán Haiman, and Kohei Inayoshi. “Radiative Feedback for Supermassive Star Formation in a Massive Cloud with H2 Molecules in an Atomic-Cooling Halo.” <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press, 2020. <a href=\"https://doi.org/10.1093/mnras/staa3227\">https://doi.org/10.1093/mnras/staa3227</a>.","mla":"Sakurai, Yuya, et al. “Radiative Feedback for Supermassive Star Formation in a Massive Cloud with H2 Molecules in an Atomic-Cooling Halo.” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 499, no. 4, Oxford University Press, 2020, pp. 5960–71, doi:<a href=\"https://doi.org/10.1093/mnras/staa3227\">10.1093/mnras/staa3227</a>.","short":"Y. Sakurai, Z. Haiman, K. Inayoshi, Monthly Notices of the Royal Astronomical Society 499 (2020) 5960–5971.","apa":"Sakurai, Y., Haiman, Z., &#38; Inayoshi, K. (2020). Radiative feedback for supermassive star formation in a massive cloud with H2 molecules in an atomic-cooling halo. <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press. <a href=\"https://doi.org/10.1093/mnras/staa3227\">https://doi.org/10.1093/mnras/staa3227</a>","ista":"Sakurai Y, Haiman Z, Inayoshi K. 2020. Radiative feedback for supermassive star formation in a massive cloud with H2 molecules in an atomic-cooling halo. Monthly Notices of the Royal Astronomical Society. 499(4), 5960–5971.","ieee":"Y. Sakurai, Z. Haiman, and K. Inayoshi, “Radiative feedback for supermassive star formation in a massive cloud with H2 molecules in an atomic-cooling halo,” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 499, no. 4. Oxford University Press, pp. 5960–5971, 2020.","ama":"Sakurai Y, Haiman Z, Inayoshi K. Radiative feedback for supermassive star formation in a massive cloud with H2 molecules in an atomic-cooling halo. <i>Monthly Notices of the Royal Astronomical Society</i>. 2020;499(4):5960-5971. doi:<a href=\"https://doi.org/10.1093/mnras/staa3227\">10.1093/mnras/staa3227</a>"},"article_type":"original","language":[{"iso":"eng"}],"date_created":"2024-09-05T09:51:17Z","publication":"Monthly Notices of the Royal Astronomical Society","oa_version":"Published Version","scopus_import":"1","type":"journal_article","main_file_link":[{"url":"https://doi.org/10.1093/mnras/staa3227","open_access":"1"}],"abstract":[{"lang":"eng","text":"Recent three-dimensional cosmological simulations of protogalaxy formation have suggested that supermassive stars (SMSs) can form in gas clouds in which H2 cooling is suppressed by dynamical heating prior to the activation of atomic cooling (Wise et al. 2019), but they stopped short of the following growth of a central protostar. Here we examine whether accretion on the protostellar core in this cloud is sufficiently rapid, in the face of the radiation feedback, to produce a SMS. We perform one-dimensional radiation-hydrodynamical simulations of the hot collapsing cloud with non-equilibrium chemical reactions directly adopting the cloud properties from Wise et al. (2019) as an initial condition. We find that the stellar Lyman-Werner (LW) radiation from the SMS dissociates H2 in the inner regions of the gas flow, increasing gas temperature and thermal pressure, and temporarily stopping the accretion. However, this negative feedback ceases when the self-gravity and inward ram pressure force on larger scales push the gas inward. The central protostar is unable to expand an HII region due to the high density, and grows to a mass of ≳105M⊙. Our results suggests the successful formation of SMSs, and resulting massive (∼105M⊙) remnant black holes in the clouds, but need to be confirmed in two- or three-dimensional simulations."