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相关论文: Gamma-Ray Bursts via Pair Plasma Fireballs from He…

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A model is proposed for gamma-ray bursts based upon a neutrino burst of about 10^52 ergs lasting a few seconds above a heated collapsing neutron star. This type of thermal neutrino burst is suggested by relativistic hydrodynamic studies of…

天体物理学 · 物理学 2009-10-31 Jay D. Salmonson , James R. Wilson , Grant J. Mathews

We report on general relativistic hydrodynamic studies which indicate several new physical processes which may contribute to powering gamma-ray bursts in neutron star binaries. Relativistically driven compression, heating, and collapse of…

天体物理学 · 物理学 2007-05-23 G. J. Mathews , J. R. Wilson , J. Salmonson

In this paper we present a model for the short (< second) population of gamma-ray bursts (GRBs). In this model heated neutron stars in a close binary system near their last stable orbit emit neutrinos at large luminosities (~ 10^53…

天体物理学 · 物理学 2009-11-07 Jay D. Salmonson , James R. Wilson

It is proposed that gamma-ray bursts are created in the mergers of double neutron star binaries and black hole neutron star binaries at cosmological distances. Bursts with complex profiles and relatively long durations are the result of…

天体物理学 · 物理学 2009-10-22 Ramesh Narayan , Bohdan Paczyński , Tsvi Piran

In this paper we present a model for the short (< 1 second) population of gamma-ray bursts. In this model heated neutron stars in a close binary system near its last stable orbit emit a large amount of neutrinos (~10^53 ergs). A fraction of…

天体物理学 · 物理学 2009-11-07 Jay D. Salmonson , James R. Wilson

We propose a mechanism by which the neutrino emission from a supernova-type explosion can be converted into a gamma-ray burst of total energy $\sim 10^{50}$ ergs. This occurs naturally if the explosion is situated inside a ball of trapped…

天体物理学 · 物理学 2009-10-22 B. Holdom , R. A. Malaney

We discuss the possibility that the sources for gamma ray bursts are hot neutron stars at cosmological distance scales. The temperature of such stars would be $T \sim 1 \MeV$. Such hot stars can produce an electromagnetic blast wave…

天体物理学 · 物理学 2016-08-30 Henning Heiselberg , Sangyong Jeon , Larry McLerran , Hua-Bin Tang

The sudden release of copious $\g$-ray photons into a compact region creates an opaque photon--lepton fireball due to the prolific production of electron--positron pairs. The photons that we observe in the bursts emerge only at the end of…

天体物理学 · 物理学 2007-05-23 Tsvi Piran

We propose that spontaneous particle--anti-particle pair creations from the discharged vacuum caused by the strong interactions in dense matter are major sources of $\gamma$-ray bursts. Two neutron star collisions or black hole-neutron star…

天体物理学 · 物理学 2009-10-31 G. Mao , S. Chiba , W. Greiner , K. Oyamatsu

Numerous reports have been made of features, either in emission or absorption, in the 10 - 1000 keV spectra of some gamma-ray bursts. Originally interpreted in the context of Galactic neutron star models as cyclotron line emission and $e^+…

天体物理学 · 物理学 2009-10-31 C. J. Hailey , F. A. Harrison , K. Mori

Gamma-ray bursts (GRBs) are believed to originate from ultra-relativistic winds/fireballs to avoid the "compactness problem". However, the most energetic photons in GRBs may still suffer from $\gamma-\gamma$ absorption leading to…

天体物理学 · 物理学 2009-11-10 Zhuo Li , Z. G. Dai , T. Lu , L. M. Song

Observations imply that gamma-ray bursts (GRBs) are produced by the dissipation of the kinetic energy of a highly relativistic fireball. Photo-meson interactions of protons with gamma-rays within the fireball dissipation region are expected…

天体物理学 · 物理学 2007-05-23 Dafne Guetta

A pedagogical derivation is presented of the ``fireball'' model of gamma-ray bursts, according to which the observable effects are due to the dissipation of the kinetic energy of a relativistically expanding wind, a ``fireball.'' The main…

天体物理学 · 物理学 2016-04-13 E. Waxman

If gamma-ray bursts originate in our Galaxy, they probably involve violent disturbances in the magnetospheres of neutron stars. Any event of this kind is likely to trigger the sudden expulsion of magnetic flux and plasma at relativistic…

天体物理学 · 物理学 2016-06-08 Mitchell C. Begelman , P. Meszaros , Martin J. Rees

A fireball of radiation plasma created near the surface of a neutron star (NS) expands under its own pressure along magnetic field lines, and produces photon emission and relativistic matter outflow. We comprehensively classify the…

高能天体物理现象 · 物理学 2023-01-18 Tomoki Wada , Kunihito Ioka

Gamma-ray bursts are short-lived, luminous explosions at cosmological distances, thought to originate from relativistic jets launched at the deaths of massive stars. They are among the prime candidates to produce the observed cosmic rays at…

高能天体物理现象 · 物理学 2015-10-15 Mauricio Bustamante , Philipp Baerwald , Kohta Murase , Walter Winter

Observations suggest that $\gamma$-ray bursts (GRBs) are produced by the dissipation of the kinetic energy of a relativistic fireball. We show that a large fraction, $\ge 10%$, of the fireball energy is expected to be converted by…

天体物理学 · 物理学 2009-10-30 Eli Waxman , John Bahcall

Gamma-ray bursts have the potential to produce the particle energies (up to $10^{21}$ eV) and the energy budget ($10^{44} \rm{erg yr^{-1} Mpc^{-3}}$) to accommodate the spectrum of the highest energy cosmic rays; on the other hand, there is…

高能天体物理现象 · 物理学 2014-11-20 J. K. Becker , F. Halzen , A. O'Murchadha , M. Olivo

$\gamma$-ray bursts have baffled theorists ever since their accidental discovery at the sixties. We suggest that these bursts originate in merger of neutron star binaries, taking place at cosmological distances. These mergers release…

天体物理学 · 物理学 2009-10-22 Tsvi Piran

We consider the physics of neutrinos in a fireball, i.e. a tightly coupled plasma of photons, positrons and electrons. Such a fireball is believed to form in the first stages of a gamma-ray burst. We assume the fireball is…

天体物理学 · 物理学 2007-05-23 Hylke B. J. Koers , Ralph A. M. J. Wijers
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