Published February 1, 2007 | Version v1
Journal article

Quark Deconfinement inside Compact Stars and Gamma Ray Bursts Inner Engine

  • 1. Dipartimento di Fisica - Universita di Ferrara and INFN Sez. di Ferrara, Via Saragat, 1 - 44100 Ferrara (Italy)

Description

The temporal structure of Gamma Ray Bursts can be interpreted assuming as a inner engine a neutron star which undergoes a progressive compactification via production of strangeness (hyperons and kaons) and quarks. We will propose a tentative identification of various emission periods of the burst with specific structural changes of the star. Each of these modifications of the composition of the compact star takes place as a deflagration and not as a detonation, so the energy released in the transition goes mainly into heat and not into a mechanical wave. This is important in order to avoid an excessive baryonic contamination of the region surrounding the compact star. In this way a ultrarelativistic plasma of electron-positron pairs and of photons can be obtained, powering the Gamma Ray Burst

Additional details

Identifiers

DOI
10.1016/j.nuclphysa.2006.10.024;
arXiv
arXiv:astro-ph/0608224v1;
PII
S0375-9474(06)00728-7;

Publishing Information

Journal Title
Nuclear Physics. A
Journal Volume
782
Journal Issue
1-4
Journal Page Range
p. 418-425
ISSN
0375-9474
CODEN
NUPABL

Conference

Title
Particle-nucleus and nucleus-nucleus scattering at relativistic energies
Acronym
5. international conference on perspectives in hadron physics
Dates
22-26 May 2006
Place
Trieste (Italy)

Optional Information

Copyright
Copyright (c) 2006 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.