On the moment of inertia of a proto neutron star

[1]
Burrows A,Lattimer J M.Ap.J,1986,307:178-196[2] Glendenning N K.Ap.J,1995,448:797-802[3] Hartle J B.Ap.J,1967,150:1005-1029[4] Hartle J B,Thorne K S.Ap.J,1968,153:807-834[5] Link B,Epstein R I,Lattimer J M.Phys.Rev.Lett.,1999,83(17):3362-3365[6] LI Wen-Fei,ZHANG Feng-Shou,CHEN Lie-Wen.HEP NP,2001,25(10):1006-1011(in Chinese)[7] Bejger M,Bulik T,Haensel P.MNRAS,2005,364:1-6[8] ZUO Wei,Lombardo U.HEP NP,2002,26(11):1134-1141(in Chinese)[9] ZUO Wei,CHEN Ji-Yan,LI Bao-An et al.HEP NP,2005,29(9):881-885(in Chinese)[10] ZHOU Shan-Gui.HEP NP,2004,28(Supp.):21-26(in Chinese)[11] Schaffner J,Dover C B,Gal A et al.Ann.Phys.(N.Y.),1994,235:35-76[12] Glendening N K.Nucl.Phys.A,1987,469:600-616[13] ZHAO Xian-Feng,WANG Shun-Jin,ZHANG Hua et al.HEP NP,2007,31(6):532-537(in Chinese)[14] Glendenning N K.Ap.J,1985,293:470[15] Schaffner J,Dover C B,Gal Aet al.Phys.Rev.Lett.,1993,71:1328-1331[16] Glendenning N K.Compact Stars:Nuclear Physics,Particle Physics,and General Relativity.New York:SpringerVerlag New York,Inc.,1997.232-233