RELATIVISTIC RADIATIVE-TRANSFER FOR SPHERICAL FLOWS

被引：29
|
作者：
REZZOLLA, L
MILLER, JC
机构：
[1] UNIV OXFORD,DEPT PHYS,OXFORD,ENGLAND
[2] OSSERV ASTRON TRIESTE,TRIESTE,ITALY
来源：
CLASSICAL AND QUANTUM GRAVITY | 1994年 / 11卷 / 07期
关键词：
D O I：
10.1088/0264-9381/11/7/018
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We present a new complete set of Lagrangian relativistic hydrodynamical equations describing the transfer of energy and momentum between a standard fluid and a radiation fluid in a general non-stationary spherical flow. The new set of equations has been derived for a particular application in the study of the cosmological quark-hadron transition, but can also be used in other contexts.
引用
收藏
页码：1815 / 1832
页数：18
相关论文
共 50 条
12345