Effects of the density dependence of the symmetry energy on neutron stars

  • In this paper, we include the density dependence behavior of the symmetry energy in the improved quark mass density dependent (IQMDD) model. Under the mean field approximation, this model is applied to investigate neutron star matter and neutron stars successfully. Effects of the density dependence of the symmetry energy on neutron
    stars are described.

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  • [1] CHEN Lie-Wen et al.Phys.Rev.C,2007,76:054316[2] LI Z H et al.Phys.Rev.C,2006,74:047304[3] Krastev P,Sammarruca F.Phys.Rev.C,2006,74:025808[4] XIAO Zhi-Cang,LI Bao-An,Chen Lie-Wen,YONG Gao-Chan,ZHANG Ming.Phys.Rev.Lett.,2009,102:062502[5] LI Bao-An.Nucl.Phys.A,2003,722:209c-214c;Huu Phat Tran,Anh Nguyen Tuan,Long Nguyen Van.Phys.Rev.C,2008,77:054321[6] Guichon P A M.Phys.Lett.B,1988,200:235[7] WU Chen,SU Ru-Keng.J.Phys.,2008,Nucl.Part.Phys.,G35:125001[8] WU Chen,SU Ru-Keng.J.Phys.,2009,Nucl.Part.Phys.,G36:095101[9] WU Chen,QIAN Wei-Liang,SU Ru-Keng.Phys.Rev.C,2005,72:035205[10] WU Chen,QIAN Wei-Liang,SU Ru-Keng.Chin.Phys.Lett.,2005,22:1866-1869[11] Horowitz C J,Piekarewicz J.Phys.Rev.C,2001,64:062802(R)[12] CHEN Lie-Wen,Ko CHE Ming,LI Bao-An.Phys.Phys.C,2005,72:064309;Phys.Rev.Lett.,2005,94:032701[13] WU Chen,QIAN Wei-Liang,SU Ru-Keng.Phys.Rev.C,2008,77:015203[14] Pickarewicz J.Phys.Phys.C,2002,60:034305[15] Avancini S S,Marinelli J R,Menezes D P,Moraes M M W,Providência C.Phys.Rev.C,2007,75:055805[16] Typel S,Wolter H H.Nucl.Phys.A,1999,656:331[17] TSANG M B,ZHANC Ying-Xun,Anielewicz P D,Famiano M,LI Zhu-Xia,Lynch W G,Steiner A W.Phys.Rev.Lett.,2009,102:122701[18] Serot B D,Walecka J D.Adv.Nucl.Phys.,1986,16:1[19] LI Bao-An.Phys.Rev.Lett.,2002,88:19[20] Lenske H,Fuchs C.Phys.Lett.B,1995,345:355[21] Fuchs C,Lenske H,Wolter H H.Phys.Rev.C,1995,52:6[22] Than Hoang Sy,T.Khoa Dao,Giai Nguyen Van.Phys.Rev.C,2009,80:064312[23] Warda M,Vias X,Roca-Maza X,Centelles M.Phys.Rev.C,2009,80:024316[24] Nakada H.Phys.Rev.C,2008,78:054301[25] Todd-Rutel B G,Piekarewicz J.Phys.Rev.Lett.,2005,95:122501[26] FU Wei-Jie,WEI Hai-Qing,LIU Yu-Xin.Phys.Rev.Lett.,2008,101:181102[27] Kubis S,Kutschera M.Phys.Lett.B,1997,399:191-195[28] Khoa D T,Than H S.Phys.Rev.C,2005,71:044601
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LIU Xiao-Jin, WU Chen and REN Zhong-Zhou. Effects of the density dependence of the symmetry energy on neutron stars[J]. Chinese Physics C, 2010, 34(11): 1709-1713. doi: 10.1088/1674-1137/34/11/008
LIU Xiao-Jin, WU Chen and REN Zhong-Zhou. Effects of the density dependence of the symmetry energy on neutron stars[J]. Chinese Physics C, 2010, 34(11): 1709-1713.  doi: 10.1088/1674-1137/34/11/008 shu
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Received: 2010-02-01
Revised: 2010-03-22
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Effects of the density dependence of the symmetry energy on neutron stars

    Corresponding author: REN Zhong-Zhou,

Abstract: 

In this paper, we include the density dependence behavior of the symmetry energy in the improved quark mass density dependent (IQMDD) model. Under the mean field approximation, this model is applied to investigate neutron star matter and neutron stars successfully. Effects of the density dependence of the symmetry energy on neutron
stars are described.

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