Rigidly rotating dust in general relativity
J.C.N. de Araujo (DAS/Inpe), A. Wang (DFT/Uerj)
TL;DR
This paper presents an exact solution to Einstein's field equations describing a rigidly rotating dust configuration with an accompanying thin matter shell, advancing understanding of rotating matter distributions in general relativity.
Contribution
It introduces a new exact solution for rigidly rotating dust with a thin shell, expanding the set of known solutions in general relativity.
Findings
Exact solution for rotating dust with a thin shell
Insights into matter distribution in rotating spacetimes
Potential applications in astrophysical modeling
Abstract
A solution to the Einstein field equations that represents a rigidly rotating dust accompanied by a thin matter shell of the same type is found.
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