Thermodynamics of irreversible particle creation phenomena and its cosmological consequence
arXiv:1708.04857 · doi:10.1007/978-3-319-70957-4_8
Abstract
The study of particle creation phenomena at the expense of the gravitational field is of great research interest. It might solve the cosmological puzzle single-handedly, without the need for either dark energy or the modified theory of gravity. In the early universe, following graceful exit from inflationary phase, it serves the purpose of reheating the cold universe, which gave way to the hot Big-Bang model. In the late universe, it led to late time cosmic acceleration, without affecting stand-ard Big-Bang-Nucleosynthesis (BBN), Cosmic Microwave Background Radiation (CMBR), or Structure Formation. In this chapter, we briefly review the present status of cosmic evolution, develop the thermodynamics for irreversible particle creation phenomena and study its consequences at the early as well as in the late universe.
28 pages, 3 figures, To appear in 'CFD Technics and Thermo-Mechanics Applications', Springer, Chapter - N0
References in corpus (22)
- Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
- Unified cosmic history in modified gravity: from F(R) theory to Lorentz non-invariant models
- Modified f(R) gravity consistent with realistic cosmology: from matter dominated epoch to dark energy universe
- Cosmological viability of f(R)-gravity as an ideal fluid and its compatibility with a matter dominated phase
- Phantom scalar dark energy as modified gravity: understanding the origin of the Big Rip singularity
- Physical non-equivalence of the Jordan and Einstein frames
- An Accelerating Cosmology Without Dark Energy
- Correspondence of Gravity Singularities in Jordan and Einstein Frames
- If Gauss-Bonnet interaction plays the role of dark energy
- Bianchi type I cosmological model with a viscous fluid
- A question mark on the equivalence of Einstein and Jordan frames
- Irrotational Bianchi V Viscous Fluid Cosmology with Heat Flux
- Dark Energy as a Modification of the Friedmann Equation
- Precision Predictions for the Primordial Power Spectra from f(R) Models of Inflation
- Cosmological Scaling Solutions of Multiple Tachyon Fields with Inverse Square Potentials
- Bianchi Type-II Cosmological Model with Viscous Fluid
- Gauss-Bonnet Chameleon Mechanism of Dark Energy
- Bianchi VI0 viscous fluid cosmology with magnetic field
- Transient Crossing of Phantom divide line under Gauss-Bonnet interaction
- Dark Matter, Dark Energy and the Chaplygin Gas
- Supernova Constraints on Braneworld Dark Energy
- Why scalar-tensor equivalent theories are not physically equivalent?