Astronomy and Astrophysics – Astrophysics
Scientific paper
2006-08-10
Nucl.Phys.A782:418-425,2007
Astronomy and Astrophysics
Astrophysics
8 pages, 7 figures, Proceedings of "Fifth International Conference on Perspectives in Hadronic Physics", Trieste 2006
Scientific paper
10.1016/j.nuclphysa.2006.10.024
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.
Drago Alessandro
Pagliara Giuseppe
Parenti Irene
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