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

近期发现有不法分子冒充我刊与作者联系，借此进行欺诈等不法行为，请广大作者加以鉴别，如遇诈骗行为，请第一时间与我刊编辑部联系确认（《中国物理C》（英文）编辑部电话：010-88235947,010-88236950），并作报警处理。

本刊再次郑重声明：

（1）本刊官方网址为cpc.ihep.ac.cn和https://iopscience.iop.org/journal/1674-1137

（2）本刊采编系统作者中心是投稿的唯一路径，该系统为ScholarOne远程稿件采编系统，仅在本刊投稿网网址（https://mc03.manuscriptcentral.com/cpc）设有登录入口。本刊不接受其他方式的投稿，如打印稿投稿、E-mail信箱投稿等，若以此种方式接收投稿均为假冒。

（3）所有投稿均需经过严格的同行评议、编辑加工后方可发表，本刊不存在所谓的“编辑部内部征稿”。如果有人以“编辑部内部人员”名义帮助作者发稿，并收取发表费用，均为假冒。

《中国物理C》（英文）编辑部

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

Abstract
HTML
Reference
Related

PDF

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

[1]	Chao Wang , Yujiang Bi , Hao Cai , Ying Chen , Ming Gong , Zhaofeng Liu . Quark chiral condensate from the overlap quark propagator. Chinese Physics C, 2017, 41(5): 053102. doi: 10.1088/1674-1137/41/5/053102
[2]	J. H. Field . A comparison of direct and indirect determinations of the masses of the Higgs Boson and the top quark. Chinese Physics C, 2017, 41(10): 103001. doi: 10.1088/1674-1137/41/10/103001
[3]	QIN Zhen-Xing , TANG Ling-Yun , LIU Jing , CHEN Xiao-Jia . Phase transitions in a hydrogen-rich compound：tetramethylsilane. Chinese Physics C, 2013, 37(9): 098001. doi: 10.1088/1674-1137/37/9/098001
[4]	ZHANG Xiao-Li , WU Ye , ZHANG Qian , DONG Jun-Cai , WU Xiang , LIU Jing , WU Zi-Yu , CHEN Dong-Liang . Pressure-induced phase transitions of multiferroic BiFeO₃. Chinese Physics C, 2013, 37(12): 128001. doi: 10.1088/1674-1137/37/12/128001
[5]	SUN Yan-Jun , WANG Zhi-Gang , HUANG Tao . B → A transitions in the light-cone QCD sum rules with the chiral current. Chinese Physics C, 2012, 36(11): 1046-1054. doi: 10.1088/1674-1137/36/11/003
[6]	CHEN Shi-Wu , GAO Li , PENG Guang-Xiong . One-gluon-exchange effect on the properties of quark matter and strange stars. Chinese Physics C, 2012, 36(10): 947-953. doi: 10.1088/1674-1137/36/10/005
[7]	ZHU Jing-Min . Quantum phase transitions about parity breaking in matrix product systems. Chinese Physics C, 2011, 35(2): 144-148. doi: 10.1088/1674-1137/35/2/007
[8]	LAI Xiao-Yu , XU Ren-Xin . Quark-clustering in cold quark matter. Chinese Physics C, 2010, 34(9): 1331-1334. doi: 10.1088/1674-1137/34/9/035
[9]	J. H. Kühn . Strong coupling, charm- and bottom-quark masses from electron-positron annihilation. Chinese Physics C, 2010, 34(6): 675-679. doi: 10.1088/1674-1137/34/6/011
[10]	Ulf-G. Meissner¹ , 2 . Isospin violation, light quark masses, and all that. Chinese Physics C, 2010, 34(9): 1163-1168. doi: 10.1088/1674-1137/34/9/003
[11]	CHEN Yan , MA Bo-Qiang . Octet baryon masses with two-gluon exchange effect. Chinese Physics C, 2009, 33(12): 1362-1365. doi: 10.1088/1674-1137/33/12/055
[12]	YANG Fang , SHEN Hong . Influence of the nuclear equation of state on the hadron-quark phase transition in neutron stars. Chinese Physics C, 2008, 32(7): 536-542. doi: 10.1088/1674-1137/32/7/005
[13]	WANG Hai-Jun , GENG Wen-Tong . Quark confinement and the fractional quantum Hall effect. Chinese Physics C, 2008, 32(9): 705-709. doi: 10.1088/1674-1137/32/9/006
[14]	YANG Fang , SHEN Hong . Hadron-quark phase transition in neutron stars. Chinese Physics C, 2008, 32(S2): 77-80.
[15]	Li Panlin , Wu Hua , Xu Mengjie . Dynamics of Phase Transition Including Quark-Fragment Effects for an Expansion Quark-Gluon Plasma. Chinese Physics C, 1997, 21(S4): 55-64.
[16]	Yu Youwen , Zhang Zongye , Shen Pengnian , Shen Xiaoyan . Effective Quark-Quark Interaction Created by Quark-Antiquark Pair Excitation. Chinese Physics C, 1992, 16(S4): 449-456.
[17]	Xing Zheng , Wu Xingju . Rotational Effect on Electromagnetic Transitions After Band-Crossing. Chinese Physics C, 1991, 15(S1): 93-100.
[18]	Xing Zheng , Chen Zingqu . Rotational Effect on Electromagnetic Transitions in Nuclei. Chinese Physics C, 1989, 13(S2): 213-219.
[19]	Jin Changhao . Down-Quark Masses and Flavor Mixing. Chinese Physics C, 1988, 12(S1): 59-68.
[20]	BAo GUAN-XIONG . GLAUBER QUARK MODEL WITH SPIN EFFECT. Chinese Physics C, 1981, 5(1): 141-144.

Access

Get Citation

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

RIS(for EndNote,Reference Manager,ProCite)

BibTex

Txt

Milestone

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

Article Metric

Article Views(1427)
PDF Downloads(606)
Cited by(0)

Policy on re-use

To reuse of subscription content published by CPC, the users need to request permission from CPC, unless the content was published under an Open Access license which automatically permits that type of reuse.

通讯作者: 陈斌, bchen63@163.com

1.
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.