Propagation of Scalar Fields in a Plane Symmetric Spacetime

被引:1
|
作者
Celestino, Juliana [1 ]
Alves, Marcio E. S. [2 ]
Barone, F. A. [3 ]
机构
[1] Univ Estado Rio De Janeiro, Dept Phys, R Sao Francisco Xavier 524, BR-20550900 Rio De Janeiro, RJ, Brazil
[2] UNESP, Inst Ciencia & Tecnol, BR-12247004 Sao Jose Dos Campos, SP, Brazil
[3] Univ Fed Itajuba, IFQ, Ave BPS 1303, BR-37500903 Itajuba, Brazil
基金
巴西圣保罗研究基金会;
关键词
Gravitational waves; Taub metric; Scalar field; COSMOLOGICAL CONSTANT; GENERAL-RELATIVITY; UNIVERSE;
D O I
10.1007/s13538-016-0458-8
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
The present article deals with solutions for a minimally coupled scalar field propagating in a static plane symmetric spacetime. The considered metric describes the curvature outside a massive infinity plate and exhibits an intrinsic naked singularity (a singular plane) that makes the accessible universe finite in extension. This solution can be interpreted as describing the spacetime of static domain walls. In this context, a first solution is given in terms of zero order Bessel functions of the first and second kind and presents a stationary pattern which is interpreted as a result of the reflection of the scalar waves at the singular plane. This is an evidence, at least for the massless scalar field, of an old interpretation given by Amundsen and Gron regarding the behaviour of test particles near the singularity. A second solution is obtained in the limit of a weak gravitational field which is valid only far from the singularity. In this limit, it was possible to find out an analytic solution for the scalar field in terms of the Kummer and Tricomi confluent hypergeometric functions.
引用
收藏
页码:784 / 792
页数:9
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