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The origin of super-massive black holes in the early universe remains poorly understood.Gravitational collapse of a massive primordial gas cloud is a promising initial process,but theoretical studies have difficulty growing the black hole…

宇宙学与河外天体物理 · 物理学 2017-10-13 Shingo Hirano , Takashi Hosokawa , Naoki Yoshida , Rolf Kuiper

The presence of supermassive black holes (SMBHs, $M_{\bullet}\sim 10^{6-10}~M_{\odot}$) in the first cosmic Gyr ($z\gtrsim 6$) challenges current models of BH formation and evolution. We propose a novel mechanism for the formation of early…

宇宙学与河外天体物理 · 物理学 2024-11-07 Francesco Ziparo , Simona Gallerani , Andrea Ferrara

Direct-collapse black holes (DCBHs) are currently one of the leading contenders for the origins of the first quasars in the universe, over 300 of which have now been found at $z >$ 6. But the birth of a DCBH in an atomically-cooling halo…

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

The first massive astrophysical black holes likely formed at high redshifts (z>10) at the centers of low mass (~10^6 Msun) dark matter concentrations. These black holes grow by mergers and gas accretion, evolve into the population of bright…

天体物理学 · 物理学 2016-01-27 Zoltan Haiman , Eliot Quataert

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

We consider the physical conditions under which supermassive black holes could have formed inside the first galaxies. Our SPH simulations indicate that metal-free galaxies with a virial temperature ~10^4 K and with suppressed H2 formation…

天体物理学 · 物理学 2009-11-07 Volker Bromm , Abraham Loeb

Observations reveal the presence of supermassive black holes (SMBH) as early as ~700 million years after the Big Bang. Their formation path is still subject to current debate. We explore the influence of magnetic fields, which are strongly…

星系天体物理 · 物理学 2019-06-12 Philipp Grete , Muhammad A. Latif , Dominik R. G. Schleicher , Wolfram Schmidt

The discovery of luminous quasars at redshift z ~ 6 indicates the presence of supermassive black holes (SMBHs) of mass ~10^9 Msun when the Universe was less than one billion years old. This finding presents several challenges for…

The observational evidence for a population of quasars powered by supermassive black holes of mass \geq 10^9 M_sun at redshifts z\geq 6 poses a great challenge for any model describing the formation of galaxies. Assuming uninterrupted…

天体物理学 · 物理学 2007-05-23 Norbert Duechting

Context. The seeds of the supermassive black holes (SMBHs) with masses of ~10^9 M_Sun observed already at z ~ 6 may have formed through the direct collapse of primordial gas in T_vir >~ 10^4 K halos, whereby the gas must stay hot (~10^4 K)…

宇宙学与河外天体物理 · 物理学 2013-06-07 C. Van Borm , M. Spaans

Observations of the most luminous quasars at redshift z>6 reveal the existence of numerous supermasssive black holes (>10^9 Msun) already in place about twelve billion years ago. In addition, the interstellar medium of the galaxies hosting…

星系天体物理 · 物理学 2017-07-26 Rosa Valiante , Bhaskar Agarwal , Melanie Habouzit , Edwige Pezzulli

Supermassive black holes with up to a $\rm 10^{9}~M_{\odot}$ dwell in the centers of present-day galaxies, and their presence has been confirmed at z $\geq$ 6. Their formation at such early epochs is still an enigma. Different pathways have…

宇宙学与河外天体物理 · 物理学 2015-06-15 M. A. Latif , D. R. G. Schleicher , W. Schmidt , J. Niemeyer

We show that seeds for quasar black holes could have originated from the initial cosmological collapse of overdense regions with unusually small rotation. The gas in these rare regions collapses into a compact disk that shrinks on a short…

天体物理学 · 物理学 2009-09-25 Daniel J. Eisenstein , Abraham Loeb

The existence of massive black holes was postulated in the sixties, when the first quasars were discovered. In the late nineties their reality was proven beyond doubt, in the Milky way and a handful nearby galaxies. Since then, enormous…

宇宙学与河外天体物理 · 物理学 2015-06-11 Marta Volonteri , Jillian Bellovary

The detection of $\rm z>6$ quasars reveals the existence of supermassive black holes of a few $\rm 10^9~M_{\odot}$. One of the potential pathways to explain their formation in the infant universe is the so-called direct collapse model which…

星系天体物理 · 物理学 2016-02-17 Muhammad A. Latif , Dominik R. G. Schleicher , Tilman Hartwig

Recent observations have shown that, only a billion years after the Big Bang, the Universe was already lit up by bright quasars fuelled by the infall of gas onto supermassive black holes. The masses of these early black holes are inferred…

天体物理学 · 物理学 2015-06-24 Rennan Barkana , Abraham Loeb

The discovery of high redshift quasars represents a challenge to the origin of supermassive black holes. Here, two evolutionary scenarios are considered. The first one concerns massive black holes in the local universe, which in a large…

星系天体物理 · 物理学 2020-01-24 José Antonio de Freitas Pacheco

When black hole jets encounter ambient medium, they can compress the gas, trigger star formation, and create stellar clusters containing tens of thousands of stars. Here, we report a remarkable discovery of such a phenomenon that happened…

星系天体物理 · 物理学 2025-09-16 Marko Mićić , Themiya Nanayakkara , Xinyu Dai , Jeremy Bailin , Miljan Kolčić

We describe a new scenario for the formation of primordial black holes (PBHs). In the early Universe, the long-range forces mediated by the scalar fields can lead to formation of halos of heavy particles even during the radiation-dominated…

宇宙学与河外天体物理 · 物理学 2021-01-28 Marcos M. Flores , Alexander Kusenko