Effect of current quark masses on quark phase transitions in supernovae

LAI Xiang-Jun; LUO Zhi-Quan; LIU Hong-Lin

doi:10.1088/1674-1137/32/6/003

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2024年10月30日

Chinese Physics C> 2008, Vol. 32> Issue(6) : 428-432 DOI: 10.1088/1674-1137/32/6/003

Effect of current quark masses on quark phase transitions in supernovae

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Abstract：
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.

References

[1]

. Witten E. Phys. Rev. D, 1984, 30: 2722. Madsen J. Lect. Notes Phys., 1999, 516: 1623. LUO Z Q, PENG Q H. Acta. Phys. Sin., 2001, 42: 3024. LUO Z Q, LIU M Q, LIN L B et al. Chin. Phys., 2005, 14:12725. Kotake K, Sato K, Takahashi K. Rept. Prog. Phys., 2006,69: 9716. Hong D K, Hsu S D H, Sannino F. Phys. Lett. B, 2001,516: 3627. Drago A, Lavagno A, Pagliara G. Phys. Rev. D, 2004, 69:0575058. DAI Z G, PENG Q H, LU T. Astrophys. J., 1995, 440: 8159. Anand J D, Goyal A, Gupta V K et al. Astrophys. J., 1997,481: 95410. Gentile N A, Aufderheide M B, Mathews G J. Astrophys.J., 1993, 414: 70111. BAO T, LIU G Z, ZHU M F et al. HEP NP, 2006, 30:961. (in Chinese)12. Heiselberg H. Phys. Scr., 1992, 46: 48513. Madsen J. Phys. Rev. D, 1993, 47: 32514. Mason Q, Trottier H D, Horgan R et al. Phys. Rev. D,2006, 73: 450115. Baron E A, Cooperstein J. Astrophys. J., 1990, 353: 59716. Burrows A, Mazurek T J, Lattimer J M. Astrophys. J.,1981, 251: 35217. Mayle R W, Tavani M, Rwilson J. Astrophys. J., 1993, 418:39818. Kernen P, Ouyed R, Jaikumar P. Astrophys. J., 2005, 618:485

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LAI Xiang-Jun, LUO Zhi-Quan and LIU Hong-Lin. Effect of current quark masses on quark phase transitions in supernovae[J]. Chinese Physics C, 2008, 32(6): 428-432. doi: 10.1088/1674-1137/32/6/003

LAI Xiang-Jun, LUO Zhi-Quan and LIU Hong-Lin. Effect of current quark masses on quark phase transitions in supernovae[J]. Chinese Physics C, 2008, 32(6): 428-432. doi: 10.1088/1674-1137/32/6/003 shu

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Received: 2007-03-23
Revised: 2008-02-16

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沈阳化工大学材料科学与工程学院沈阳 110142

Effect of current quark masses on quark phase transitions in supernovae

Corresponding author: LAI Xiang-Jun,

Received Date: 2007-03-23
Accepted Date: 2008-02-16
Available Online: 2008-06-05

Abstract:

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.