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Gamma Ray Bursts (GRBs) are unpredictable and brief flashes of gamma rays that occur about once a day in random locations in the sky. Since gamma rays do not penetrate the Earth's atmosphere, they are detected by satellites, which…

高能天体物理现象 · 物理学 2015-06-05 A. Gomboc

The cosmological gamma-ray burst (GRB) phenomenon is reviewed. The broad observational facts and empirical phenomenological relations of the GRB prompt emission and afterglow are outlined. A well-tested, successful fireball shock model is…

天体物理学 · 物理学 2007-05-23 Bing Zhang , Peter Meszaros

The recent progress in studies of gamma-ray bursts, their afterglows, and host galaxies is discussed. The emphasis is given to high-energy phenomena associated with gamma-ray burst explosions: high-energy cosmic rays, neutrinos,…

天体物理学 · 物理学 2007-05-23 K. A. Postnov

Understanding of the nature of gamma-ray bursts (GRBs) is one of the challenging problem facing the astrophysics community. The field of gamma ray bursts is a rapidly developing one and we expect that new missions, like SWIFT and GLAST will…

天体物理学 · 物理学 2008-11-26 A. Lazarian , V. Petrosian , H. Yan , J. Cho

Cosmic explosions called $\gamma$-ray bursts are the most energetic bursting events in the universe. Observations of extremely high-energy emission from two $\gamma$-ray bursts provide a new way to study these gigantic explosions.

高能天体物理现象 · 物理学 2020-01-08 Bing Zhang

The observational diversity of ``gamma-ray bursts'' (GRBs) has been increasing, and the natural inclination is a proliferation of models. We explore the possibility that at least part of this diversity is a consequence of a single basic…

天体物理学 · 物理学 2008-11-26 S. E. Woosley , Weiqun Zhang

We discuss some open problems concerning the origin and the emission mechanism of gamma-ray bursts (GRBs) in light of recent developments. If GRBs originate at extragalactic distances, we are facing four crises: (1) an energy crisis, models…

天体物理学 · 物理学 2007-05-23 Marco Tavani

Long gamma-ray bursts (GRBs) are believed to be related to the explosion of type Ic supernovae, which have been stripped of their hydrogen and helium envelopes. There appear to be two types of these explosions: those which are approximately…

天体物理学 · 物理学 2009-11-10 B. Paczynski , P. Haensel

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

Gamma Ray Bursts (GRBs) are among the most powerful sources in the Universe: they emit up to 10^54 erg in the hard X-ray band in few tens of seconds. The cosmological origin of GRBs has been confirmed by several spectroscopic measurements…

天体物理学 · 物理学 2011-07-19 G. Ghirlanda , G. Ghisellini , C. Firmani

When a star undergoes core collapse, a vast amount of energy is released in a ~10 s long burst of neutrinos of all species. Inverse beta decay in the star's hydrogen envelope causes an electromagnetic cascade which ultimately results in a…

高能天体物理现象 · 物理学 2024-08-06 Cecilia Lunardini , Joshua Loeffler , Mainak Mukhopadhyay , Matthew J. Hurley , Ebraheem Farag , F. X. Timmes

Astrophysical explosions result from the release of magnetic, gravitational, or thermonuclear energy on dynamical timescales, typically the sound-crossing time for the system. These explosions include solar and stellar flares, eruptive…

高能天体物理现象 · 物理学 2015-06-03 J. Craig Wheeler

Since their first discovery in the late 1960s, Gamma-ray bursts have attracted an exponentially growing interest from the international community due to their central role in the most highly debated open questions of the modern research of…

Very high energy, short wavelength, neutrinos may interact with the space-time foam predicted by theories of quantum gravity. They would propagate like light through a crystal lattice and be delayed, with the delay depending on the energy.…

高能物理 - 唯象学 · 物理学 2009-11-11 M. C. Gonzalez-Garcia , F. Halzen

Mirror matter models have been suggested recently as an explanation of neutrino puzzles and microlensing anomalies. We show that mirror supernovae can be a copious source of energetic gamma rays if one assumes that the quantum gravity scale…

天体物理学 · 物理学 2011-05-23 R. N. Mohapatra , S. Nussinov , V. L. Teplitz

A complete model for the origin of high-energy >~10^{14} eV) cosmic rays from gamma-ray bursts (GRBs) and implications of this hypothesis are described. Detection of high-energy neutrinos from GRBs provide an unambiguous test of the model.…

天体物理学 · 物理学 2010-11-11 C. Dermer

The internal/external synchrotron shock scenario has proved very successful in interpreting the key observations about gamma ray bursts. There still remains, however, some big uncertainties. The hottest issue concerns the nature of the…

天体物理学 · 物理学 2007-05-23 G. Ghisellini

We discuss the possibility that gamma-ray bursts may result from cosmological relativistic blob emitting neutron star jets that precess past the line of sight. Beaming reduces the energy requirements, so that the jet emission can last…

天体物理学 · 物理学 2009-10-28 Eric G. Blackman , Insu Yi , George B. Field

The origin of energetic gamma-ray bursts is still unknown. But the detection of polarization of gamma-rays provides fresh insight into the mechanism driving these powerful explosions.

天体物理学 · 物理学 2009-11-07 E. Waxman

I argue that cosmic Gamma-ray Bursts (GRB) may be produced by collapses or mergers of stars made of `mirror' matter. The mirror neutrinos (which are sterile for our matter) produced at these events can oscillate into ordinary neutrinos. The…

天体物理学 · 物理学 2007-05-23 S. Blinnikov