pith. sign in

arxiv: gr-qc/0305016 · v1 · pith:QP6ONFU6new · submitted 2003-05-04 · 🌀 gr-qc

Note on Matter Collineations in Kantowski-Sachs, Bianchi Types I and III Spacetimes

classification 🌀 gr-qc
keywords spacetimesbianchicollineationskantowski-sachsmattertypescamcieinstein
0
0 comments X
read the original abstract

We show that the classification of Kantowski-Sachs, Bianchi Types I and III spacetimes admitting Matter Collineations (MCs) presented in a recent paper by Camci et al. [Camci, U., and Sharif, M. {Matter Collineations in Kantowski-Sachs, Bianchi Types I and III Spacetimes}, 2003 Gen. Relativ. Grav. vol. 35, 97-109] is incomplete. Furthermore for these spacetimes and when the Einstein tensor is non-degenerate, we give the complete Lie Algebra of MCs and the algebraic constraints on the spatial components of the Einstein tensor.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.