}],"status":"public","issue":"4","volume":499,"month":"10","year":"2020","publication_status":"published","page":"5960-5971","author":[{"last_name":"Sakurai","first_name":"Yuya","full_name":"Sakurai, Yuya"},{"first_name":"Zoltán","last_name":"Haiman","full_name":"Haiman, Zoltán","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36"},{"last_name":"Inayoshi","first_name":"Kohei","full_name":"Inayoshi, Kohei"}],"doi":"10.1093/mnras/staa3227","publisher":"Oxford University Press","extern":"1","date_published":"2020-10-17T00:00:00Z","_id":"17538","quality_controlled":"1","day":"17","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","oa":1,"title":"Radiative feedback for supermassive star formation in a massive cloud with H2 molecules in an atomic-cooling halo","article_processing_charge":"No","publication_identifier":{"issn":["0035-8711","1365-2966"]}},{"publication_identifier":{"issn":["0035-8711","1365-2966"]},"article_processing_charge":"No","title":"Evolution of gas disc–embedded intermediate mass ratio inspirals in the LISA band","oa":1,"user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","day":"29","date_published":"2020-12-29T00:00:00Z","_id":"17540","quality_controlled":"1","extern":"1","publisher":"Oxford University Press","doi":"10.1093/mnras/staa3976","author":[{"first_name":"A","last_name":"Derdzinski","full_name":"Derdzinski, A"},{"last_name":"D’Orazio","first_name":"D","full_name":"D’Orazio, D"},{"first_name":"P","last_name":"Duffell","full_name":"Duffell, P"},{"last_name":"Haiman","first_name":"Zoltán","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","full_name":"Haiman, Zoltán"},{"full_name":"MacFadyen, A","first_name":"A","last_name":"MacFadyen"}],"page":"3540-3557","publication_status":"published","year":"2020","month":"12","volume":501,"issue":"3","status":"public","abstract":[{"text":"Among the potential milliHz gravitational wave (GW) sources for the upcoming space-based interferometer LISA are extreme- or intermediate-mass ratio inspirals (EMRI/IMRIs). These events involve the coalescence of supermassive black holes in the mass range 105M⊙≲M≲107M⊙ with companion BHs of much lower masses. A subset of E/IMRIs are expected to occur in the accretion discs of active galactic nuclei (AGN), where torques exerted by the disc can interfere with the inspiral and cause a phase shift in the GW waveform. Here we use a suite of two-dimensional hydrodynamical simulations with the moving-mesh code DISCO to present a systematic study of disc torques. We measure torques on an inspiraling BH and compute the corresponding waveform deviations as a function of the binary mass ratio q≡M2/M1, the disc viscosity (α), and gas temperature (or equivalently Mach number; M). We find that the absolute value of the gas torques is within an order of magnitude of previously determined planetary migration torques, but their precise value and sign depends non-trivially on the combination of these parameters. The gas imprint is detectable by LISA for binaries embedded in AGN discs with surface densities above Σ0≥104−6gcm−2, depending on q, α and M. Deviations are most pronounced in discs with higher viscosities, and for E/IMRIs detected at frequencies where LISA is most sensitive. Torques in colder discs exhibit a noticeable dependence on the GW-driven inspiral rate as well as strong fluctuations at late stages of the inspiral. Our results further suggest that LISA may be able to place constraints on AGN disc parameters and the physics of disc-satellite interaction.","lang":"eng"}],"type":"journal_article","main_file_link":[{"url":"https://doi.org/10.1093/mnras/staa3976","open_access":"1"}],"oa_version":"Published Version","scopus_import":"1","date_created":"2024-09-05T09:55:24Z","publication":"Monthly Notices of the Royal Astronomical Society","language":[{"iso":"eng"}],"article_type":"original","citation":{"chicago":"Derdzinski, A, D D’Orazio, P Duffell, Zoltán Haiman, and A MacFadyen. “Evolution of Gas Disc–Embedded Intermediate Mass Ratio Inspirals in the LISA Band.” <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press, 2020. <a href=\"https://doi.org/10.1093/mnras/staa3976\">https://doi.org/10.1093/mnras/staa3976</a>.","apa":"Derdzinski, A., D’Orazio, D., Duffell, P., Haiman, Z., &#38; MacFadyen, A. (2020). Evolution of gas disc–embedded intermediate mass ratio inspirals in the LISA band. <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press. <a href=\"https://doi.org/10.1093/mnras/staa3976\">https://doi.org/10.1093/mnras/staa3976</a>","ista":"Derdzinski A, D’Orazio D, Duffell P, Haiman Z, MacFadyen A. 2020. Evolution of gas disc–embedded intermediate mass ratio inspirals in the LISA band. Monthly Notices of the Royal Astronomical Society. 