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The hypothesis that dark matter consists of superheavy particles with the mass close to the Grand Unification scale is investigated. These particles were created from vacuum by the gravitation of the expanding Universe and their decay led…

广义相对论与量子宇宙学 · 物理学 2008-11-26 A. A. Grib , Yu. V. Pavlov

Dark matter has been recognized as an essential part of matter for over 70 years now, and many suggestions have been made, what it could be. Most of these ideas have centered on Cold Dark Matter, particles that are predicted in extensions…

天体物理学 · 物理学 2016-11-15 Peter L. Biermann , Faustin Munyaneza

The supermassive black holes harboured in active galactic nuclei are at the origin of powerful jets which can emit copious amounts of gamma-rays. The exact interplay between the infalling matter, the black hole and the relativistic outflow…

高能天体物理现象 · 物理学 2015-03-17 Berrie Giebels , Felix Aharonian , Hélène Sol

Active Galactic Nuclei (AGN) are known to show flux variability over all observable timescales and across the entire electromagnetic spectrum. Over the past decade, a growing number of sources have been observed to show dramatic flux and…

星系天体物理 · 物理学 2022-11-11 Claudio Ricci , Benny Trakhtenbrot

Hypothetical axion-like particles (ALPs) are of interest because of their potential to act as dark matter or to reveal information about yet undiscovered fundamental constituents of matter. Such particles can be created when photons…

高能天体物理现象 · 物理学 2025-08-19 Denys Malyshev , Lidiia Zadorozhna , Yuriy Bidasyuk , Andrea Santangelo , Oleg Ruchayskiy

Dark matter has been recognized as an essential part of matter for over 70 years now, and many suggestions have been made, what it could be. Most of these ideas have centered on Cold Dark Matter, particles that are expected in extensions of…

天体物理学 · 物理学 2009-11-13 Peter L. Biermann , Faustin Munyaneza

It has long been suspected that Active Galactic Nuclei are powered by accretion of matter onto massive black holes and this belief implies their presence in the nuclei of most nearby galaxies as "relics" of past activity. Just a few years…

天体物理学 · 物理学 2007-05-23 Alessandro Marconi

Recent observations of high-energy neutrinos from active galactic nuclei (AGN), NGC 1068 and TXS 0506+056, suggest that cosmic rays (CRs) are accelerated in the vicinity of the central supermassive black hole and high-energy protons and…

高能物理 - 唯象学 · 物理学 2024-07-25 Gonzalo Herrera , Kohta Murase

A significant fraction of nearby galaxies show evidence of weak nuclear activity unrelated to normal stellar processes. Recent high-resolution, multiwavelength observations indicate that the bulk of this activity derives from black hole…

天体物理学 · 物理学 2010-04-21 Luis C. Ho

This paper summarizes the observations which provide the best evidence for the presence of black holes in active galactic nuclei. This includes: X-ray variability; kinematical studies using optical emission lines as well as the distribution…

天体物理学 · 物理学 2007-05-23 Greg M. Madejski

Considerable observational evidence suggests that the activity of supermassive black holes in galactic nuclei is transient. The term ``active galactic nuclei archaeology'' has even been coined. This implies the possibility of reconstructing…

星系天体物理 · 物理学 2026-03-23 A. V. Moiseev , A. Arshinova , A. A. Smirnova

It is shown that the matter concentration observed through stellar motion at the galactic center (Eckart & Genzel, 1997, MNRAS, 284, 576 and Genzel et al., 1996, ApJ, 472, 153) is consistent with a supermassive object of $2.5 \times 10^6$…

天体物理学 · 物理学 2009-10-30 David Tsiklauri , Raoul D. Viollier

The hypothesis that cold dark matter consists of primordial superheavy particles, the decay of short lifetime component of which led to the observable mass of matter while long living component survived up to modern times manifesting its…

广义相对论与量子宇宙学 · 物理学 2009-11-07 A. A. Grib , Yu. V. Pavlov

Sterile neutrinos with keV masses can constitute all or part of the cosmological dark matter. The electroweak-singlet fermions, which are usually introduced to explain the masses of active neutrinos, need not be heavier than the electroweak…

天体物理学 · 物理学 2017-08-23 Alexander Kusenko

If cold dark matter is present at the galactic center, as in current models of the dark halo, it is accreted by the central black hole into a dense spike. Particle dark matter then annihilates strongly inside the spike, making it a compact…

天体物理学 · 物理学 2009-10-31 Paolo Gondolo , Joseph Silk

Multidimensional modification of gravity with a smaller mass scale of the gravitational interaction is considered. Stable by assumption dark matter particles could decay via interactions with virtual black holes. The decay rates of such…

高能物理 - 唯象学 · 物理学 2023-12-12 E. V. Arbuzova , A. D. Dolgov , A. A. Nikitenko

Sterile neutrinos ($\nu_s$) that mix with active neutrinos ($\nu_a$) are interesting dark matter candidates with a rich cosmological and astrophysical phenomenology. In their simplest incarnation, their production is severely constrained by…

高能物理 - 唯象学 · 物理学 2022-01-25 Gonzalo Alonso-Álvarez , James M. Cline

Solar, atmospheric and reactor neutrino experiments established that neutrinos are massive. It is quite natural then to consider neutrinos as candidate particles for explaining the dark matter in halos around galaxies. We study the…

高能物理 - 唯象学 · 物理学 2015-06-04 A. Nicolaidis

Primordial micro black holes can constitute dark matter if short-distance gravity is modified by extra dimensions or a large number of species and if the memory-burden effect sufficiently suppresses Hawking evaporation. The resulting black…

高能物理 - 唯象学 · 物理学 2026-03-18 Manuel Ettengruber , Florian Kühnel

A widely accepted viewpoint is to consider candidates for cosmological dark matter as neutral and weakly interacting particles, as well as to consider only light elements in the pregalactic chemical composition. It is shown that stable…

天体物理学 · 物理学 2008-01-03 M. Yu. Khlopov
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