Slowly rotating scalar field wormholes: The second order approximation

被引:51
作者
Kashargin, P. E. [1 ]
Sushkov, S. V. [1 ,2 ]
机构
[1] Kazan VI Lenin State Univ, Dept Gen Relat & Gravitat, Kazan 420008, Russia
[2] Tatar State Univ Humanities & Educ, Dept Math, Kazan 420021, Russia
来源
PHYSICAL REVIEW D | 2008年 / 78卷 / 06期
关键词
D O I
10.1103/PhysRevD.78.064071
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We discuss rotating wormholes in general relativity with a scalar field with negative kinetic energy. To solve the problem, we use the assumption about slow rotation. The role of a small dimensionless parameter plays the ratio of the linear velocity of rotation of the wormhole's throat and the velocity of light. We construct the rotating wormhole solution in the second-order approximation with respect to the small parameter. The analysis shows that the asymptotical mass of the rotating wormhole is greater than that of the nonrotating one, and the null energy condition violation in the rotating wormhole spacetime is weaker than that in the nonrotating one.
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页数:10
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