501(3), 3540–3557.","ama":"Derdzinski A, D’Orazio D, Duffell P, Haiman Z, MacFadyen A. Evolution of gas disc–embedded intermediate mass ratio inspirals in the LISA band. <i>Monthly Notices of the Royal Astronomical Society</i>. 2020;501(3):3540-3557. doi:<a href=\"https://doi.org/10.1093/mnras/staa3976\">10.1093/mnras/staa3976</a>","ieee":"A. Derdzinski, D. D’Orazio, P. Duffell, Z. Haiman, and A. MacFadyen, “Evolution of gas disc–embedded intermediate mass ratio inspirals in the LISA band,” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 501, no. 3. Oxford University Press, pp. 3540–3557, 2020.","mla":"Derdzinski, A., et al. “Evolution of Gas Disc–Embedded Intermediate Mass Ratio Inspirals in the LISA Band.” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 501, no. 3, Oxford University Press, 2020, pp. 3540–57, doi:<a href=\"https://doi.org/10.1093/mnras/staa3976\">10.1093/mnras/staa3976</a>.","short":"A. Derdzinski, D. D’Orazio, P. Duffell, Z. Haiman, A. MacFadyen, Monthly Notices of the Royal Astronomical Society 501 (2020) 3540–3557."},"date_updated":"2024-09-12T09:54:26Z","intvolume":"       501"},{"publication_status":"published","year":"2020","month":"07","volume":897,"issue":"1","author":[{"full_name":"Visbal, Eli","last_name":"Visbal","first_name":"Eli"},{"first_name":"Greg L.","last_name":"Bryan","full_name":"Bryan, Greg L."},{"full_name":"Haiman, Zoltán","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","last_name":"Haiman","first_name":"Zoltán"}],"arxiv":1,"date_updated":"2024-09-12T13:28:25Z","intvolume":"       897","external_id":{"arxiv":["2001.11118"]},"status":"public","abstract":[{"lang":"eng","text":"We present a new semianalytic model of the formation of the first stars. Our method takes dark matter halo merger trees (including three-dimensional spatial information) from cosmological N-body simulations as input and applies analytic prescriptions to compute both the Population III and metal-enriched star formation histories. We have developed a novel method to accurately compute the major feedback processes affecting Population III star formation: H2 photodissociation from Lyman–Werner (LW) radiation, suppression of star formation due to inhomogeneous reionization, and metal enrichment via supernova winds. Our method utilizes a grid-based approach relying on fast Fourier transforms to rapidly track the LW intensity, ionization fraction, and metallicity in three dimensions throughout the simulation box. We present simulations for a wide range of astrophysical model parameters from z ≈ 30 to 6. Initially long-range LW feedback and local metal enrichment and reionization feedback dominate. However, for z ≲ 15 we find that the star formation rate density (SFRD) of Population III stars is impacted by the combination of external metal enrichment (metals from one halo polluting other pristine halos) and inhomogeneous reionization. We find that the interplay of these processes is particularly important for the Population III SFRD at z ≲ 10. Reionization feedback delays star formation long enough for metal bubbles to reach halos that would otherwise form Population III stars. Including these effects can lead to more than an order-of-magnitude decrease in the Population III SFRD at z = 6 compared to LW feedback alone."}],"type":"journal_article","main_file_link":[{"url":" https://doi.org/10.48550/arXiv.2001.11118","open_access":"1"}],"date_created":"2024-09-05T09:58:26Z","publication":"The Astrophysical Journal","scopus_import":"1","oa_version":"Preprint","language":[{"iso":"eng"}],"citation":{"ista":"Visbal E, Bryan GL, Haiman Z. 2020. Self-consistent semianalytic modeling of feedback during primordial star formation and reionization. The Astrophysical Journal. 897(1), 95.","ieee":"E. Visbal, G. L. Bryan, and Z. Haiman, “Self-consistent semianalytic modeling of feedback during primordial star formation and reionization,” <i>The Astrophysical Journal</i>, vol. 897, no. 1. American Astronomical Society, 2020.","ama":"Visbal E, Bryan GL, Haiman Z. Self-consistent semianalytic modeling of feedback during primordial star formation and reionization. <i>The Astrophysical Journal</i>. 