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Gamma-ray bursts (GRBs) are short, intense flashes of soft gamma-rays coming from the distant Universe. Long-duration GRBs (those lasting more than ~2 s) are believed to originate from the deaths of massive stars, mainly on the basis of a…

We propose a novel class of compact dark matter objects in theories where the dark matter consists of multiple sectors. We call these objects $N$-MACHOs. In such theories neither the existence of dark matter species nor their extremely weak…

Cosmology and Nongalactic Astrophysics · Physics 2020-04-27 Gia Dvali , Emmanouil Koutsangelas , Florian Kuhnel

Nontopological solitons formed during first-order phase transitions can serve as macroscopic dark matter candidates, with their stability ensured by a charge asymmetry traditionally assumed to originate from baryogenesis. Following this…

High Energy Physics - Phenomenology · Physics 2026-02-26 Shinya Kanemura , Shao-Ping Li , Ke-Pan Xie

We analyze here late evolutionary stages of massive (with initial mass higher than 8 masses of the Sun) close binary stars. Our purposes are to study possible mechanisms of gamma ray bursts (GRBs) origin. We suppose in this paper that GRB…

Astrophysics · Physics 2009-03-19 A. I. Bogomazov , V. M. Lipunov , A. V. Tutukov

A possible unified model of short and long gamma-ray bursts (GRBs), X-ray rich GRBs, and X-ray flashes is proposed. It is assumed that the jet of a GRB consists of many emitting sub-shells (i.e., an inhomogeneous jet model). The…

Astrophysics · Physics 2007-05-23 Ryo Yamazaki , Kunihito Ioka , Takashi Nakamura , Kenji Toma

Cosmological nucleosynthesis calculations imply that many of the baryons in the Universe must be dark. We discuss the likelihood that some of these dark baryons may reside in the discs or halos of galaxies. If they were in the form of…

Astrophysics · Physics 2007-05-23 B. J. Carr

Primordial black holes (PBHs) represent a natural candidate for one of the components of the dark matter (DM) in the Universe. In this review, we shall discuss the basics of their formation, abundance and signatures. Some of their…

Cosmology and Nongalactic Astrophysics · Physics 2021-06-03 Pablo Villanueva-Domingo , Olga Mena , Sergio Palomares-Ruiz

In this essay, we assume that negative mass objects can exist in the extragalactic space and analyze the consequences of their microlensing on light from distant Active Galactic Nuclei. We find that such events have very similar features to…

General Relativity and Quantum Cosmology · Physics 2010-12-03 Diego F. Torres , Gustavo E. Romero , Luis A. Anchordoqui

Naked singularities appear naturally in dynamically evolving solutions of Einstein equations involving gravitational collapse of radiation, dust and perfect fluids, provided the rate of accretion is less than a critical value. We propose…

High Energy Physics - Theory · Physics 2009-10-22 Sandip K. Chakrabarti , Pankaj S. Joshi

Current understanding of core collapse and thermonuclear supernovae is reviewed. Recent progress in unveiling the nature of cosmic gamma-ray bursts (GRB) is discussed, with the focus on the apparent link of several GRBs with an energetic…

Astrophysics · Physics 2007-05-23 Konstantin Postnov

Although the dark matter is usually assumed to be some form of elementary particle, primordial black holes (PBHs) could also provide some of it. However, various constraints restrict the possible mass windows to $10^{16}$ - $10^{17}\,$g,…

Cosmology and Nongalactic Astrophysics · Physics 2020-09-08 Bernard Carr , Florian Kuhnel

Gamma-Ray Bursts (GRBs) fall into two classes: short-hard and long-soft bursts. The latter are now known to have X-ray and optical afterglows, to occur at cosmological distances in star-forming galaxies, and to be associated with the…

Active galactic nuclei, hosting supermassive black holes and launching relativistic jets, are the most numerous objects on the gamma-ray sky. At the other end of the mass scale, phenomena related to stellar mass black holes, in particular…

High Energy Astrophysical Phenomena · Physics 2017-06-28 Elina Lindfors

Black holes can be produced in collapse of small-scale dark matter structures, which can happen at any time from the early to present-day universe. Microstructure black holes (MSBHs) can have a wide range of masses. Small MSBHs evaporate…

Cosmology and Nongalactic Astrophysics · Physics 2023-09-06 Zachary S. C. Picker , Alexander Kusenko

We propose a possible unified model of short and long gamma-ray bursts (GRBs), X-ray rich GRBs, and X-ray flashes. The jet of a GRB is assumed to consist of multiple sub-jets or sub-shells (i.e., an inhomogeneous jet model). The…

Astrophysics · Physics 2010-11-11 Ryo Yamazaki , Kunihito Ioka , Takashi Nakamura , Kenji Toma

The formation and growth of black holes can strongly influence the distribution of dark matter around them. I discuss here the different types of dark matter overdensities around black holes, including dark matter cusps, spikes, mounds,…

Cosmology and Nongalactic Astrophysics · Physics 2024-04-18 Gianfranco Bertone

The influence of a possible low gravity scale, concretely through the presence of extra dimensions or additional species, on radiation properties of micro black holes is investigated. In particular, the suppression of evaporation through…

High Energy Physics - Theory · Physics 2025-07-02 Manuel Ettengruber , Florian Kuhnel

Cosmological nucleosynthesis calculations imply that many of the baryons in the Universe must be dark. We discuss the likelihood that some of these dark baryons may reside in galaxies as Massive Compact Halo Objects (MACHOs), the remnants…

Astrophysics · Physics 2007-05-23 B. J. Carr

Striking similarities exist between high energy gamma ray emission from active galactic nuclei (AGN) and gamma ray bursts (GRBs). They suggest that GRBs are generated by inverse Compton scattering from highly relativistic electrons in…

Astrophysics · Physics 2009-10-22 Nir J. Shaviv , Arnon Dar

We note that if the GRB phenomenon follows from the collapse of a massive object forming a black hole and a torus accreting into it, the resulting ejecta can be only related to the mass and angular momentum that characterize the black hole.…

Astrophysics · Physics 2007-05-23 Guido Barbiellini , Annalisa Celotti , Francesco Longo