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Particle creation in a f(R) theory with cosmological constraints
(Springer, 2014-04-01)
In this paper we study the creation of super-massive real scalar particles in the framework of a f (R) = R - beta/R-n modified gravity theory, with parameters constrained by observational data. The analysis is restrict to ...
Quantized fields and gravitational particle creation in f (R) expanding universes
(ELSEVIER SCIENCE BV, 2010)
The problem of cosmological particle creation for a spatially flat, homogeneous and isotropic universes is discussed in the context of f (R) theories of gravity. Different from cosmological models based on general relativity ...
Particle creation in a f(R) theory with cosmological constraints
(Springer, 2015)
Creation of mass dimension one fermionic particles in asymptotically expanding universe
(2017-10-01)
In the present work we study the process of particle creation for mass dimension one fermionic fields (sometimes named Elko) as a consequence of expansion of the universe. We study the effect driven by an expanding background ...
CCDM model from quantum particle creation: constraints on dark matter mass
(Iop Publishing Ltd, 2014-07-01)
In this work the results from the quantum process of matter creation have been used in order to constrain the mass of the dark matter particles in an accelerated Cold Dark Matter model (Creation Cold Dark Matter, CCDM). ...
Particle creation in a f(R) theory with cosmological constraints
(Springer, 2015)
CCDM model from quantum particle creation: constraints on dark matter mass
(Iop Publishing Ltd, 2015)
Particle creation due to tachyonic instability in relativistic stars
(2012-11-07)
Dense enough compact objects were recently shown to lead to an exponentially fast increase of the vacuum energy density for some free scalar fields properly coupled to the spacetime curvature as a consequence of a ...
Particle creation due to tachyonic instability in relativistic stars
(Amer Physical Soc, 2012-11-07)
Dense enough compact objects were recently shown to lead to an exponentially fast increase of the vacuum energy density for some free scalar fields properly coupled to the spacetime curvature as a consequence of a ...