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The cosmic reionization era, which includes formation of the first stars, galaxies, and AGN, is now one of the most active frontiers of cosmological research. We review briefly our current understanding of the early structure formation, and…

天体物理学 · 物理学 2016-11-09 S. G. Djorgovski

We estimate collapse rates of axion stars in our galaxy based on the axion minicluster mass function of the Milky Way dark matter halo. We consider axion-like particles with different temperature evolution of the axion mass, including the…

高能物理 - 唯象学 · 物理学 2024-10-18 Dennis Maseizik , Joshua Eby , Hyeonseok Seong , Günter Sigl

Dark matter annihilation might power the first luminous stars in the Universe. These types of stars, known as dark stars, could form in $(10^6\mathrm{-}10^8)\,M_\odot$ protohalos at redshifts $z \sim 20$, and they could be much more…

高能物理 - 唯象学 · 物理学 2022-08-30 Youjia Wu , Sebastian Baum , Katherine Freese , Luca Visinelli , Hai-Bo Yu

We investigate the ab-initio formation of super-massive stars in a pristine atomic cooling halo. The halo is extracted from a larger self-consistent parent simulation. The halo remains metal-free and star formation is suppressed due to a…

星系天体物理 · 物理学 2021-01-08 John A. Regan , John H. Wise , Tyrone E. Woods , Turlough P. Downes , Brian W. O'Shea , Michael L. Norman

The primordial black holes (PBHs) play as a novel source to radiate light elementary particles of energies in the region of a few hundred MeV. We explore the possibility that the axion-like particles (ALPs) with mass less than 1 MeV are…

高能物理 - 唯象学 · 物理学 2022-12-07 Tong Li , Rui-Jia Zhang

In this work, we study the luminosity that results from the conversion of QCD axion particles into photons in the magnetic field of the plasma accreting onto black holes (BHs). For the luminosities to be large two conditions need to be met:…

高能物理 - 唯象学 · 物理学 2024-04-22 Ricardo Z. Ferreira , Ángel Gil Muyor

The cosmological scenario where the Peccei-Quinn symmetry is broken after inflation is investigated. In this scenario, topological defects such as strings and domain walls produce a large number of axions, which contribute to the cold dark…

高能物理 - 唯象学 · 物理学 2015-08-12 Masahiro Kawasaki , Ken'ichi Saikawa , Toyokazu Sekiguchi

We review the current status of knowledge concerning the early phases of star formation during cosmic dawn. This includes the first generations of stars forming in the lowest mass dark matter halos in which cooling and condensation of gas…

星系天体物理 · 物理学 2020-04-29 Lionel Haemmerlé , Lucio Mayer , Ralf S. Klessen , Takashi Hosokawa , Piero Madau , Volker Bromm

We show that primordial black holes (PBHs) develop non-negligible spins through Hawking emission of the large number of axion-like particles generically present in string theory compactifications. This is because scalars can be emitted in…

宇宙学与河外天体物理 · 物理学 2021-10-27 Marco Calzà , John March-Russell , João G. Rosa

We study the gravitational collapse of axion dark matter fluctuations in the post-inflationary scenario, so-called axion miniclusters, with N-body simulations. Largely confirming theoretical expectations, overdensities begin to collapse in…

宇宙学与河外天体物理 · 物理学 2020-07-22 Benedikt Eggemeier , Javier Redondo , Klaus Dolag , Jens C. Niemeyer , Alejandro Vaquero

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

Searches for dark matter imprints are one of the most active areas of current research. We focus here on light fields with mass $m_B$, such as axions and axion-like candidates. Using perturbative techniques and full-blown nonlinear…

广义相对论与量子宇宙学 · 物理学 2015-09-15 Richard Brito , Vitor Cardoso , Hirotada Okawa

Dark matter axions form a rethermalizing Bose-Einstein condensate. This provides an opportunity to distinguish axions from other forms of dark matter on observational grounds. I show that if the dark matter is axions, tidal torque theory…

星系天体物理 · 物理学 2015-05-18 Pierre Sikivie

We present a scenario that ameliorates the tuning problems present in models of primordial black hole dark matter from inflation. Our setup employs the advantages of gravitational collapse in a long epoch of early matter domination with…

宇宙学与河外天体物理 · 物理学 2020-06-23 Guillermo Ballesteros , Julián Rey , Fabrizio Rompineve

We consider a cosmological scenario in which the very early Universe experienced a transient epoch of matter domination due to the formation of a large population of primordial black holes (PBHs) with masses $M \lesssim 10^{9}\,\textrm{g}$,…

高能物理 - 唯象学 · 物理学 2021-09-03 Francesco Schiavone , Daniele Montanino , Alessandro Mirizzi , Francesco Capozzi

Growing amount of data show evidence for statistical and apparent physical association between low-redshift galaxies and high-redshift quasi-stellar objects, suggesting noncosmological origin of their redshift and failure of classical…

天体物理学 · 物理学 2007-05-23 Anatoly A. Svidzinsky

It has recently been suggested that the presence of a plenitude of light axions, an Axiverse, is evidence for the extra dimensions of string theory. We discuss the observational consequences of these axions on astrophysical black holes…

高能物理 - 理论 · 物理学 2011-08-17 Asimina Arvanitaki , Sergei Dubovsky

We study a modification of the primordial black hole (PBH) formation model from axion bubbles. We assume that the Peccei-Quinn scalar rolls down in the radial direction from a large field value to the potential minimum during inflation,…

宇宙学与河外天体物理 · 物理学 2023-10-23 Kentaro Kasai , Masahiro Kawasaki , Naoya Kitajima , Kai Murai , Shunsuke Neda , Fuminobu Takahashi

If the dark matter is made of ultra-light axions, stable solitonic cores form at the centers of virialized halos. In some range for the mass $m$ of the axion particle, these cores are sufficiently compact and can mimic supermassive black…

宇宙学与河外天体物理 · 物理学 2020-04-08 Vincent Desjacques , Adi Nusser

We study the clustering of primordial black holes (PBHs) and axion miniclusters produced in the model proposed to explain the LIGO/Virgo events or the seeds of the supermassive black holes (SMBHs) in arXiv:2006.13137. It is found that this…

宇宙学与河外天体物理 · 物理学 2025-07-18 Kentaro Kasai , Masahiro Kawasaki , Naoya Kitajima , Kai Murai , Shunsuke Neda , Fuminobu Takahashi