Entropy of the stiffest stars

被引:11
作者
Banks, T [1 ]
Fischler, W
Kashani-Poor, A
McNees, R
Paban, S
机构
[1] Univ Calif Santa Cruz, Dept Phys, Santa Cruz, CA 95064 USA
[2] Univ Calif Santa Cruz, Inst Particle Phys, Santa Cruz, CA 95064 USA
[3] Rutgers State Univ, Dept Phys & Astron, NHETC, Piscataway, NJ 08855 USA
[4] Univ Texas, Dept Phys, Austin, TX 78712 USA
基金
美国国家科学基金会;
关键词
D O I
10.1088/0264-9381/19/18/307
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We analyse the properties of stars whose interior is described by the stiffest equation of state consistent with causality. We note the remarkable fact that the entropy of such stars scales like the area.
引用
收藏
页码:4717 / 4728
页数:12
相关论文
共 18 条
[1]  
[Anonymous], GRQC9310026
[2]  
BANKS T, 2001, HEPTH0111142
[3]  
Banks T., HEPTH0102077
[5]  
BOUSSO R, 2002, HEPTH0203101
[6]  
FISCHLER W, 1998, HEPTH9806039
[7]  
Harrison B.K., 1965, GRAVITATION THEORY G
[8]   SINGULAR HYPERSURFACES AND THIN SHELLS IN GENERAL RELATIVITY [J].
ISRAEL, W .
NUOVO CIMENTO B, 1966, 44 (01) :1-&
[9]  
Misner C.W., 1970, GRAVITATION
[10]   HIGH-DENSITY BEHAVIOR + DYNAMICAL STABILITY OF NEUTRON STAR MODELS [J].
MISNER, CW ;
ZAPOLSKY, HS .
PHYSICAL REVIEW LETTERS, 1964, 12 (22) :635-&