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Quantum dynamics of scalar particles in the space–time of a cosmic string in the context of gravity's rainbow
(2020-10-01)
We analyze the dynamics of scalar particles in gravity's rainbow considering the space–time of a cosmic string in this modified gravity. Thus, we solve the Klein–Gordon equation for two types of potential in which two ...
Cosmic String Signatures in Anisotropies of the Cosmic Microwave Background
(Elsevier, 2002-12)
We briefly review certain aspects of cosmic microwave background anisotropies as generated in passive and active models of structure formation. We then focus on cosmic strings based models and discuss their status in the ...
Vacuum polarization by a magnetic flux in a cosmic string background.
(Elsevier B.V., 2004-02-01)
In this paper we analyse the vacuum polarization effects due to a magnetic flux on massless fermionic fields in a cosmic string background. Three distinct configurations of magnetic fields are considered. In all of them ...
Cosmic Microwave background bispectrum from Active Models of Structure Formation
(American Physical Society, 2001-12)
We propose a method for a numerical computation of the angular bispectrum of the cosmic microwave background (CMB) anisotropies arising from active models such as cosmic topological defects, using a modified Boltzmann code ...
Scalar bosons with Coulomb potentials in a cosmic string background: scattering and bound states
(2020-01-01)
The relativistic quantum motion of scalar bosons under the influence of a full vector (minimal Aμ and nonminimal Xμ) and scalar (Vs) interactions embedded in the background of a cosmic string is explored in the context of ...
Vacuum polarization by a magnetic flux in a cosmic string background.
(Elsevier B.V., 2015)
Vacuum polarization by a magnetic flux in a cosmic string background.
(Elsevier B.V., 2015)
ON THE INTERACTION OF NULL FLUIDS IN COSMOLOGY
(Elsevier Science BvAmsterdamHolanda, 1993)
Vacuum fluctuations of twisted fields in the spacetime of a cosmic string
(1990-01-01)
A twisted scalar field conformally coupled to gravitation is used to calculate the vacuum stress-energy tensor in the background spacetime generated by an infinite straight gauge cosmic string. The result found has an ...