English
Related papers

Related papers: Gamma-Ray Bursts From Neutron Star Phase Transitio…

200 papers

We identify a novel physical mechanism that may be responsible for energy release in $\gamma$-ray bursts. Radial perturbations in the neutron core, induced by its collision with collapsing outer layers during the early stages of supernova…

High Energy Astrophysical Phenomena · Physics 2015-06-04 Anastasios Avgoustidis , Raul Jimenez , Luis Alvarez-Gaume , Miguel A. Vazquez-Mozo

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…

High Energy Astrophysical Phenomena · Physics 2024-08-06 Cecilia Lunardini , Joshua Loeffler , Mainak Mukhopadhyay , Matthew J. Hurley , Ebraheem Farag , F. X. Timmes

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…

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

We study the conversion of a neutron star to a strange star as a possible energy source for gamma-ray bursts. We use different recent models for the equation of state of neutron star matter and strange quark matter. We show that the total…

Astrophysics · Physics 2009-10-31 Ignazio Bombaci , Bhaskar Datta

(Abridged) We interpret gamma ray bursts as relativistic, electromagnetic explosions. Specifically, we propose that they are created when a rotating, relativistic, stellar-mass progenitor loses much of its rotational energy in the form of a…

Astrophysics · Physics 2007-05-23 Maxim Lyutikov , Roger Blandford

In this contribution we briefly introduce a mechanism for short gamma ray burst emission different from the usually assumed compact object binary merger progenitor model. It is based on the energy release in the central regions of neutron…

High Energy Astrophysical Phenomena · Physics 2015-06-12 M. Angeles Perez-Garcia , Frederic Daigne , Joseph Silk

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…

Astrophysics · Physics 2016-06-08 Mitchell C. Begelman , P. Meszaros , Martin J. Rees

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…

Astrophysics · Physics 2007-05-23 G. J. Mathews , J. R. Wilson , J. Salmonson

Core collapse of massive stars and binary neutron stars or black hole-neutron star binary mergers are likely progenitors of long and short duration gamma-ray bursts respectively. Neutronized material in the former and neutron star material…

Astrophysics · Physics 2007-05-23 Soebur Razzaque , Peter Meszaros

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

The 'event' that triggers a gamma ray burst cannot last for more than a few seconds. This is, however, long compared with the dynamical timescale of a compact stellar-mass object ($\sim 10^{-3}$ seconds). Energy is assumed to be released as…

Astrophysics · Physics 2009-10-22 M. J. Rees , P. Meszaros

The idea that gamma-ray bursts might be a kind of phenomena associated with neutron star kicks was first proposed by Dar & Plaga (1999). Here we study this mechanism in more detail and point out that the neutron star should be a high speed…

Astrophysics · Physics 2009-11-07 Y. F. Huang , Z. G. Dai , T. Lu , K. S. Cheng , X. F. Wu

We present a new model for gamma-ray bursts (GRBs) that are not only associated with supernovae but also have small baryon contamination. In this model, we assume a newborn neutron star to move outward at a kick velocity of $\sim 10^3 {\rm…

Astrophysics · Physics 2007-05-23 K. S. Cheng , Z. G. Dai

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…

Astrophysics · Physics 2008-11-26 S. E. Woosley , Weiqun Zhang

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

We describe observational evidence and theoretical calculations which support the high velocity neutron star model of gamma-ray bursts. We estimate the energetic requirements in this model, and discuss possible energy sources. we also…

Astrophysics · Physics 2009-10-28 Donald Q. Lamb , Tomasz Bulik , Paolo S. Coppi

We exploit the fact that General Theory of Relativity (GTR) predicts the existence of compact objects having surface gravitational redshift z_s < =z_c=0.615 when the Equation of State (EOS) has the stringest general constraint that the…

Astrophysics · Physics 2007-05-23 Abhas Mitra

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…

High Energy Astrophysical Phenomena · Physics 2015-10-15 Mauricio Bustamante , Philipp Baerwald , Kohta Murase , Walter Winter

It is known that Neutron Stars may be converted into more compact Strange Stars (SS) on capture/formation of a ``seed'' of strange matter. It is also known that the binding energy of the nascent hot SS is likely to be radiated as $\nu…

Astrophysics · Physics 2007-05-23 Abhas Mitra

We study the dynamical evolution of a phase-transition-induced collapse neutron star to a hybrid star, which consists of a mixture of hadronic matter and strange quark matter. The collapse is triggered by a sudden change of equation of…

High Energy Astrophysical Phenomena · Physics 2015-05-13 K. S. Cheng , T. Harko , Y. F. Huang , L. M. Lin , W. M. Suen , X. L. Tian
‹ Prev 1 2 3 10 Next ›