EFFECT OF NUCLEAR CURVATURE ENERGY ON THE TRANSITION BETWEEN NUCLEI AND BUBBLES IN DENSE MATTER

被引:16
作者
PETHICK, CJ
RAVENHALL, DG
LATTIMER, JM
机构
[1] NORDITA,DK-2100 COPENHAGEN O,DENMARK
[2] SUNY STONY BROOK,DEPT EARTH & SPACE SCI,STONY BROOK,NY 11794
关键词
D O I
10.1016/0370-2693(83)90376-3
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
引用
收藏
页码:137 / 140
页数:4
相关论文
共 9 条
[1]   NEUTRON STAR MATTER [J].
BAYM, G ;
BETHE, HA ;
PETHICK, CJ .
NUCLEAR PHYSICS A, 1971, A175 (02) :225-&
[2]   A MEAN-FIELD CALCULATION OF THE EQUATION OF STATE OF SUPER-NOVA MATTER [J].
BONCHE, P ;
VAUTHERIN, D .
NUCLEAR PHYSICS A, 1981, 372 (03) :496-526
[3]  
BONCHE P, 1982, ASTRON ASTROPHYS, V112, P168
[4]   HOT DENSE MATTER AND STELLAR COLLAPSE [J].
LAMB, DQ ;
LATTIMER, JM ;
PETHICK, CJ ;
RAVENHALL, DG .
PHYSICAL REVIEW LETTERS, 1978, 41 (23) :1623-1626
[5]  
LAMB DQ, UNPUB NUCL PHYS
[6]  
LAMB DW, UNPUB
[7]   THE EQUATION OF STATE OF HOT DENSE MATTER AND SUPER-NOVAE [J].
LATTIMER, JM .
ANNUAL REVIEW OF NUCLEAR AND PARTICLE SCIENCE, 1981, 31 :337-374
[8]   NEUTRON STAR MATTER AT SUB-NUCLEAR DENSITIES [J].
NEGELE, JW ;
VAUTHERIN, D .
NUCLEAR PHYSICS A, 1973, A207 (02) :298-320
[9]  
RAVENHALL DG, UNPUB NUCL PHYS