THERMAL CONDUCTION AND THE STABILITY OF SELF-GRAVITATING SPHERES

被引：3

作者：

HERRERA, L

JIMENEZ, J

BARRETO, W

ESCULPI, M

LEDENMAT, G

SANTOS, NO

机构：

[1] UNIV ORIENTE,ESCUELA CIENCIAS NUCL SUCRE,DEPT FIS,CUMANA,VENEZUELA

[2] CENT UNIV VENEZUELA,FAC PHYS SOLIDES,DEPT FIS APLICADA,CARACAS,VENEZUELA

[3] INST POINCARE,PHYS THEOR LAB,F-75231 PARIS 05,FRANCE

[4] OBSERV NACL,CTR NACL PESQUISAS,DEPT ASTRON,RIO DE JANEIRO,BRAZIL

来源：

ASTROPHYSICS AND SPACE SCIENCE | 1990年 / 165卷 / 02期

关键词：

D O I：

10.1007/BF00653289

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Recent calculations (analytical and semi-analytical), indicating that thermal effects in the relativistic regime may enhance the stability of spherically-symmetric models, are confirmed in a new example. © 1990 Kluwer Academic Publishers.

引用

页码：211 / 218

页数：8

共 6 条

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JIMENEZ, J ;

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[3] EVOLUTION OF RADIATING FLUID SPHERES IN GENERAL-RELATIVITY [J].

HERRERA, L ;

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[4]

HERRERA L, 1990, MON NOT R ASTRON SOC, V237, P257

[5]

LANDAU L, 1959, FLUID MECHANICS, P9

[6] Static solutions of Einstein's field equations for spheres of fluid [J].

Tolman, RC .

PHYSICAL REVIEW, 1939, 55 (04) :0364-0373

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