Particle creation in a f(R) theory with cosmological constraints
arXiv:1402.5004 · doi:10.1007/s10714-014-1699-x
Abstract
In this paper we study the creation of super-massive real scalar particles in the framework of a modified gravity theory, with parameters constrained by observational data. The analysis is restrict to a homogeneous and isotropic flat and radiation dominated universe. We compare the results to the standard Einstein gravity with cosmological constant ( model), and we show that the total number density of created particles in the model is very close to the standard case. Another interesting result is that the spectrum of created particles is independent at early times.
To appear in the General Relativity and Gravitation. arXiv admin note: text overlap with arXiv:1108.3346
References in corpus (9)
- Unified cosmic history in modified gravity: from F(R) theory to Lorentz non-invariant models
- Are f(R) dark energy models cosmologically viable ?
- Modified non-local-F(R) gravity as the key for the inflation and dark energy
- f(R) gravity theories in Palatini formalism: cosmological dynamics and observational constraints
- Viable Palatini-f(R) cosmologies with generalized dark matter
- Gödel-type universes in f(R) gravity
- Quantized fields and gravitational particle creation in f(R) expanding universes
- Cosmological Constraints from Hubble Parameter on f(R) Cosmologies
- Space-Time Description of Scalar Particle Creation by a Homogeneous Isotropic Gravitational Field