Particle creation in flat FRW Universe in the framework of gravity
arXiv:1111.2821 · doi:10.1139/cjp-2012-0427
Abstract
We study particle production aspect in the flat FRW universe in the framework of gravity. The matter is minimally coupled with the gravity and an exact power-law solution is obtained by solving the Friedmann equations, and matter is assumed to be minimally coupled with gravitation. The torsion scalar appears to plays the same role as the the curvature (Ricci scalar) in the the General Relativity (GR) and its modified theories . Specially in phantom phase, we observe that the vacuum state corresponds to a vanishing torsion scalar and particle production becomes important as the torsion scalar diverges. This aspect, not only provides the equivalence between the teleparallel gravity and the GR, but also between their respective modified versions, f(T) and f(R), in the view of massless particle production phenomenon when the matter is minimally coupled with the gravity. However, when the gravitational and scalar fields are not minimally coupled, it appears that this similarity between the teleparallel and GR may break down, due to the fact that the torsion scalar has no longer the same time dependent expression as the Ricci scalar.
16 pages, 1 figure. Accepted for publication in Canadian Journal of Physics (CJP)
References in corpus (15)
- Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
- Dynamics of dark energy
- Dark torsion as the cosmic speed-up
- Modified teleparallel gravity: inflation without inflaton
- Einstein's Other Gravity and the Acceleration of the Universe
- On Born-Infeld Gravity in Weitzenbock spacetime
- Static Anisotropic Solutions in f(T) Theory
- New Static Solutions in f(T) Theory
- Stability of a non-minimally conformally coupled scalar field in F(T) cosmology
- Anisotropic fluid for a set of non-diagonal tetrads in f(T) gravity
- Power-law solutions in gravity
- Sudden singularities survive massive quantum particle production
- Reconstruction of f(T) gravity according to holographic dark energy
- Modified gravity as realistic candidate for dark energy, inflation and dark matter
- Effects of Quantized Scalar Fields in Cosmological Spacetimes with Big Rip Singularities