WIGGLY STRINGS OF RADIAL CONFIGURATION IN THE KERR BLACK HOLE

被引：1

作者：

Suzuki, Hiromi ^{[1
]}

机构：

[1] Tokyo Womans Christian Univ, Coll Arts & Sci, Suginami Ku, Tokyo 1678585, Japan

来源：

MODERN PHYSICS LETTERS A | 2011年 / 26卷 / 26期

关键词：

Wiggly string; Kerr black hole; AXISYMMETRICAL SPACETIMES; COSMIC STRINGS; DYNAMICS;

D O I：

10.1142/S0217732311036425

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Previously we investigated classical motion of a string in (3 + 1)-dimensional spherically symmetric neutral and charged black holes. As an extension the solutions in (3 + 1)-dimensional axially symmetric rotating black hole are investigated. The solutions for the wiggly string exhibit. open strings lying in the radial direction in the equatorial plane outside the horizon.

引用

页码：1933 / 1942

页数：10

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