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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.

参考文献

[1] CHEN Lie-Wen et al.[J].Physical Review C:Nuclear Physics,2007,76:054316.
[2] LI Z H et al.[J].Physical Review C:Nuclear Physics,2006,74:047304.
[3] Krastev P;Sammarruca F .[J].Physical Review C:Nuclear Physics,2006,74:025808.
[4] XIAO Zhi-Cang;LI Bao-An;Chen Lie-Wen;YONG Gao-Chan ZHANG Ming .[J].Physical Review Letters,2009,102:062502.
[5] LI Bao-An .[J].Nuclear Physics A,2003,722:209c-214c.
[6] Huu Phat Tran;Anh Nguyen Tuan;Long Nguyen Van .[J].Physical Review C:Nuclear Physics,2008,77:054321.
[7] Guichon P A M .[J].Physics Letters B,1988,200:235.
[8] WU Chen;SU Ru-Keng .[J].J Phys Nucl Part Phys,2008,G35:125001.
[9] WU Chen;SU Ru-Keng .[J].J Phys Nucl Part Phys,2009,G36:095101.
[10] WU Chen;QIAN Wei-Liang;SU Ru-Keng .[J].Physical Review C:Nuclear Physics,2005,72:035205.
[11] WU Chen,QIAN Wei-Liang,SU Ru-Keng.Improved Quark Mass Density-Dependent Model with Non-Linear Scalar Interaction[J].中国物理快报(英文版),2005(08):1866-1869.
[12] Horowitz C J;Piekarewicz J .[J].Physical Review C:Nuclear Physics,2001,64:062802(R).
[13] CHEN Lie-Wen;Ko CHE Ming;LI Bao-An .[J].Phys Phys C,2005,72:064309.
[14] [J].Physical Review Letters,2005,94:032701.
[15] WU Chen;QIAN Wei-Liang;SU Ru-Keng .[J].Physical Review C:Nuclear Physics,2008,77:015203.
[16] Pickarewicz J .[J].Phys Phys C,2002,60:034305.
[17] Avancini S S;Marinelli J R;Menezes D P;Moraes M M W Provid(e)ncia C .[J].Physical Review C:Nuclear Physics,2007,75:055805.
[18] Typel S;Wolter H H .[J].Nuclear Physics A,1999,656:331.
[19] TSANG M B;ZHANC Ying-Xun;Anielewicz P D;Famiano M LI Zhu-Xia Lynch W G Steiner A W .[J].Physical Review Letters,2009,102:122701.
[20] Serot B D;Walecka J D .[J].Advances in Nuclear Physics,1986,16:1.
[21] LI Bao-An .[J].Physical Review Letters,2002,88:19.
[22] Lenske H;Fuchs C .[J].Physics Letters B,1995,345:355.
[23] Fuchs C;Lenske H;Wolter H H .[J].Physical Review C:Nuclear Physics,1995,52:6.
[24] Than Hoang Sy;T.Khoa Dao;Giai Nguyen Van .[J].Physical Review C:Nuclear Physics,2009,80:064312.
[25] Warda M;Vi(n)as X;Roca-Maza X;Centelles M .[J].Physical Review C:Nuclear Physics,2009,80:024316.
[26] Nakada H .[J].Physical Review C:Nuclear Physics,2008,78:054301.
[27] Todd-Rutel B G;Piekarewicz J .[J].Physical Review Letters,2005,95:122501.
[28] FU Wei-Jie;WEI Hai-Qing;LIU Yu-Xin .[J].Physical Review Letters,2008,101:181102.
[29] Kubis S;Kutschera M .Nuclear matter in relativistic mean field theory with isovector scalar meson[J].Physics Letters, B. Nuclear Physics and High Energy Physics,1997(3/4):191-195.
[30] Khoa D T;Than H S .[J].Physical Review C:Nuclear Physics,2005,71:044601.
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