2020;897(1). doi:<a href=\"https://doi.org/10.3847/1538-4357/ab994e\">10.3847/1538-4357/ab994e</a>","apa":"Visbal, E., Bryan, G. L., &#38; Haiman, Z. (2020). Self-consistent semianalytic modeling of feedback during primordial star formation and reionization. <i>The Astrophysical Journal</i>. American Astronomical Society. <a href=\"https://doi.org/10.3847/1538-4357/ab994e\">https://doi.org/10.3847/1538-4357/ab994e</a>","short":"E. Visbal, G.L. Bryan, Z. Haiman, The Astrophysical Journal 897 (2020).","mla":"Visbal, Eli, et al. “Self-Consistent Semianalytic Modeling of Feedback during Primordial Star Formation and Reionization.” <i>The Astrophysical Journal</i>, vol. 897, no. 1, 95, American Astronomical Society, 2020, doi:<a href=\"https://doi.org/10.3847/1538-4357/ab994e\">10.3847/1538-4357/ab994e</a>.","chicago":"Visbal, Eli, Greg L. Bryan, and Zoltán Haiman. “Self-Consistent Semianalytic Modeling of Feedback during Primordial Star Formation and Reionization.” <i>The Astrophysical Journal</i>. American Astronomical Society, 2020. <a href=\"https://doi.org/10.3847/1538-4357/ab994e\">https://doi.org/10.3847/1538-4357/ab994e</a>."},"article_type":"original","title":"Self-consistent semianalytic modeling of feedback during primordial star formation and reionization","oa":1,"user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","day":"07","publication_identifier":{"issn":["0004-637X","1538-4357"]},"article_processing_charge":"No","extern":"1","publisher":"American Astronomical Society","doi":"10.3847/1538-4357/ab994e","article_number":"95","_id":"17542","quality_controlled":"1","date_published":"2020-07-07T00:00:00Z"},{"publication_status":"published","year":"2020","month":"05","issue":"4","volume":495,"author":[{"last_name":"Hu","first_name":"Betty X","full_name":"Hu, Betty X"},{"last_name":"D’Orazio","first_name":"Daniel J","full_name":"D’Orazio, Daniel J"},{"first_name":"Zoltán","last_name":"Haiman","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","full_name":"Haiman, Zoltán"},{"full_name":"Smith, Krista Lynne","first_name":"Krista Lynne","last_name":"Smith"},{"full_name":"Snios, Bradford","first_name":"Bradford","last_name":"Snios"},{"last_name":"Charisi","first_name":"Maria","full_name":"Charisi, Maria"},{"full_name":"Di Stefano, Rosanne","last_name":"Di Stefano","first_name":"Rosanne"}],"page":"4061-4070","date_updated":"2024-09-18T10:14:15Z","intvolume":"       495","abstract":[{"lang":"eng","text":"We examine the light curves of two quasars, motivated by recent suggestions that a supermassive black hole binary (SMBHB) can exhibit sharp lensing spikes. We model the variability of each light curve as due to a combination of two relativistic effects: the orbital relativistic Doppler boost and gravitational binary self-lensing. In order to model each system we extend previous Doppler plus self-lensing models to include eccentricity. The first quasar is identified in optical data as a binary candidate with a 20-yr period (Ark 120), and shows a prominent spike. For this source, we rule out the lensing hypothesis and disfavor the Doppler-boost hypothesis due to discrepancies in the measured vs. recovered values of the binary mass and optical spectral slope. The second source, which we nickname Spikey, is the rare case of an active galactic nucleus (AGN) identified in Kepler's high-quality, high-cadence photometric data. For this source, we find a model, consisting of a combination of a Doppler modulation and a narrow symmetric lensing spike, consistent with an eccentric SMBHB with a total mass of approximately 30 million solar masses, rest-frame orbital period T=418 days, eccentricity e=0.5, and seen at an inclination of 8 degrees from edge-on. This interpretation can be tested by monitoring Spikey for periodic behavior and recurring flares in the next few years. In preparation for such monitoring we present the first X-ray observations of this object taken by the Neil Gehrels Swift observatory."