Big Bang Nucleosynthesis and Entropy Evolution in Gravity
arXiv:2004.04684 · doi:10.1140/epjp/s13360-020-00361-4
Abstract
The present article is devoted to constrain the model parameter for the gravity model by employing the constraints coming from big bang nucleosynthesis. We solve the field equations and constrain in the range (where ) from the primordial abundances of light elements such as helium-4, deuterium and lithium-7. We found the abundances of helium-4 and deuterium agrees with theoretical predictions, however the lithium problem persists for the gravity model. We also investigate the evolution of entropy for the constrained parameter space of for the radiation and dust universe. We report that entropy is constant when for the radiation dominated universe, whereas for the dust universe, entropy increases with time. We finally use the constraints to show that has negligible influence on the cold dark matter annihilation cross section.
8 pages, 3 figures, Accepted version at European Physical Journal Plus
References in corpus (13)
- Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
- f(R,T) gravity
- Primordial Nucleosynthesis in the Precision Cosmology Era
- The Primordial Lithium Problem
- Thermodynamic interpretation of the generalized gravity models with geometry - matter coupling
- Modelling wormholes in gravity
- Dark Matter From f(R,T) Gravity
- Non-exotic matter wormholes in a trace of the energy-momentum tensor squared gravity
- Wormholes in -gravity within the formalism
- Constraining The Early-Universe Baryon Density And Expansion Rate
- Propagation of Polar Gravitational Waves in f(R,T) Scenario
- Baryogenesis in Nonminimally Coupled Theories
- Temporally Varying Universal Gravitational "Constant" and Speed of Light in Energy Momentum Squared Gravity