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...
        Saved in:
      
    
          | Published in | Chinese physics C Vol. 32; no. 6; pp. 428 - 432 | 
|---|---|
| Main Author | |
| Format | Journal Article | 
| Language | English | 
| Published | 
            IOP Publishing
    
        01.06.2008
     Institute of Theoretical Physics, China West Normal University, Nanchong 637002, China  | 
| Subjects | |
| Online Access | Get full text | 
| ISSN | 1674-1137 0254-3052 2058-6132  | 
| DOI | 10.1088/1674-1137/32/6/003 | 
Cover
| 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 |