Loading…

Kantowski–Sachs metrics with source: A massless scalar field

Solutions of the coupled Einstein massless scalar field equation are discussed under the assumption that the metric belongs to the ‘‘Kantowski–Sachs’’ class of metrics. More precisely, the general solution of the coupled Einstein massless scalar field equations is derived under the following assumpt...

Full description

Saved in:
Bibliographic Details
Published in:Journal of mathematical physics 1992-04, Vol.33 (4), p.1415-1419
Main Authors: Xanthopoulos, Basilis C., Zannias, Thomas
Format: Article
Language:English
Subjects:
Citations: Items that this one cites
Items that cite this one
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
Description
Summary:Solutions of the coupled Einstein massless scalar field equation are discussed under the assumption that the metric belongs to the ‘‘Kantowski–Sachs’’ class of metrics. More precisely, the general solution of the coupled Einstein massless scalar field equations is derived under the following assumptions: (a) The scalar field is massless minimally coupled to gravity and obeys the Klein–Gordon equation; and (b) the metric belongs to the spherical Kantowski–Sachs class of metrics. The main feature of the results is a tractable, very simple, compact form of the space‐time metric. This is accomplished by expressing the solution in a special coordinate gauge. An analysis of the geometry shows the presence of curvature singularities which consist of a spacelike part and a null part. The spacelike singularity appears to ‘‘squeeze’’ the SO(3) orbits to zero proper area while simultaneously stretching their proper separation to infinity length. The null part appears to squeeze to zero values both SO(3) orbits and their proper separation as well. There also exists a subclass of metrics for which the singularity structure is different. The null singularity is replaced by a spacelike part. Both ‘‘initial’’ and ‘‘final’’ singularities exhibit the same qualitative features and they are of finite proper time away from each other.
ISSN:0022-2488
1089-7658
DOI:10.1063/1.529717