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相关论文: If quasars form from primordial black holes

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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

We investigate the hypothesis that quasars formed together with the stellar populations of early-type galaxies. This hypothesis, in conjunction with the stellar ages of early-type galaxies from population synthesis models, the relation of…

天体物理学 · 物理学 2009-11-07 A. Cattaneo , M. Bernardi

With detections of quasars powered by increasingly massive black holes (BHs) at increasingly early times in cosmic history over the past decade, there has been correspondingly rapid progress made on the theory of early BH formation and…

星系天体物理 · 物理学 2016-03-23 Jarrett L. Johnson , Francesco Haardt

A mechanism of creation of stellar-like objects in the very early universe, from the QCD phase transition till BBN and somewhat later, is studied. It is argued that in the considered process primordial black holes with masses above a few…

宇宙学与河外天体物理 · 物理学 2014-01-15 A. D. Dolgov , S. I. Blinnikov

We show that heavy primordial black holes may originate from much lighter ones if the latter are strongly clustered at the time of their formation. While this population is subject to the usual constraints from late-time universe…

宇宙学与河外天体物理 · 物理学 2023-05-10 Valerio De Luca , Gabriele Franciolini , Antonio Riotto

The formation of massive black holes may precede the epoch that characterises the peak of galaxy formation, as characterized by the star formation history in luminous galaxies. Hence protogalactic star formation may be profoundly affected…

天体物理学 · 物理学 2011-05-05 Joseph Silk , Martin J. Rees

The most massive black holes, lurking at the centers of large galaxies, must have formed less than a billion years after the big bang, as they are visible today in the form of bright quasars at redshift larger than six. Their early…

天体物理学 · 物理学 2009-11-11 M. C. Richter , G. B. Tupper , R. D. Viollier

Building on the insight that primordial black holes can arise from the formation and subsequent gravitational collapse of bound states of stable supermassive elementary particles during the early radiation era, we offer a comprehensive…

高能天体物理现象 · 物理学 2021-06-30 Krzysztof A. Meissner , Hermann Nicolai

The tight relationship between the masses of black holes and galaxy spheroids in nearby galaxies implies a causal connection between the growth of these two components. Optically luminous quasars host the most prodigious accreting black…

天体物理学 · 物理学 2010-04-06 D. M. Alexander , I. Smail , F. E. Bauer , S. C. Chapman , A. W. Blain , W. N. Brandt , R. J. Ivison

The hypothesis of existence of primordial black holes with large masses (\geq 10^6 M\odot), formed at the earliest stages of the Universe evolution, is considered in the paper. The possibility does not contradict some theories, see e.g.…

宇宙学与河外天体物理 · 物理学 2013-09-17 V. K. Dubrovich , S. I. Glazyrin

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

We propose the model of first quasars formation around the cluster of rimordial black holes (PBHs). It is supposed, that mass fraction of the universe ~10^-3 is composed of the compact clusters of PBHs, produced during the phase transitions…

天体物理学 · 物理学 2007-05-23 Vyacheslav Dokuchaev , Yury Eroshenko , Sergei Rubin

Model of supermassive black holes formation inside the clusters of primordial black holes is developed. Namely, it is supposed, that some mass fraction of the universe ~10^-3 is composed of the compact clusters of primordial (relic) black…

天体物理学 · 物理学 2009-11-13 V. I. Dokuchaev , Yu. N. Eroshenko , S. G. Rubin

We review recent theoretical results on the formation of the first stars and quasars in the universe, and emphasize related open questions. In particular, we list important differences between the star formation process at high redshifts…

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

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 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

We discuss the production of primordial black holes in an early matter dominated era, which typically takes place in string inspired early universe cosmological models. In particular, we consider a pre-big bang scenario (extending previous…

广义相对论与量子宇宙学 · 物理学 2023-08-14 Pietro Conzinu , Giovanni Marozzi

The next generation of electromagnetic and gravitational wave observatories will open unprecedented windows to the birth of the first supermassive black holes. This has the potential to reveal their origin and growth in the first billion…

Scalar condensates with large expectation values can form in the early universe, for example, in theories with supersymmetry. The condensate can undergo fragmentation into Q-balls before decaying. If the Q-balls dominate the energy density…

宇宙学与河外天体物理 · 物理学 2017-11-15 Eric Cotner , Alexander Kusenko

Black holes, an extreme consequence of the mathematics of General Relativity, have long been suspected of being the prime movers of quasars, which emit more energy than any other objects in the Universe. Recent evidence indicates that…

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