Distribution of Energy-Momentum in a Schwarzschild-Quintessence Space-Time Geometry

被引：1

作者：

Radinschi, Irina ^{[1
]}

Grammenos, Theophanes ^{[2
]}

Spanou, Andromahi ^{[3
]}

机构：

[1] Gh Asachi Tech Univ, Dept Phys, Iasi 700050, Romania

[2] Univ Thessaly, Dept Civil Engn, Volos 38334, Greece

[3] Natl Tech Univ Athens, Sch Appl Math & Phys Sci, Athens 15780, Greece

来源：

INTERNATIONAL JOURNAL OF THEORETICAL PHYSICS | 2013年 / 52卷 / 11期

关键词：

Energy-momentum complexes; Schwarzschild black hole; Dark energy; Quintessence; QUASI-NORMAL MODES; BLACK-HOLE; ANGULAR-MOMENTUM; GENERAL-RELATIVITY; STATIONARY BEAM; LOCALIZATION; PRINCIPLE;

D O I：

10.1007/s10773-013-1724-y

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

An analysis of the energy-momentum localization for a four-dimensional Schwarzschild black hole surrounded by dark energy in the form of quintessence is presented in order to provide expressions for the distributions of energy and momentum. The calculations are performed by using the Landau-Lifshitz and the Weinberg energy-momentum complexes. It is shown that all the momenta vanish, while the expression for the energy depends on the mass M of the black hole, the state parameter w (q) and the normalization factor c. The special case of is studied and some limiting cases are examined.

引用

页码：4100 / 4109

页数：10

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