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Gamma-ray bursts are the most luminous explosions in the Universe, and their origin and mechanism are the focus of intense research and debate. More than three decades after their discovery, and after pioneering breakthroughs from space and…

天体物理学 · 物理学 2010-04-06 P. Meszaros

Gamma ray bursts (GRBs) are astronomical phenomena detected at highest energies. The gamma ray photons carry energies on the order of mega-electronovolts and arrive to us from the point-like sources that are uniformly distributed on the…

高能天体物理现象 · 物理学 2021-04-21 A. Janiuk , B. James , K. Sapountzis

The mechanism responsible for the prompt emission of gamma-ray bursts (GRBs) is still a debated issue. The prompt phase-related GRB correlations can allow to discriminate among the most plausible theoretical models explaining this emission.…

高能天体物理现象 · 物理学 2018-02-01 Maria Dainotti , Roberta Del Vecchio , Mariusz Tarnopolski

It is generally believed that cosmological Gamma Ray Bursts (GRBs) are produced by the deceleration of relativistic objects with Lorentz factor (Gamma) >~ 100. We study the possibility that some GRBs are produced along with relativistic…

天体物理学 · 物理学 2016-08-30 Hideyuki Umeda

Recent high energy gamma-ray observations of both single supernova remnants and superbubbles, together with observations of supernovae, star formation regions, and local cosmic ray composition, now provide an integrated framework tying…

高能天体物理现象 · 物理学 2018-10-31 Richard E. Lingenfelter

Gamma-ray bursts are the most powerful explosions in the universe and are mainly placed at very large redshifts, up to $z\simeq 9$. In this short review, we first discuss gamma-ray burst classification and morphological properties. We then…

高能天体物理现象 · 物理学 2021-10-28 Orlando Luongo , Marco Muccino

The recent success of a proposal from some time ago to explain the spectrum of cosmic rays allows some strong conclusions to be made on the physics of supernovae: In the context of this specific proposal to explain the origin of cosmic…

天体物理学 · 物理学 2007-05-23 Peter L. Biermann , Sergej Moiseenko , Samvel Ter-Antonyan , Ana Vasile

Gamma-ray burst sources appear to fulfill all the conditions for being efficient cosmic ray accelerators, and being extremely compact, are also expected to produce multi-GeV to PeV neutrinos. I review the basic model predictions for the…

高能天体物理现象 · 物理学 2015-11-05 P. Mészáros

We give an upper estimate for the number of gamma ray bursts from ordinary (non-superconducting) cosmic strings expected to be observed at terrestrial detectors. Assuming that cusp annihilation is the mechanism responsible for the bursts we…

高能物理 - 唯象学 · 物理学 2016-09-01 R. H. Brandenberger , A. T. Sornborger , M. Trodden

We argue that gamma-ray bursts (GRBs) may be the origin of the cosmic gamma-ray background radiation observed in GeV range. It has theoretically been discussed that protons may carry a much larger amount of energy than electrons in GRBs,…

天体物理学 · 物理学 2009-10-31 Tomonori Totani

Major advances have been made in the field of gamma-ray bursts in the last two years. The successful discovery of X-ray, optical and radio afterglows, which were predicted by theory, has made possible the identification of host galaxies at…

天体物理学 · 物理学 2009-10-31 P. Meszaros

We investigate the theoretical and observational implications of the acceleration of protons and heavier nuclei in supernova remnants (SNRs). By adopting a semi-analytical technique, we study the non-linear interplay among particle…

高能天体物理现象 · 物理学 2017-08-23 D. Caprioli , P. Blasi , E. Amato

Cosmological gamma-ray bursts (GRBs) are probably powered by systems harboring a rotating black hole. These may result from hypernovae or black hole-neutron star coalescence. We identify short/long bursts with hyper- and suspended-accretion…

天体物理学 · 物理学 2017-08-23 Maurice H. P. M. van Putten

Correlation analysis of Swift gamma-ray burst coordinates and nearby star locations (catalog Gliese) reveals 4 coincidences with good angular accuracy. The random probability is 4\times 10^{-5}, so evidencing that coincident stars are…

高能天体物理现象 · 物理学 2011-04-19 B. I. Luchkov

In almost any scenario for 'cosmological' gamma-ray bursts (and in many models where they originate in our own Galaxy), the initial energy density is so large that the resulting relativistic plasma expands with $v\sim c$ producing a blast…

天体物理学 · 物理学 2009-10-22 P. Meszaros , M. J. Rees

The successful discovery of X-ray, optical and radio afterglows of gamma-ray bursts has significantly helped our understanding of these sources, and made possible the identification of host galaxies at cosmological distances. The energy…

天体物理学 · 物理学 2007-05-23 P. Meszaros

This article gives an overview of gamma-ray bursts (GRBs) and their relation to astroparticle physics and cosmology. GRBs are the most powerful explosions in the universe that occur roughly once per day and are characterized by flashes of…

高能天体物理现象 · 物理学 2019-02-27 Jakub Ripa

Nuclear physics offers us a powerful tool: using nuclear resonance absorption lines to infer the physical conditions in astrophysical settings which are otherwise difficult to deduce. Present-day technology provides an increase in…

天体物理仪器与方法 · 物理学 2009-02-23 J. Greiner , S. E. Boggs , G. DiCocco , K. T. Freese , N. Gehrels , D. H. Hartmann , A. Iyudin , G. Kanbach , A. A. Zdziarski

Gamma-ray bursts (GRBs) are sources of energetic, highly variable fluxes of gamma rays, which demonstrates that they are powerful particle accelerators. Besides relativistic electrons, GRBs should also accelerate high-energy hadrons, some…

天体物理学 · 物理学 2009-11-11 Charles D. Dermer , Armen Atoyan

Supercriticality of the same kind as that in a nuclear pile can take place in high-energy astrophysical objects producing a number of impressive effects. For example, it could cause an explosive release of the energy of a cloud of…

天体物理学 · 物理学 2011-03-10 Boris E. Stern , Juri Poutanen