{"quality_controlled":"1","scopus_import":"1","month":"11","year":"2010","publication":"AIP Conference Proceedings","publication_identifier":{"issn":["0094-243X"]},"doi":"10.1063/1.3518857","oa":1,"volume":1294,"_id":"17664","extern":"1","title":"The origin and detection of high-redshift supermassive black holes","conference":{"name":"The First Stars and Galaxies: Challenges for the Next Decade","location":"Austin, TX, United States","end_date":"2010-03-11","start_date":"2010-03-08"},"external_id":{"arxiv":["1007.4741"]},"publication_status":"published","abstract":[{"text":"Supermassive black holes (SMBHs) are common in local galactic nuclei, and SMBHs as massive as several billion solar masses already exist at redshift z=6. These earliest SMBHs may arise by the combination of Eddington-limited growth and mergers of stellar-mass seed BHs left behind by the first generation of metal-free stars, or by the rapid direct collapse of gas in rare special environments where the gas can avoid fragmenting into stars. In this contribution, I review these two competing scenarios. I also briefly mention some more exotic ideas and how the different models may be distinguished in the future by LISA and other instruments.","lang":"eng"}],"intvolume":"      1294","article_processing_charge":"No","status":"public","day":"03","main_file_link":[{"open_access":"1","url":" https://doi.org/10.48550/arXiv.1007.4741"}],"date_published":"2010-11-03T00:00:00Z","issue":"1","language":[{"iso":"eng"}],"page":"215-224","author":[{"id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","last_name":"Haiman","full_name":"Haiman, Zoltán","first_name":"Zoltán"},{"last_name":"Whalen","first_name":"Daniel J.","full_name":"Whalen, Daniel J."},{"last_name":"Bromm","full_name":"Bromm, Volker","first_name":"Volker"},{"first_name":"Naoki","full_name":"Yoshida, Naoki","last_name":"Yoshida"}],"date_created":"2024-09-06T07:41:39Z","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","publisher":"American Institute of Physics","type":"conference","oa_version":"Preprint","citation":{"ista":"Haiman Z, Whalen DJ, Bromm V, Yoshida N. 2010. The origin and detection of high-redshift supermassive black holes. AIP Conference Proceedings. The First Stars and Galaxies: Challenges for the Next Decade vol. 1294, 215–224.","ieee":"Z. Haiman, D. J. Whalen, V. Bromm, and N. Yoshida, “The origin and detection of high-redshift supermassive black holes,” in <i>AIP Conference Proceedings</i>, Austin, TX, United States, 2010, vol. 1294, no. 1, pp. 215–224.","chicago":"Haiman, Zoltán, Daniel J. Whalen, Volker Bromm, and Naoki Yoshida. “The Origin and Detection of High-Redshift Supermassive Black Holes.” In <i>AIP Conference Proceedings</i>, 1294:215–24. American Institute of Physics, 2010. <a href=\"https://doi.org/10.1063/1.3518857\">https://doi.org/10.1063/1.3518857</a>.","short":"Z. Haiman, D.J. Whalen, V. Bromm, N. Yoshida, in:, AIP Conference Proceedings, American Institute of Physics, 2010, pp. 215–224.","ama":"Haiman Z, Whalen DJ, Bromm V, Yoshida N. The origin and detection of high-redshift supermassive black holes. In: <i>AIP Conference Proceedings</i>. Vol 1294. American Institute of Physics; 2010:215-224. doi:<a href=\"https://doi.org/10.1063/1.3518857\">10.1063/1.3518857</a>","apa":"Haiman, Z., Whalen, D. J., Bromm, V., &#38; Yoshida, N. (2010). The origin and detection of high-redshift supermassive black holes. In <i>AIP Conference Proceedings</i> (Vol. 1294, pp. 215–224). Austin, TX, United States: American Institute of Physics. <a href=\"https://doi.org/10.1063/1.3518857\">https://doi.org/10.1063/1.3518857</a>","mla":"Haiman, Zoltán, et al. “The Origin and Detection of High-Redshift Supermassive Black Holes.” <i>AIP Conference Proceedings</i>, vol. 1294, no. 1, American Institute of Physics, 2010, pp. 215–24, doi:<a href=\"https://doi.org/10.1063/1.3518857\">10.1063/1.3518857</a>."},"date_updated":"2024-09-25T07:40:43Z"}