45,784 research outputs found
Primordial magnetic fields from metric perturbations
We study the amplification of electromagnetic vacuum fluctuations induced by
the evolution of scalar metric perturbations at the end of inflation. Such
perturbations break the conformal invariance of Maxwell equations in
Friedmann-Robertson-Walker backgrounds and allow the growth of magnetic fields
on super-Hubble scales. We relate the strength of the fields generated by this
mechanism with the power spectrum of scalar perturbations and estimate the
amplification on galactic scales for different values of the spectral index.
Finally we discuss the possible effects of finite conductivity during
reheating.Comment: 10 pages, 1 figure. Final version to appear in Phys. Rev.
Gravitino production during preheating
We study the production of gravitinos during the preheating era after
inflation by means of the non-perturbative Bogolyubov technique. Considering
only the helicity states, the problem is reduced to the simpler Dirac
fermions case. We calculate the production in a particular supergravity model
in an expanding universe and obtain the spectrum and number density. Finally we
compare the results with the nucleosynthesis bounds and extract some
consequences.Comment: 10 pages, LaTeX, 2 figures. Talk given in the International Workshop
on Particles in Astrophysics and Cosmology, Valencia (Spain), May 3-8, 199
Dark energy rest frame and the CMB dipole
If dark energy can be described as a perfect fluid, then, apart from its
equation of state relating energy density and pressure, we should also especify
the corresponding rest frame. Since dark energy is typically decoupled from the
rest of components of the universe, in principle such a frame could be
different from that of matter and radiation. In this work we consider the
potential observable effects of the motion of dark energy and the possibility
to measure the dark energy velocity relative to matter. In particular we
consider the modification of the usual interpretation of the CMB dipole and its
implications for the determination of matter bulk flows on very large scales.
We also comment on the possible origin of a dark energy flow and its evolution
in different models.Comment: 7 pages, 2 figures. Contribution to the Proceedings of the
International Workshop The Dark Side of the Universe, Madrid, June 20-24,
200
Primordial torsion fields as an explanation of the anisotropy in cosmological electromagnetic propagation
In this note we provide a simple explanation of the recent finding of
anisotropy in electromagnetic (EM) propagation claimed by Nodland and Ralston
(astro-ph/9704196). We consider, as a possible origin of such effect, the
effective coupling between EM fields and some tiny background torsion field.
The coupling is obtained after integrating out charged fermions, it is gauge
invariant and does not require the introduction of any new physics.Comment: 8 pages, LaTeX, one figure, enlarged version with minor correction
On the tension between growth rate and CMB data
We analyze the claimed tension between redshift space distorsions
measurements of and the predictions of standard CDM
(Planck 2015 and 2018) cosmology. We consider a dataset consisting of 17 data
points extending up to redshift and corrected for the Alcock-Paczynski
effect. Thus, calculating the evolution of the growth factor in a CDM
cosmology, we find that the tension for the best fit parameters ,
and with respect to the Planck 2018 CDM parameters is below
in all the marginalized confidence regions.Comment: 6 pages, 4 figures. Final version to appear in Eur. Phys. J.
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