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相关论文: Gamma-Ray Bursts and Quantum Cosmic Censorship

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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

We propose that the cosmological gamma ray bursts arise from the collapse of neutron stars to black holes triggered by collisions or mergers with main sequence stars. This scenario represents a cosmological history qualitatively different…

天体物理学 · 物理学 2009-10-30 Brad M. S. Hansen , Chigurupati Murali

The origin of cosmic gamma-ray bursts remains one of the most intriguing puzzles in astronomy. We suggest that purely general relativistic effects in the collapse of massive stars could account for these bursts. The late formation of closed…

广义相对论与量子宇宙学 · 物理学 2016-12-21 Pankaj Joshi , Naresh Dadhich , Roy Maartens

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

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

We propose that repeated photoexcitation/ionization of high Z atoms of highly relativistic flows by star light in dense stellar regions followed by emission of decay/recombination photons, which are beamed and boosted to gamma ray energies…

天体物理学 · 物理学 2008-02-03 Nir J. Shaviv , Arnon Dar

$\gamma$-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

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

We suggest that the collapsing core of a massive rotating star may fragment to produce two or more compact objects. Their coalescence under gravitational radiation gives the resulting black hole or neutron star a significant kick velocity,…

天体物理学 · 物理学 2009-11-07 Melvyn B. Davies , Andrew King , Stephan Rosswog , Graham Wynn

$\gamma$-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 2007-05-23 Tsvi Piran

We indicate a possible mechanism of generating gamma ray bursts. They are generated by a collision between an axionic boson star and a neutron star. The axionic boson star can dissipates its whole energy $10^{50}$ erg in the magnetized…

天体物理学 · 物理学 2009-10-31 Aiichi Iwazaki

Cosmological GRBs are discussed with an emphasis on their plausible connection with black holes. GRBs can be triggered by collapse of stellar-mass objects that leads to formation of a black hole and a transient debris disk with a huge…

天体物理学 · 物理学 2008-11-26 Andrei M. Beloborodov

Gamma-ray bursts are believed to be the most luminous objects in the Universe. There has been some suggestion that these arise from quantum processes around naked singularities. The main problem with this suggestion is that all known…

广义相对论与量子宇宙学 · 物理学 2015-06-25 H. M. Antia

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

I summarize recent results about how a neutron star binary coalescence can produce short gamma-ray bursts (GRBs). Two possibilities are discussed: the annihilation of neutrino anti-neutrino pairs above the merged remnant and the exponential…

天体物理学 · 物理学 2010-11-11 S. Rosswog

Binary neutron stars merger (NS$^2$M) at cosmological distances is probably the only $\gamma$-ray bursts model based on an independently observed phenomenon which is known to be taking place at a comparable rate. We describe this model, its…

天体物理学 · 物理学 2015-06-24 T. Piran

We propose a model to explain how a Gamma Rays Burst can take place days or years after a supernova explosion. Our model is based on the conversion of a pure hadronic star (neutron star) into a star made at least in part of deconfined quark…

天体物理学 · 物理学 2008-11-26 Z. Berezhiani , I. Bombaci , A. Drago , F. Frontera , A. Lavagno

We propose that the gravitational collapse of supermassive objects ($ M\ga 10^4 M_\odot$), either as relativistic star clusters or as single supermassive stars (which may result from stellar mergers in dense star clusters), could be a…

天体物理学 · 物理学 2016-08-30 George M. Fuller , Xiangdong Shi

Gamma-ray bursts are characterized by a duration of milliseconds to several minutes in which an enormous amount of radiation is emitted. The origin of these phenomena is still unknown because proposed models fail to explain all the observed…

天体物理学 · 物理学 2009-10-30 Simon Portegies Zwart

The properties of the cosmic Gamma-ray Bursts (GRBs) are briefly summarized. A detailed bibliography is given with titles of the papers. Two fundamental theoretical problems are pointed out: the problem of the energy source, and the problem…

天体物理学 · 物理学 2015-06-24 S. Blinnikov
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