Rotating and twisting locally rotationally symmetric imperfect fluids

Abstract

Rotating and twisting locally rotationally symmetric imperfect fluids in general relativity admit a much larger set of solutions than the self-similar ones recently suggested in the literature. Explicit forms of the metrics are given and the self-similar sub-cases are discussed.

6 pages, corrected several typos, added comments

References in corpus (3)

• Cosmological models from a geometric point of view
• New class of LRS spacetimes with simultaneous rotation and spatial twist
• Rotating and twisting locally rotationally symmetric spacetimes: a general solution

Cited by in corpus (3)

• Existence of gradient CKV and gradient conformally stationary LRS spacetimes
• Quantum Kasner transition in a locally rotationally symmetric Bianchi II universe
• Gradient conformal stationarity and the CMC condition in LRS spacetimes