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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

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

The rapid emergence of supermassive black holes (SMBHs) in the early Universe poses a challenge to current models of black hole growth. One promising formation pathway is the direct collapse black hole (DCBH) scenario, in which gas in…

Observations from the James Webb Space Telescope (JWST) have uncovered supermassive black holes (SMBHs) with masses exceeding $10^6 \mathrm{M}_{\odot}$ at redshifts $z > 8$, posing significant challenges to existing models of early black…

星系天体物理 · 物理学 2026-01-22 Daxal H. Mehta , John A. Regan , Lewis Prole

We predict the existence and observational signatures of a new class of objects that assembled early, during the first billion years of cosmic time: Obese Black-hole Galaxies (OBGs). OBGs are objects in which the mass of the central black…

宇宙学与河外天体物理 · 物理学 2015-06-15 Bhaskar Agarwal , Andrew J. Davis , Sadegh Khochfar , Priyamvada Natarajan , James S. Dunlop

Overmassive black hole galaxies (OBGs) at redshifts $z \sim$ 10, or 450 Myr after the Big Bang, are one of the most puzzling discoveries by the James Webb Space Telescope to date because they formed by such early epochs and their black-hole…

星系天体物理 · 物理学 2026-05-05 Muhammad A. Latif , Daniel J. Whalen , Sadegh Khochfar , Fergus Cullen

JWST is discovering star forming `candidate' galaxies with photometric redshifts $z>9$ and little attenuation. We model presumptive massive black holes (MBHs) in such galaxies and find that their unobscured emission is fainter than the…

星系天体物理 · 物理学 2023-03-06 Marta Volonteri , Melanie Habouzit , Monica Colpi

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…

While supermassive black holes (BHs) are widely observed in the nearby and distant universe, their origin remains debated with two viable formation scenarios with light and heavy seeds. In the light seeding model, the first BHs form from…

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

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 of high-redshift quasars indicate that super massive black holes (SMBHs) with masses greater than ${\sim}10^9~M_\odot$ were assembled within the first billion years after the Big Bang. It is unclear how such massive black holes…

星系天体物理 · 物理学 2018-09-26 Eli Visbal , Zoltan 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

The recent observations of supermassive black holes (SMBHs) at high redshift challenge our understanding of their formation and growth. There are different proposed pathways to form black hole (BH) seeds, such as the remnants of the first…

星系天体物理 · 物理学 2020-01-22 Tilman Hartwig

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

JWST reveals numerous high-z galaxies and Supermassive Black Holes (SMBHs), suggesting that stars and SMBH seeds formation at $z \gtrsim 10$ may be more efficient than previously derived. One popular SMBH seed scenario is the Direct…

星系天体物理 · 物理学 2025-03-31 Meng Zhang , Bin Yue , Yidong Xu , Andrea Ferrara

The James Webb Space Telescope (JWST) will have the sensitivity to detect early low-mass black holes as they transition from "seeds" to supermassive black holes (BHs). Based on the JAGUAR mock catalog of galaxies, we present a clean color…

星系天体物理 · 物理学 2023-03-17 Andy D. Goulding , Jenny E. Greene

The recent Chandra-JWST discovery of a quasar in the z = 10.1 galaxy UHZ1 reveals that accreting supermassive black holes (SMBHs) were already in place 470 million years after the Big Bang. The Chandra X-ray source detected in UHZ1 is a…

高能天体物理现象 · 物理学 2023-11-28 Priyamvada Natarajan , Fabio Pacucci , Angelo Ricarte , Akos Bogdan , Andy D. Goulding , Nico Cappelluti

Massive Black Hole (MBH) seeds at redshift $z \gtrsim 10$ are now thought to be key ingredients to explain the presence of the super-massive ($10^{9-10} \, \mathrm{M_{\odot}}$) black holes in place $ < 1 \, \mathrm{Gyr}$ after the Big Bang.…

高能天体物理现象 · 物理学 2015-10-27 Fabio Pacucci , Andrea Ferrara , Marta Volonteri , Guillaume Dubus

The nature of the seeds of high-redshift supermassive black holes (SMBHs) is a key question in cosmology. Direct collapse black holes (DCBH) that form in pristine, atomic-line cooling halos, illuminated by a Lyman-Werner (LW) UV flux…

星系天体物理 · 物理学 2015-06-19 Mark Dijkstra , Andrea Ferrara , Andrei Mesinger
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