Thermodynamic Behavior of Time-Dependent Wormholes in Palatini Gravity
arXiv:2101.06372 · doi:10.1007/s10714-020-02773-0
Abstract
In the frame work of Palatini approach to modified theories of gravity, we attempt to investigate the thermodynamic behavior of time-dependent wormhole geometries. By considering an evolving wormhole spacetime, we find the field equations in Palatini gravity. The energy density and pressure are redefined in order to satisfy the continuity equation. To discuss the thermodynamic behavior, an expression for the variation of total entropy is obtained. Then, we extend our discussions to apparent and event horizons of evolving wormholes. We employ the radius of apparent and event horizons to determine the validity of generalized second law (GSL) of thermodynamics which states that the variation of total entropy is non-negative.
References in corpus (9)
- Palatini Approach to Modified Gravity: f(R) Theories and Beyond
- Thermodynamic route to Field equations in Lanczos-Lovelock Gravity
- Traversable wormholes in gravity with constant and variable redshift functions
- Evolving Lorentzian wormholes supported by phantom matter and cosmological constant
- Noether Charge and Black Hole Entropy in Modified Theories of Gravity
- Time-Dependent Wormhole Solutions of Theory of Gravity and Energy Conditions
- Correspondence between Jordan-Einstein frames and Palatini-metric formalisms
- Thermodynamics of Evolving Lorentzian Wormholes at Apparent Horizon in Theory of Gravity
- Entropy of Microwave Background Radiation in Observable Universe