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More than 300 supermassive black holes have been detected at redshifts larger than 6, and they are abundant in the centers of local galaxies. Their formation mechanisms, however, are still rather unconstrained. A possible origin of these…

The statistics of black holes and their masses strongly suggests that their mass distribution has a cutoff towards lower masses near $3 \times 10^{6}$ M$_{\odot}$. This is consistent with a classical formation mechanism from the…

宇宙学与河外天体物理 · 物理学 2015-06-19 Peter L. Biermann , Biman B. Nath , Laurenţiu I. Caramete , Benjamin C. Harms , Todor Stanev , Julia Becker Tjus

The James Webb Space Telescope (JWST) has recently uncovered a new record-breaking quasar, UHZ1, at a redshift of $z\sim10$. This discovery continues JWST's trend of confronting the expectations from the standard $\Lambda$CDM model of…

星系天体物理 · 物理学 2023-12-22 Cosmin Ilie , Katherine Freese , Andreea Petric , Jillian Paulin

The detection of quasars at $z>6$ unveils the presence of supermassive black holes (BHs) of a few billion solar masses. The rapid formation process of these extreme objects remains a fascinating and open issue. Such discovery implies that…

星系天体物理 · 物理学 2016-10-26 Muhammad A. Latif , Andrea Ferrara

There are several puzzling phenomena from recent JWST observations, which seem to push the standard {\Lambda}CDM cosmology over the edge. All those puzzles can be understood in a coherent way if we assume that first massive black holes…

星系天体物理 · 物理学 2025-08-14 Xiaobo Dong , Yongda Zhu , Marcia Rieke , George Rieke , Xinyu Li , Peter Behroozi , Haixia Ma , Runyu Meng , Zhiying Mao , Zhe Sun

The so-called `impossibly early galaxy' problem, first identified via the Hubble Space Telescope's observation of galaxies at redshifts z > 10, appears to have been exacerbated by the more recent James Webb Space Telescope (JWST) discovery…

宇宙学与河外天体物理 · 物理学 2023-08-01 Fulvio Melia

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

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

High-redshift quasars ($z\gtrsim6$), powered by black holes (BHs) with large inferred masses, imply rapid BH growth in the early Universe. The most extreme examples have inferred masses of $\sim \! 10^9\,$M$_\odot$ at $z = 7.5$ and $\sim \!…

星系天体物理 · 物理学 2023-11-09 Jake S. Bennett , Debora Sijacki , Tiago Costa , Nicolas Laporte , Callum Witten

These notes review theoretical models of massive black hole formation, growth and observables. They start with a brief summary of basic properties of massive black hole properties. The current view on massive black holes and active galactic…

星系天体物理 · 物理学 2025-10-07 Marta Volonteri

JWST has detected many overmassive galactic systems at $z > 4$, where the mass of the black hole, $M_\bullet$, is $10-100$ times larger than expected from local relations, given the host's stellar mass, $M_\star$. This Letter presents a…

星系天体物理 · 物理学 2024-03-29 Fabio Pacucci , Abraham Loeb

We have obtained deep, multi-band imaging observations around three of the most distant known quasars at redshifts z>6. Standard accretion theory predicts that the supermassive black holes present in these quasars were formed at a very…

We report for the first time a sample of 12 supermassive black holes (SMBHs) hosted by low-mass galaxies at cosmic noon, i.e., in a redshift range consistent with the peak of star formation history: $z \sim 1-3$. These black holes are two…

星系天体物理 · 物理学 2024-04-23 Mar Mezcua , Fabio Pacucci , Hyewon Suh , Malgorzata Siudek , Priyamvada Natarajan

We investigate the coupled formation and evolution of galaxies and their embedded supermassive black holes using state-of-the-art hydrodynamic simulations of cosmological structure formation. For the first time, we self-consistently follow…

天体物理学 · 物理学 2009-11-13 Tiziana Di Matteo , Joerg Colberg , Volker Springel , Lars Hernquist , Debora Sijacki

Recent results from combined cosmological probes indicate that the Dark Energy component of the Universe could be dynamical. The simplest explanation envisages the presence of a quintessence field rolling into a potential, where the Dark…

宇宙学与河外天体物理 · 物理学 2026-02-06 N. Menci , M. Castellano , P. Mukherjee , D. Roberts , P. Santini , A. A. Sen , F. Shankar

Observations of the most luminous quasars at high redshifts ($z > 6$) have revealed that the largest supermassive black holes (SMBHs) at those epochs tend to be substantially overmassive relative to their host galaxies compared to the local…

星系天体物理 · 物理学 2022-09-01 Haojie Hu , Kohei Inayoshi , Zoltán Haiman , Wenxiu Li , Eliot Quataert , Rolf Kuiper

Recent astronomical discoveries of supermassive black holes (quasars), gamma-bursters, supernovae, and dust at high redshifts, z = (5 --10), are reviewed. Such a dense population of the early universe is at odds with the conventional…

宇宙学与河外天体物理 · 物理学 2017-11-22 A. D. Dolgov

The presence of supermassive black holes at redshift z > 6 raises some questions about their formation and growth in the early universe. Due to the construction of new telescopes like the ELT to observe and detect SMBHs, it will be useful…

宇宙学与河外天体物理 · 物理学 2023-05-31 M. Liempi , L. Almonacid , D. R. G. Schleicher , A. Escala

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

We discuss constraints on the assembly history of supermassive black holes from the observed remnant black holes in nearby galaxies and from the emission caused by accretion onto these black holes. We also summarize the results of a…

天体物理学 · 物理学 2007-05-23 Martin G. Haehnelt , Guinevere Kauffmann