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Related papers: Gamma-Ray Bursts from Neutron Star Kicks

200 papers

As a new kind of radio transient sources detected at $\sim 1.4$ GHz, fast radio bursts are specially characterized by their short durations and high intensities. Although only ten events are detected so far, fast radio bursts may actually…

High Energy Astrophysical Phenomena · Physics 2015-12-22 Y. F. Huang , J. J. Geng

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…

Astrophysics · Physics 2016-08-30 Henning Heiselberg , Sangyong Jeon , Larry McLerran , Hua-Bin Tang

The consistence of the distributions of pulsar's kick velocities from the model of GRB and from the pulsar observations is tested based on the supernova-GRB ($\gamma$-ray burst) association and under the assumption that the GRB asymmetric…

Astrophysics · Physics 2009-11-13 X. H. Cui , H. G. Wang , R. X. Xu , G. J. Qiao

The little we do know of the physical conditions in gamma-ray bursters makes them conducive to the acceleration of high-energy cosmic rays, especially if they are at cosmological distances. We find that, with the observed statistics and…

Astrophysics · Physics 2008-11-26 Mordehai Milgrom , Vladimir Usov

We consider the early cooling evolution of strongly magnetized strange stars in a CFL phase with high gap Delta > 100 MeV. We demonstrate how this model may explain main features of the gamma-ray burst phenomena and also yield a strong star…

Astrophysics · Physics 2009-11-11 J. Berdermann , D. Blaschke , H. Grigorian , D. N. Voskresensky

Fast radio bursts are mysterious millisecond-duration transients prevalent in the radio sky. Rapid accumulation of data in recent years has facilitated an understanding of the underlying physical mechanisms of these events. Knowledge gained…

High Energy Astrophysical Phenomena · Physics 2020-11-11 Bing Zhang

It is no longer necessary to `sell' the idea of pulsar kicks, the notion that neutron stars receive a large velocity (a few hundred to a thousand km s$^{-1}$) at birth. However, the origin of the kicks remains mysterious. We review the…

Astrophysics · Physics 2016-01-27 Dong Lai

Many neutron stars are observed to be moving with spatial velocities, in excess of 500km/s. A number of mechanisms have been proposed to give neutron stars these high velocities. One of the leading classes of models proposed invokes…

Astrophysics · Physics 2009-11-10 Chris L. Fryer

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…

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…

Astrophysics · Physics 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…

Astrophysics · Physics 2008-11-26 Z. Berezhiani , I. Bombaci , A. Drago , F. Frontera , A. Lavagno

Gamma-ray bursts are violent events occurring randomly in the sky. In this review, I will present the fireball model, proposed to explain the phenomenon of gamma-ray bursts. This model has important consequences for the production and…

Astrophysics · Physics 2008-07-25 B. Gendre

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,…

Astrophysics · Physics 2009-11-07 Melvyn B. Davies , Andrew King , Stephan Rosswog , Graham Wynn

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…

Astrophysics · Physics 2009-10-31 Aiichi Iwazaki

The gamma ray burst phenomenon is reviewed from a theoretical point of view, with emphasis on the fireball shock scenario of the prompt emission and the longer wavelenght afterglow. Recent progress and issues are discussed, including…

Astrophysics · Physics 2009-11-07 P. Meszaros

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…

Astrophysics · Physics 2009-10-31 Jay D. Salmonson , James R. Wilson , Grant J. Mathews

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…

Astrophysics · Physics 2008-02-03 Nir J. Shaviv , Arnon Dar

Conversion from neutron stars to strange stars as a possible mechanism of cosmological gamma-ray bursts (GRBs) has been discussed in previous works, although the existence of strange stars is still an open question. On the basis of this…

Astrophysics · Physics 2007-05-23 X. Y. Wang , Z. G. Dai , T. Lu , D. M. Wei , Y. F. Huang

Gamma-ray bursts are the most luminous explosions in the Universe, whose origin and mechanism is the focus of intense interest. They appear connected to supernova remnants from massive stars or the merger of their remnants, and their…

High Energy Astrophysical Phenomena · Physics 2015-06-11 Peter Mészáros , Neil Gehrels

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…

Astrophysics · Physics 2009-10-22 B. Holdom , R. A. Malaney