Effect of current quark masses on quark phase transitions in supernovae

The current quark mass model is adopted to study the phase transition of two-flavor quark matter to more stable three-flavor quark matter in the whole core of a supernova. It shows that the timescale of the process is shorter than 10^-8 seconds, that'the u-and d-quark masses can be neglected complet...

Full description

Saved in:
Bibliographic Details
Published inChinese physics C Vol. 32; no. 6; pp. 428 - 432
Main Author 赖祥军 罗志全 刘宏林
Format Journal Article
LanguageEnglish
Published IOP Publishing 01.06.2008
Institute of Theoretical Physics, China West Normal University, Nanchong 637002, China
Subjects
Online AccessGet full text
ISSN1674-1137
0254-3052
2058-6132
DOI10.1088/1674-1137/32/6/003

Cover

More Information
Summary:The current quark mass model is adopted to study the phase transition of two-flavor quark matter to more stable three-flavor quark matter in the whole core of a supernova. It shows that the timescale of the process is shorter than 10^-8 seconds, that'the u-and d-quark masses can be neglected completely in this model, and that the temperature and the total neutrino energies in the core after the conversion increase nearly by 40% and 20% on the average compared with former results, respectively. The last result can further enhance the probability of success for a supernova explosion significantly.
Bibliography:11-5641/O4
TM933
O572.2
quark phase transition, current quark mass, supernova
ISSN:1674-1137
0254-3052
2058-6132
DOI:10.1088/1674-1137/32/6/003