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《中国物理C》(英文)编辑部
2024年10月30日

One-gluon-exchange effect on the properties of quark matter and strange stars

  • We present a modified version of quark mass scaling via considering the important one-gluon-exchange interaction between quarks in the quark mass density-dependent model. The properties of strange quark matter and the structure of strange stars are then studied with the new scaling and a self-consistent thermodynamic treatment. It is found that the one-gluon-exchange effect lowers the system energy considerably, makes the equation of state stiffer, and the sound velocity tends to the ultra-relativistic value faster, which make the biggest value of the maximum mass of strange stars become as big as approximately 2 times the solar mass, in accordance with the latest astronomical observations.
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  • [1] Bodmer A R. Phys. Rev. D, 1971, 4: 1601[2] Witten E. Phys. Rev. D, 1984, 30: 272[3] Farhi E, Jaffe R L. Phys. Rev. D, 1984, 30: 2379[4] Madsen J, Jensen Dan M, Christiansen M B. Phys. Rev. D, 1993, 47: 5156; Phys. Rev. D, 1994, 50: 3328; Phys. Rev. C, 1996, 53: 1883[5] PENG Guang-Xiong, NING Ping-Zhi, CHIANG Huan-Ching. Phys. Rev. C, 1997, 56: 491[6] PENG Guang-Xiong et al. Phys. Rev. C, 1999, 59: 3452[7] Parija B C. Phys. Rev. C, 2003, 48: 2483[8] WEN Xin-Jian et al. Phys. Rev. C, 2010, 82: 025809[9] Madsen J. Phys. Rev. Lett., 1998, 81: 3311[10] For a recent review, see Weiner R M. Int. J. Mod. Phys. E, 2006, 15: 37, and quoted therein[11] PENG Guang-Xiong et al. Phys. Rev. C, 1999, 61: 015201[12] PENG Guang-Xiong, CHIANG Huan-Ching, NING Ping-Zhi. Phys. Rev. C, 2000, 62: 025801[13] WANG Ping. Phys. Rev. C, 2000, 62: 015204[14] ZHANG Yun, SU Ru-Keng. Phys. Rev. C, 2002, 65: 035202[15] WEN Xin-Jian et al. Phys. Rev. C, 2005, 72: 015204[16] MAO H et al. Phys. Rev. C, 2006, 74: 055204[17] WU Chen et al. Phys. Rev. C, 2008, 77: 015203[18] YIN Shao-Yu, SU Ru-Keng. Phys. Rev. C, 2008, 77: 055204[19] PENG Guang-Xiong, LI Ang, Lomberto U. Phys. Rev. C, 2008, 77: 065807[20] Fowler G N, Raha S, Weiner R M. Z. Phys. C, 1981, 9: 271[21] Chakrabarty S, Raha S, Sinha B. Phys. Lett. B, 1989, 229: 112; Chakrabaty S. Phys. Rev. D, 1991, 43: 627; Phys. Rev. D, 1993, 48: 1409[22] Benvenuto O G, Lugones G. Phys. Rev. D, 1995, 51: 1989; Lugones G, Benvenuto O G, 1995, 52: 1276[23] WEN Xin-Jian, PENG Guang-Xiong, CHEN Yue-De. J. Phys. G, 2007, 34: 1697[24] WEN Xin-Jian, PENG Guang-Xiong, SHEN Peng-Nian. Int. J. Mod. Phys. A, 2007, 22: 1649[25] Modarres M, Gholizade H. Int. J. Mod. Phys. E, 2008, 17: 1335[26] ZHANG Yun et al. Europhys. Lett., 2001, 56: 361; ZHANG Yun, SU Ru-Keng. Phys. Rev. C, 2003, 67: 015202[27] PENG Guang-Xiong et al. Int. J. Mod. Phys. A, 2003, 18: 3151[28] CHEN Shi-Wu, PENG Guang-Xiong. Commun. Theor. Phys., 2012, 57: 1037[29] YAO W M et al. J. Phys. G, 2006, 33: 1[30] Shirkov D V, Solovtsov I L. JINR Rapid Commun., 1996, 76: 5[31] LAI Xiao-Yu, XU Ren-Xin. Mon. Not. R. Astron. Soc., 2009, 398: L31—L35[32] LAI Xiao-Yu, XU Ren-Xin. Astroparticle Physics, 2009, 31: 128[33] Freire P C C et al. The Astrophysical Journal, 2008, 679: 1433[34] LI Ang et al. Mon. Not. R. Astron. Soc., 2010, 402: 2715[35] Demorest P et al. Nature, 2010, 467: 1081
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CHEN Shi-Wu, GAO Li and PENG Guang-Xiong. One-gluon-exchange effect on the properties of quark matter and strange stars[J]. Chinese Physics C, 2012, 36(10): 947-953. doi: 10.1088/1674-1137/36/10/005
CHEN Shi-Wu, GAO Li and PENG Guang-Xiong. One-gluon-exchange effect on the properties of quark matter and strange stars[J]. Chinese Physics C, 2012, 36(10): 947-953.  doi: 10.1088/1674-1137/36/10/005 shu
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Received: 2012-02-24
Revised: 1900-01-01
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One-gluon-exchange effect on the properties of quark matter and strange stars

Abstract: We present a modified version of quark mass scaling via considering the important one-gluon-exchange interaction between quarks in the quark mass density-dependent model. The properties of strange quark matter and the structure of strange stars are then studied with the new scaling and a self-consistent thermodynamic treatment. It is found that the one-gluon-exchange effect lowers the system energy considerably, makes the equation of state stiffer, and the sound velocity tends to the ultra-relativistic value faster, which make the biggest value of the maximum mass of strange stars become as big as approximately 2 times the solar mass, in accordance with the latest astronomical observations.

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