}],"status":"public","scopus_import":"1","date_created":"2024-09-05T10:16:03Z","publication":"Monthly Notices of the Royal Astronomical Society","oa_version":"Published Version","main_file_link":[{"open_access":"1","url":"https://doi.org/10.1093/mnras/staa1312"}],"type":"journal_article","citation":{"short":"B.X. Hu, D.J. D’Orazio, Z. Haiman, K.L. Smith, B. Snios, M. Charisi, R. Di Stefano, Monthly Notices of the Royal Astronomical Society 495 (2020) 4061–4070.","mla":"Hu, Betty X., et al. “Spikey: Self-Lensing Flares from Eccentric SMBH Binaries.” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 495, no. 4, Oxford University Press, 2020, pp. 4061–70, doi:<a href=\"https://doi.org/10.1093/mnras/staa1312\">10.1093/mnras/staa1312</a>.","ista":"Hu BX, D’Orazio DJ, Haiman Z, Smith KL, Snios B, Charisi M, Di Stefano R. 2020. Spikey: self-lensing flares from eccentric SMBH binaries. Monthly Notices of the Royal Astronomical Society. 495(4), 4061–4070.","ieee":"B. X. Hu <i>et al.</i>, “Spikey: self-lensing flares from eccentric SMBH binaries,” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 495, no. 4. Oxford University Press, pp. 4061–4070, 2020.","ama":"Hu BX, D’Orazio DJ, Haiman Z, et al. Spikey: self-lensing flares from eccentric SMBH binaries. <i>Monthly Notices of the Royal Astronomical Society</i>. 2020;495(4):4061-4070. doi:<a href=\"https://doi.org/10.1093/mnras/staa1312\">10.1093/mnras/staa1312</a>","apa":"Hu, B. X., D’Orazio, D. J., Haiman, Z., Smith, K. L., Snios, B., Charisi, M., &#38; Di Stefano, R. (2020). Spikey: self-lensing flares from eccentric SMBH binaries. <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press. <a href=\"https://doi.org/10.1093/mnras/staa1312\">https://doi.org/10.1093/mnras/staa1312</a>","chicago":"Hu, Betty X, Daniel J D’Orazio, Zoltán Haiman, Krista Lynne Smith, Bradford Snios, Maria Charisi, and Rosanne Di Stefano. “Spikey: Self-Lensing Flares from Eccentric SMBH Binaries.” <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press, 2020. <a href=\"https://doi.org/10.1093/mnras/staa1312\">https://doi.org/10.1093/mnras/staa1312</a>."},"article_type":"original","language":[{"iso":"eng"}],"oa":1,"title":"Spikey: self-lensing flares from eccentric SMBH binaries","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","day":"11","publication_identifier":{"issn":["0035-8711","1365-2966"]},"article_processing_charge":"No","extern":"1","publisher":"Oxford University Press","doi":"10.1093/mnras/staa1312","_id":"17552","date_published":"2020-05-11T00:00:00Z","quality_controlled":"1"},{"_id":"17554","quality_controlled":"1","date_published":"2020-06-10T00:00:00Z","extern":"1","publisher":"Oxford University Press","doi":"10.1093/mnras/staa1643","publication_identifier":{"issn":["0035-8711","1365-2966"]},"article_processing_charge":"No","title":"Testing the relativistic Doppler boost hypothesis for the binary candidate quasar PG1302-102 with multiband Swift data","oa":1,"user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","day":"10","status":"public","abstract":[{"lang":"eng","text":"The bright quasar PG1302-102 has been identified as a candidate supermassive black hole binary from its near-sinusoidal optical variability. While the significance of its optical periodicity has been debated due to the stochastic variability of quasars, its multiwavelength variability in the ultraviolet (UV) and optical bands is consistent with relativistic Doppler boost caused by the orbital motion in a binary. However, this conclusion was based previously on sparse UV data that were not taken simultaneously with the optical data. Here, we report simultaneous follow-up observations of PG1302-102 with the Ultraviolet Optical Telescope on the Neil Gehrels Swift Observatory in six optical + UV bands. The additional nine Swift observations produce light curves roughly consistent with the trend under the Doppler boost hypothesis, which predicts that UV variability should track the optical, but with a ∼2.2 times higher amplitude. We perform a statistical analysis to quantitatively test this hypothesis. We find that the data are consistent with the Doppler boost hypothesis when we compare the the amplitudes in optical B-band and UV light curves. However, the ratio of UV to V-band variability is larger than expected and is consistent with the Doppler model, only if either the UV/optical spectral slopes vary, the stochastic variability makes a large contribution in the UV, or the sparse new optical data underestimate the true optical variability. We have evidence for the latter from comparison with the optical light curve from All-Sky Automated Survey for Supernovae. Additionally, the simultaneous analysis of all four bands strongly disfavours the Doppler boost model whenever Swift V band is involved. Additional, simultaneous optical + UV observations tracing out another cycle of the 5.2-yr proposed periodicity should lead to a definitive conclusion."