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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 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

$\gamma$-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 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 propose a model in which ultra high energy cosmic rays and gamma ray bursts are produced by collisions between neutron stars and axion stars. The acceleration of such a cosmic ray is made by the electric field, $\sim 10^{15} (B/10^{12}…

高能物理 - 唯象学 · 物理学 2007-05-23 Aiichi Iwazaki

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 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

In this paper we model the emission from a relativistically expanding electron-positron pair plasma fireball originating near the surface of a heated neutron star. This pair fireball is deposited via the annihilation of neutrino pairs…

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

Gamma-ray bursts are believed to result from the coalescence of binary neutron stars. However, the standard proposals for conversion of the gravitational energy to thermal energy have difficulties. We show that if the merger of the two…

广义相对论与量子宇宙学 · 物理学 2015-06-25 T. P. Singh

The standard unbroken electroweak theory is known to erase baryon number. The baryon number symmetry can be restored in the core of a neutron star as its density diverges via gravitational instability due to a binary merger event. We argue…

天体物理学 · 物理学 2009-10-30 Ue-Li Pen , Abraham Loeb , Neil Turok

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

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

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

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 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

We propose a model in which ultra high energy cosmic rays are produced by collisions between neutron stars and axion stars. The acceleration of such a cosmic ray is made by the electric field, $\sim 10^{15} (B/10^{12} {G}) {eV} {cm}^{-1}$,…

高能物理 - 唯象学 · 物理学 2009-10-31 Aiichi Iwazaki

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

A gamma-ray burst (GRB) releases an amount of energy similar to that of a supernova explosion, which combined with its rapid variability suggests an origin related to neutron stars or black holes. Since these compact stellar remnants form…

天体物理学 · 物理学 2020-11-25 Ralph A. M. J. Wijers , Joshua S. Bloom , Jasjeet S. Bagla , Priyamvada Natarajan

Three-dimensional hydrodynamical simulations are presented for the direct head-on or off-center collision of two neutron stars, employing a basically Newtonian PPM code but including the emission of gravitational waves and their…

天体物理学 · 物理学 2007-05-23 Maximilian Ruffert , H. -Thomas Janka

The phase-transition induced collapse of a neutron star to a more compact configuration (typically a ``strange'' star) and the subsequent core bounce is often invoked as a model for gamma-ray bursts. We present the results of numerical…

天体物理学 · 物理学 2016-02-17 C. L. Fryer , S. E. Woosley
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