A connection between Rastall-type and f(R, T) gravities
arXiv:2003.02064 · doi:10.1209/0295-5075/129/20004
Abstract
Recently a Lagrangian formulation for Rastall Gravity (RG) has been proposed in the framework of f(R, T) gravity. In the present work we obtain Lagrangian formulation for the standard Rastall theory assuming the matter content is a perfect fluid with linear Equation of State (EoS). We therefore find a relation between the coupling constant of the Lagrangian, the Rastall gravitational coupling constant and the EoS parameter. We also propose a Lagrangian for the Generalized Rastall Gravity (GRG). In this case the Rastall parameter which is a constant is replaced by a variable one. More exactly, it appears as a function of the Ricci scalar and the trace of the Energy Momentum Tensor (EMT). In both mentioned models, the Lagrangians are constructed by a linear function of R and T.
12 pages,
References in corpus (11)
- f(R,T) gravity
- Einstein and Rastall Theories of Gravitation in Comparison
- Dark Matter From f(R,T) Gravity
- Accelerated cosmos in a non-extensive setup
- Limits on Gravity from Earth's Atmosphere
- The Brans-Dicke-Rastall theory
- Wormhole Solutions in Rastall Gravity Theory
- Propagation of Polar Gravitational Waves in f(R,T) Scenario
- Gravitational Collapse in Rastall Gravity
- The commutator algebra of covariant derivative as general framework for extended gravity. The Rastall theory case and the role of the torsion
- On Gödel-type Solution in Rastall's Gravity