}],"type":"journal_article","main_file_link":[{"open_access":"1","url":"https://doi.org/10.1093/mnras/staa1643"}],"date_created":"2024-09-05T10:22:00Z","publication":"Monthly Notices of the Royal Astronomical Society","scopus_import":"1","oa_version":"Published Version","language":[{"iso":"eng"}],"article_type":"original","citation":{"chicago":"Xin, Chengcheng, Maria Charisi, Zoltán Haiman, David Schiminovich, Matthew J Graham, Daniel Stern, and Daniel J D’Orazio. “Testing the Relativistic Doppler Boost Hypothesis for the Binary Candidate Quasar PG1302-102 with Multiband Swift Data.” <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press, 2020. <a href=\"https://doi.org/10.1093/mnras/staa1643\">https://doi.org/10.1093/mnras/staa1643</a>.","mla":"Xin, Chengcheng, et al. “Testing the Relativistic Doppler Boost Hypothesis for the Binary Candidate Quasar PG1302-102 with Multiband Swift Data.” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 496, no. 2, Oxford University Press, 2020, pp. 1683–96, doi:<a href=\"https://doi.org/10.1093/mnras/staa1643\">10.1093/mnras/staa1643</a>.","short":"C. Xin, M. Charisi, Z. Haiman, D. Schiminovich, M.J. Graham, D. Stern, D.J. D’Orazio, Monthly Notices of the Royal Astronomical Society 496 (2020) 1683–1696.","apa":"Xin, C., Charisi, M., Haiman, Z., Schiminovich, D., Graham, M. J., Stern, D., &#38; D’Orazio, D. J. (2020). Testing the relativistic Doppler boost hypothesis for the binary candidate quasar PG1302-102 with multiband Swift data. <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press. <a href=\"https://doi.org/10.1093/mnras/staa1643\">https://doi.org/10.1093/mnras/staa1643</a>","ama":"Xin C, Charisi M, Haiman Z, et al. Testing the relativistic Doppler boost hypothesis for the binary candidate quasar PG1302-102 with multiband Swift data. <i>Monthly Notices of the Royal Astronomical Society</i>. 2020;496(2):1683-1696. doi:<a href=\"https://doi.org/10.1093/mnras/staa1643\">10.1093/mnras/staa1643</a>","ista":"Xin C, Charisi M, Haiman Z, Schiminovich D, Graham MJ, Stern D, D’Orazio DJ. 2020. Testing the relativistic Doppler boost hypothesis for the binary candidate quasar PG1302-102 with multiband Swift data. Monthly Notices of the Royal Astronomical Society. 496(2), 1683–1696.","ieee":"C. Xin <i>et al.</i>, “Testing the relativistic Doppler boost hypothesis for the binary candidate quasar PG1302-102 with multiband Swift data,” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 496, no. 2. Oxford University Press, pp. 1683–1696, 2020."},"date_updated":"2024-09-18T10:23:02Z","intvolume":"       496","author":[{"last_name":"Xin","first_name":"Chengcheng","full_name":"Xin, Chengcheng"},{"last_name":"Charisi","first_name":"Maria","full_name":"Charisi, Maria"},{"full_name":"Haiman, Zoltán","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","first_name":"Zoltán","last_name":"Haiman"},{"last_name":"Schiminovich","first_name":"David","full_name":"Schiminovich, David"},{"full_name":"Graham, Matthew J","first_name":"Matthew J","last_name":"Graham"},{"last_name":"Stern","first_name":"Daniel","full_name":"Stern, Daniel"},{"full_name":"D’Orazio, Daniel J","last_name":"D’Orazio","first_name":"Daniel J"}],"page":"1683-1696","publication_status":"published","year":"2020","month":"06","volume":496,"issue":"2"},{"doi":"10.1146/annurev-astro-120419-014455","publisher":"Annual Reviews","extern":"1","_id":"17564","date_published":"2020-03-30T00:00:00Z","quality_controlled":"1","day":"30","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","title":"The Assembly of the First Massive Black