Title Titans of the early Universe: The Prato statement on the origin of the first supermassive black holes
Authors Woods, Tyrone E.
Agarwal, Bhaskar
Bromm, Volker
Bunker, Andrew
Chen, Ke-Jung
Chon, Sunmyon
Ferrara, Andrea
Glover, Simon C. O.
Haemmerle, Lionel
Haiman, Zoltan
Hartwig, Tilman
Heger, Alexander
Hirano, Shingo
Hosokawa, Takashi
Inayoshi, Kohei
Klessen, Ralf S.
Kobayashi, Chiaki
Koliopanos, Filippos
Latif, Muhammad A.
Li, Yuexing
Mayer, Lucio
Mezcua, Mar
Natarajan, Priyamvada
Pacucci, Fabio
Rees, Martin J.
Regan, John A.
Sakurai, Yuya
Salvadori, Stefania
Schneider, Raffaella
Surace, Marco
Tanaka, Takamitsu L.
Whalen, Daniel J.
Yoshida, Naoki
Affiliation Monash Univ, Monash Ctr Astrophys, Sch Phys & Astron, Clayton, Vic 3800, Australia
Univ Birmingham, Sch Phys & Astron, Birmingham Inst Gravitat Wave Astron, Birmingham B15 2TT, W Midlands, England
Heidelberg Univ, Zentrum Astron, Inst Theoret Astrophys, Albert Ueberle Str 2, D-69120 Heidelberg, Germany
Univ Texas Austin, Dept Astron, 2511 Speedway, Austin, TX 78712 USA
Univ Oxford, Dept Phys, Keble Rd, Oxford OX1 3RH, England
Univ Tokyo, Todai Inst Adv Study, Kavli IPMU WPI, 5-1-5 Kashiwanoha, Kashiwa, Chiba 2778583, Japan
Acad Sinica, Inst Astron & Astrophys, Taipei 10617, Taiwan
Tohoku Univ, Astron Inst, Sendai, Miyagi 9808578, Japan
Scuola Normale Super Pisa, Piazza Cavalieri 7, I-56126 Pisa, Italy
Georgia Inst Technol, Sch Phys, Atlanta, GA 30332 USA
Univ Geneva, Observ Geneve, Chemin Maillettes 51, CH-1290 Sauverny, Switzerland
Columbia Univ, Dept Astron, New York, NY 10027 USA
Univ Tokyo, Sch Sci, Dept Phys, Bunkyo Ku, Tokyo 1130033, Japan
Univ Tokyo, UTIAS, Kavli IPMU WPI, Kashiwa, Chiba 2778583, Japan
Tsung Dao Lee Inst, Shanghai 200240, Peoples R China
Kyushu Univ, Fac Sci, Dept Earth & Planetary Sci, Fukuoka, Fukuoka 8190395, Japan
Kyoto Univ, Dept Phys, Sakyo Ku, Kyoto 6068502, Japan
Peking Univ, Kavli Inst Astron & Astrophys, Beijing 100871, Peoples R China
Heidelberg Univ, Interdisziplinares Zentrum Wissensch Rechnen, INF 205, D-69120 Heidelberg, Germany
Univ Hertfordshire, Ctr Astrophys Res, Sch Phys Astron & Math, Hatfield AL1O 9AB, Herts, England
CNRS, IRAP, 9 Av Colonel Roche,BP 44346, F-31028 Toulouse 4, France
Univ Toulouse, UPS OMP, IRAP, F-31400 Toulouse, France
United Arab Emirates Univ, Coll Sci, Phys Dept, Al Ain 00000, U Arab Emirates
Penn State Univ, Dept Astron & Astrophys, 525 Davey Lab, University Pk, PA 16802 USA
Penn State Univ, Inst Cosmol & Grav, University Pk, PA 16802 USA
Univ Zurich, Ctr Theoret Astrophys & Cosmol, Winterthurerstr 190, CH-8057 Zurich, Switzerland
CSIC, ICE, Inst Space Sci, Campus UAB,Carrer Magrans, Barcelona 08193, Spain
IEEC, Carrer Gran Capita, Barcelona 08034, Spain
Yale Univ, Dept Astron, POB 208101, New Haven, CT 06520 USA
Yale Univ, Dept Phys, POB 208121, New Haven, CT 06520 USA
Univ Cambridge, Inst Astron, Madingley Rd, Cambridge CB3 0HA, England
Dublin City Univ, Ctr Astrophys & Relat, Sch Math Sci, Glasnevin D09 E432, Ireland
Univ Firenze, Dipartimento Fis & Astron, Via G Sansone 1, I-50019 Sesto Fiorentino, Italy
INAF, Osservatorio Astrofis Arcetri, Largo E Fermi 5, I-50125 Florence, Italy
PSL Univ, Observ Paris, CNRS, GEPI, Pl Jules Janssen, F-92195 Meudon, France
Sapienza Univ Roma, Dipartimento Fis, Piazzale A Moro 2, I-00185 Rome, Italy
Univ Portsmouth, Inst Cosmol & Gravitat, Portsmouth PO1 3FX, Hants, England
Keywords first stars - quasars
supermassive black holes
high-redshift - Population III
massive
binaries
Issue Date 2019
Publisher PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA
Abstract In recent years, the discovery of massive quasars at $z\sim7$ has provided a striking challenge to our understanding of the origin and growth of supermassive black holes in the early Universe. Mounting observational and theoretical evidence indicates the viability of massive seeds, formed by the collapse of supermassive stars, as a progenitor model for such early, massive accreting black holes. Although considerable progress has been made in our theoretical understanding, many questions remain regarding how (and how often) such objects may form, how they live and die, and how next generation observatories may yield new insight into the origin of these primordial titans. This review focusses on our present understanding of this remarkable formation scenario, based on the discussions held at the Monash Prato Centre from November 20 to 24, 2017, during the workshop 'Titans of the Early Universe: The Origin of the First Supermassive Black Holes'.
URI http://hdl.handle.net/20.500.11897/551719
ISSN 1323-3580
DOI 10.1017/pasa.2019.14
Indexed SCI(E)
EI
Appears in Collections: 科维理天文与天体物理研究所

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