Paper · Feb 23, 2024
Characterizations of generalized Robertson-Walker spacetimes concerning gradient solitons
As on arXiv
Abstract
In this article, we examine gradient type Ricci solitons and -quasi Einstein solitons in generalized Robertson-Walker () spacetimes. Besides, we demonstrate that in this scenario the spacetime presents the Robertson-Walker () spacetime and the perfect fluid () spacetime presents the phantom era. Consequently, we show that if a spacetime permits a gradient - Einstein solitons, then it also represents a spacetime under certain condition.
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Background reading
The guides for the topics of this paper: what each idea is, why it matters, and the papers to read first.
In the guidebook
- 11B.1Ricci Solitons
Self-similar solutions: the Gaussian, cylinders, the cigar and the Bryant soliton.
- 12B.2The Asymptotic Soliton and Three-Dimensional Shrinkers
Perelman's Proposition 11.2 proved with Morgan and Tian: the reduced-length bounds on κ-solutions, the limit of rescalings, the equality case, and the classification of shrinking solitons in dimensions two and three.