Holes","oa":1,"article_processing_charge":"No","publication_identifier":{"issn":["0066-4146","1545-4282"]},"intvolume":"        58","arxiv":1,"date_updated":"2024-09-18T13:06:37Z","language":[{"iso":"eng"}],"article_type":"original","citation":{"chicago":"Inayoshi, Kohei, Eli Visbal, and Zoltán Haiman. “The Assembly of the First Massive Black Holes.” <i>Annual Review of Astronomy and Astrophysics</i>. Annual Reviews, 2020. <a href=\"https://doi.org/10.1146/annurev-astro-120419-014455\">https://doi.org/10.1146/annurev-astro-120419-014455</a>.","apa":"Inayoshi, K., Visbal, E., &#38; Haiman, Z. (2020). The Assembly of the First Massive Black Holes. <i>Annual Review of Astronomy and Astrophysics</i>. Annual Reviews. <a href=\"https://doi.org/10.1146/annurev-astro-120419-014455\">https://doi.org/10.1146/annurev-astro-120419-014455</a>","ista":"Inayoshi K, Visbal E, Haiman Z. 2020. The Assembly of the First Massive Black Holes. Annual Review of Astronomy and Astrophysics. 58(1), 27–97.","ama":"Inayoshi K, Visbal E, Haiman Z. The Assembly of the First Massive Black Holes. <i>Annual Review of Astronomy and Astrophysics</i>. 2020;58(1):27-97. doi:<a href=\"https://doi.org/10.1146/annurev-astro-120419-014455\">10.1146/annurev-astro-120419-014455</a>","ieee":"K. Inayoshi, E. Visbal, and Z. Haiman, “The Assembly of the First Massive Black Holes,” <i>Annual Review of Astronomy and Astrophysics</i>, vol. 58, no. 1. Annual Reviews, pp. 27–97, 2020.","mla":"Inayoshi, Kohei, et al. “The Assembly of the First Massive Black Holes.” <i>Annual Review of Astronomy and Astrophysics</i>, vol. 58, no. 1, Annual Reviews, 2020, pp. 27–97, doi:<a href=\"https://doi.org/10.1146/annurev-astro-120419-014455\">10.1146/annurev-astro-120419-014455</a>.","short":"K. Inayoshi, E. Visbal, Z. Haiman, Annual Review of Astronomy and Astrophysics 58 (2020) 27–97."},"type":"journal_article","main_file_link":[{"open_access":"1","url":" https://doi.org/10.48550/arXiv.1911.05791"}],"oa_version":"Preprint","date_created":"2024-09-05T12:04:49Z","publication":"Annual Review of Astronomy and Astrophysics","scopus_import":"1","status":"public","external_id":{"arxiv":["1911.05791"]},"abstract":[{"text":"The existence of ≈10^9 Msun supermassive black holes (SMBHs) within the first billion year of the universe has stimulated numerous ideas for the prompt formation and rapid growth of BHs in the early universe. Here we review ways in which the seeds of massive BHs may have first assembled, how they may have subsequently grown as massive as ≈10^9 Msun, and how multi-messenger observations could distinguish between different SMBH assembly scenarios. We conclude the following: (1) The ultra-rare ≈10^9 Msun SMBHs represent only the tip of the iceberg. Early BHs likely fill a continuum from stellar-mass (approx. 10 Msun) to the super-massive (≈10^9 Msun) regime, reflecting a range of initial masses and growth histories. (2) Stellar-mass BHs were likely left behind by the first generation of stars at redshifts as high as z=30, but their initial growth was typically stunted due to the shallow potential wells of their host galaxies. (3) Conditions in some larger, metal-poor galaxies soon became conducive to the rapid formation and growth of massive `seed' holes, via gas accretion and by mergers in dense stellar clusters. (4) BH masses depend on the environment (such as the number and properties of nearby radiation sources and the local baryonic streaming velocity), and on the metal enrichment and assembly history of the host galaxy. (5) Distinguishing between assembly mechanisms will be difficult, but a combination of observations by LISA (probing massive BH growth via mergers) and by deep multi-wavelength electromagnetic observations (probing growth via gas accretion) is particularly promising.","lang":"eng"}],"volume":58,"issue":"1","month":"03","year":"2020","publication_status":"published","page":"27-97","author":[{"last_name":"Inayoshi","first_name":"Kohei","full_name":"Inayoshi, Kohei"},{"last_name":"Visbal","first_name":"Eli","full_name":"Visbal, Eli"},{"first_name":"Zoltán","last_name":"Haiman","full_name":"Haiman, Zoltán","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36"}]}]