ACKNOWLEDGMENT This work was supported in part by the National Natural Science Foundation of China (Grant No. 10675064). [1] F. Weber, Prog. Part. Nucl. Phys. 54 , 193 (2005). [2] H. Heiselberg and M. Hjorth-Jensen, Phys. Rep. 328 , 237 (2000). [3] J. M. Lattimer and M. Prakash, Phys. Rep. 442 , 109 (2007). [4] J. Schaffner and I. N. Mishustin, Phys. Rev. C 53 , 1416 (1996). [5] S. Pal, M. Hanauske, I. Zakout, H. St¨ ocker, and W. Greiner, Phys. Rev. C 60 , 015802 (1999). [6] P. K. Panda, D. P. Menezes, and C. Providencia, Phys. Rev. C 69 , 025207 (2004). [7] H. Shen, Phys. Rev. C 65 , 035802 (2002). [8] N. K. Glendenning, Phys. Rev. C 64 , 025801 (2001). [9] D. B. Kaplan and A. E. Nelson, Phys. Lett. B175 , 57 (1986). [10] P. Yue and H. Shen, Phys. Rev. C 77 , 045804 (2008). [11] F. Yang and H. Shen, Phys. Rev. C 77 , 025801 (2008). [12] M. Buballa, Phys. Rep. 407 , 205 (2005). [13] I. Shovkovy, M. Hanauske, and M. Huang, Phys. Rev. D 67 , 103004 (2003). [14] M. Huang, P. Zhuang, and W. Chao, Phys. Rev. D 67 , 065015 (2003). [15] D. J. Dean and M. Hjorth-Jensen, Rev. Mod. Phys. 75 , 607 (2003). [16] D. Page, M. Prakash, J. M. Lattimer, and A. W. Steiner, Phys. Rev. Lett. 85 , 2048 (2000). [17] S. Balberg, I. Lichtenstadt, and G. B. Cook, Astrophys. J. Suppl. Ser. 121 , 515 (1999). [18] C. Ishizuka, A. Ohnishi, K. Tsubakihara, K. Sumiyoshi, and S. Yamada, J. Phys. G 35 , 085201 (2008). [19] P. Yue, F. Yang, and H. Shen, Phys. Rev. C 79 , 025803 (2009). [20] S. Balberg and N. Barnea, Phys. Rev. C 57 , 409 (1998). [21] T. Takatsuka and R. Tamagaki, Prog. Theor. Phys. 102 , 1043 (1999). [22] T. Takatsuka and R. Tamagaki, Nucl. Phys. A670 , 222c (2000). [23] T. Tanigawa, M. Matsuzaki, and S. Chiba, Phys. Rev. C 68 , 015801 (2003). [24] T. Takatsuka, S. Nishizaki, Y. Yamamoto, and R. Tamagaki, Prog. Theor. Phys. 115 , 355 14