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Raychaudhuri Equations, Tidal Forces, and the Weak-Field Limit in Schwarzshild–Finsler–Randers Spacetime.

Authors :
Triantafyllopoulos, Alkiviadis
Kapsabelis, Emmanuel
Stavrinos, Panayiotis C.
Source :
Universe (2218-1997). Jan2024, Vol. 10 Issue 1, p26. 20p.
Publication Year :
2024

Abstract

In this article, we study the form of the deviation of geodesics (tidal forces) and the Raychaudhuri equation in a Schwarzschild–Finsler–Randers (SFR) spacetime which has been investigated in previous papers. This model is obtained by considering the structure of a Lorentz tangent bundle of spacetime and, in particular, the kind of the curvatures in generalized metric spaces where there is more than one curvature tensor, such as Finsler-like spacetimes. In these cases, the concept of the Raychaudhuri equation is extended with extra terms and degrees of freedom from the dependence on internal variables such as the velocity or an anisotropic vector field. Additionally, we investigate some consequences of the weak-field limit on the spacetime under consideration and study the Newtonian limit equations which include a generalization of the Poisson equation. [ABSTRACT FROM AUTHOR]

Details

Language :
English
ISSN :
22181997
Volume :
10
Issue :
1
Database :
Academic Search Index
Journal :
Universe (2218-1997)
Publication Type :
Academic Journal
Accession number :
175132362
Full Text :
https://doi.org/10.3390/universe10010026