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The origin of supermassive black holes (SMBHs) remains a long-standing problem in astrophysics. Recent JWST observations reveal an unexpectedly abundant population of overmassive black holes at z>4-6, where the BH masses lie far above local…

星系天体物理 · 物理学 2026-01-09 Sunmyon Chon , Shingo Hirano , Tomoaki Ishiyama , Seok-Jun Chang , Volker Springel

Observations with the James Webb Space Telescope (JWST) have identified an abundant population of supermassive black holes (SMBHs) already in place during the first few hundred million years of cosmic history. Most of them appear…

A group of massive galaxies at redshifts of $z\gtrsim 7$ have been recently detected by the James Webb Space Telescope (JWST), which were unexpected to form so early within the framework of standard Big Bang cosmology. In this work, we…

宇宙学与河外天体物理 · 物理学 2024-08-13 Guan-Wen Yuan , Lei Lei , Yuan-Zhu Wang , Bo Wang , Yi-Ying Wang , Chao Chen , Zhao-Qiang Shen , Yi-Fu Cai , Yi-Zhong Fan

The presence of supermassive black holes (SMBHs) at high redshifts ($z>5$), as revealed by James Webb Space Telescope (JWST), challenges standard black hole (BH) formation scenarios. We propose a mechanism in which non-annihilating dark…

高能物理 - 唯象学 · 物理学 2026-01-05 Sulagna Bhattacharya , Debajit Bose , Basudeb Dasgupta , Jaya Doliya , Ranjan Laha

Recent observations of quasars powered by supermassive black holes (SMBHs) out to z > 7 constrain both the initial seed masses and the growth of the most massive black holes (BHs) in the early universe. Here we elucidate the implications of…

宇宙学与河外天体物理 · 物理学 2015-06-12 Jarrett L. Johnson , Daniel J. Whalen , Hui Li , Daniel E. Holz

It has long been suggested that a fraction of the dark matter in the Universe could exist in the form of primordial black holes (PBHs) that have existed since the radiation dominated era. Recent studies have suggested that these PBHs may be…

星系天体物理 · 物理学 2025-09-03 Lewis R. Prole , John A. Regan , Daxal Mehta , Peter Coles , Pratika Dayal

Observations with the James Webb Space Telescope (JWST) have revealed active galactic nuclei (AGN) powered by supermassive black holes (SMBHs) with estimated masses of $10^7-10^8$ M$_\odot$ at redshifts $z\sim7-9$. Some reside in…

星系天体物理 · 物理学 2024-12-17 Junehyoung Jeon , Volker Bromm , Boyuan Liu , Steven L. Finkelstein

Presence of supermassive black holes (SMBHs) with mass $(10^{6}-10^{9}) M_{\odot}$ at $z = 10$ has been recently revealed by James Webb Space Telescope (JWST) observations. In this study we generate seeds for the above range of SMBHs in…

宇宙学与河外天体物理 · 物理学 2026-02-02 Nirmali Das , Sanjeev Kalita , Ankita Kakati

The James Webb Space Telescope (JWST) has revealed a puzzling population of massive black holes in the first billion years, many of which are over-massive compared to their hosts (obese black holes), and reside in metal-poor hosts, posing a…

星系天体物理 · 物理学 2026-04-24 Pratika Dayal

The growth of the first super massive black holes (SMBHs) at z > 6 is still a major challenge for theoretical models. If it starts from black hole (BH) remnants of Population III stars (light seeds with mass ~ 100 Msun) it requires…

星系天体物理 · 物理学 2016-02-10 Rosa Valiante , Raffaella Schneider , Marta Volonteri , Kazuyuki Omukai

Growing the supermassive black holes (~10^9 Msun) that power the detected luminous, highest redshift quasars (z > 6) from light seeds - the remnants of the first stars - within ~ 1 Gyr of the Big Bang poses a timing challenge for growth…

The high redshift ($z>10$) galaxies GHZ9 and UHZ1 observed by the James Webb Space Telescope (JWST) are very massive and have exceptionally high black hole-to-star mass ratios with the central black hole masses $M\gtrsim 10^7\rm~M_\odot$.…

星系天体物理 · 物理学 2024-10-10 Hai-Long Huang , Yu-Tong Wang , Yun-Song Piao

Observations of hyper-luminous quasars at $z>6$ reveal the rapid growth of supermassive black holes (SMBHs $>10^9 \rm M_{\odot}$) whose origin is still difficult to explain. Their progenitors may have formed as remnants of massive, metal…

星系天体物理 · 物理学 2021-06-30 F. Sassano , R. Schneider , R. Valiante , K. Inayoshi , S. Chon , K. Omukai , L. Mayer , P. R. Capelo

In this white paper we explore the capabilities required to identify and study supermassive black holes formed from heavy seeds ($\mathrm{M_{\bullet}} \sim 10^4 - 10^6 \, \mathrm{M_{\odot}}$) in the early Universe. To obtain an unequivocal…

The advent of new and near-future observatories probing the earliest epochs of the Universe has opened the opportunity to investigate the formation and growth of the first massive black holes (MBHs). Additionally, the use of high resolution…

星系天体物理 · 物理学 2025-01-30 Joe McCaffrey , John Regan , Britton Smith , John Wise , Brian O'Shea , Michael Norman

The existence of $\approx$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…

星系天体物理 · 物理学 2020-11-11 Kohei Inayoshi , Eli Visbal , Zoltán Haiman

Supermassive black holes (SMBHs) with masses of $\sim 10^9 {\rm M_\odot}$ within the first billion year of the universe challenge our conventional understanding of black hole formation and growth. One pathway to these SMBHs proposes that…

星系天体物理 · 物理学 2024-06-11 Matthew T. Scoggins , Zoltán Haiman

The James Webb Space Telescope (JWST) has unearthed black holes as massive as $10^{6.2-8.1}M_\odot$ at redshifts of $z \sim 8.5-10.6$ with many systems showing unexpectedly high black hole to stellar mass ratios >=30%, posing a crucial…

星系天体物理 · 物理学 2024-10-09 Pratika Dayal

Understanding the formation and growth of supermassive black holes (SMBHs) at high redshift represents a major challenge for theoretical models. In this work we investigate the early evolution of the first SMBHs by constraining their…

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 grow by the combination of radiation-pressure-limited…

宇宙学与河外天体物理 · 物理学 2015-06-04 Zoltán Haiman
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