Bounding f(R,T) gravity by particle creation
arXiv:1908.07839 · doi:10.1142/S0219887819501536
Abstract
We consider the possibility of the quantum vacuum states in f(R,T) gravity. Particularly, we study the Bogoliubov transformations associated to different vacuum states for some f(R,T) models. The method consists of fixing the f(R,T) free parameters by requiring the Bogoliubov coefficients to be minimized. In such a way, the particle production is related to the value of the Hubble parameter and also the given f(R,T) model.
arXiv commentPublished online: Int. J. Geom. Methods Mod. Phys (2019)
References in corpus (18)
- Measurements of Omega and Lambda from 42 High-Redshift Supernovae
- Dynamics of dark energy
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic Results
- Cosmological parameters from SDSS and WMAP
- A Phantom Menace? Cosmological consequences of a dark energy component with super-negative equation of state
- f(R,T) gravity
- An alternative to quintessence
- Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
- Dark Energy and the Accelerating Universe
- Dark Matter and Dark Energy
- Can the Chaplygin gas be a plausible model for dark energy?
- Generalized energy conditions in Extended Theories of Gravity
- Cosmographic bounds on the cosmological deceleration-acceleration transition redshift in gravity
- Quantum Effects In Cosmology
- Initial and final de Sitter universes from modified gravity
- Vacuum Choices and the Predictions of Inflation
- Space-Time Description of Scalar Particle Creation by a Homogeneous Isotropic Gravitational Field
- Bounding gravity by particle production rate