EVOLUTION OF THE BEL-ROBINSON ENERGY IN GOWDY T3XR SPACE-TIMES

被引：6

作者：

ISENBERG, J

JACKSON, M

MONCRIEF, V

机构：

[1] YALE UNIV, DEPT PHYS, DEPT MATH, NEW HAVEN, CT 06511 USA

[2] UNIV PARIS 12, F-94010 CRETEIL, FRANCE

[3] UNIV OREGON, INST THEORET SCI, DEPT PHYS, EUGENE, OR 97403 USA

来源：

JOURNAL OF MATHEMATICAL PHYSICS | 1990年 / 31卷 / 02期

关键词：

D O I：

10.1063/1.528885

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

The evolution of the Bel-Robinson (BR) energy in Gowdy T 3×ℝ space-times is studied. It is found that a quantity closely related to the BR energy decreases monotonically as the space-time evolves toward the final singularity, except in the special case of Kasner data where this quantity is constant. © 1990 American Institute of Physics.

引用

页码：517 / 519

页数：3

共 7 条

[1]

BEL L, 1959, CR HEBD ACAD SCI, V248, P1297

[2]

DESER S, 1987, GRAVITATION GEOMETRY, P115

[3] VACUUM SPACETIMES WITH 2-PARAMETER SPACE-LIKE ISOMETRY GROUPS AND COMPACT INVARIANT HYPERSURFACES - TOPOLOGIES AND BOUNDARY-CONDITIONS [J].