Matter--Geometry interplay in new scalar tensor theories of gravity
The paper studies the possible interplay between matter and geometry in scalar tensor theories of gravitation where the energy--momentum tensor is directly coupled with the Einstein tensor. After obtaining the scalar tensor representation of the $f(R, G_{\mu\nu}T^{\mu\nu})$ gravity, the analysis con...
Saved in:
Main Author | |
---|---|
Format | Journal Article |
Language | English |
Published |
06.10.2024
|
Subjects | |
Online Access | Get full text |
Cover
Loading…
Summary: | The paper studies the possible interplay between matter and geometry in
scalar tensor theories of gravitation where the energy--momentum tensor is
directly coupled with the Einstein tensor. After obtaining the scalar tensor
representation of the $f(R, G_{\mu\nu}T^{\mu\nu})$ gravity, the analysis
continue with an approach based on the thermodynamics of irreversible processes
in open systems. To this regard, various thermodynamic properties are directly
obtained in this manner, like the matter creation (annihilation) rate and the
corresponding creation (annihilation) pressure. In the case of the
Roberson--Walker metric several analytic and numerical solutions are found in
the asymptotic regime. In the last part of the manuscript a specific
parametrization for the Hubble rate is constrained using the Markov Chain Monte
Carlo algorithms in the case of cosmic chronometers (CC) and BAO observations,
obtaining an approximate numerical solution which can describe the cosmological
model. For this model, we have obtained by fine--tuning some numerical
solutions which exhibit creation mechanisms in different specific regimes. |
---|---|
DOI: | 10.48550/arxiv.2410.04584 |