Reduction of the geometrical mass of the Reissner-Nordstrom spacetime

被引：5

作者：

Barbachoux, C

Gariel, J

Marcilhacy, G

Santos, NO

机构：

[1] Univ Paris 06, CNRS, LRM, UMR 8540,ERGA, F-75005 Paris 05, France

[2] Lab Nacl Computacao Cient, BR-25651070 Petropolis, RJ, Brazil

[3] Ctr Brasileiro Pesquisas Fis, BR-22290180 Rio De Janeiro, Brazil

来源：

INTERNATIONAL JOURNAL OF MODERN PHYSICS D | 2002年 / 11卷 / 08期

关键词：

D O I：

10.1142/S0218271802002311

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We derive the Teixeira, Wolk and Som method,(1) for obtaining electrostatic solutions from some given vacuum solutions, in its inverse form. Then We use it to obtain the geometrical mass M-S in the Schwarzschild spacetime, and we find M-S(2) = M-2 - Q(2), S where M and Q are, respectively, the mass and charge parameters of the Reissner-Nordstrom spacetime. We compare M-S to the corresponding active gravitational mass and mass function.

引用

页码：1255 / 1263

页数：9

共 37 条

[1] A SIMPLE-MODEL OF A SUPERNOVA [J].