354 research outputs found
Tensor-to-Scalar Ratio in Eddington-inspired Born-Infeld Inflation
We investigate the scalar perturbation of the inflation model driven by a
massive-scalar field in Eddington-inspired Born-Infeld gravity. We focus on the
perturbation at the attractor stage in which the first and the second slow-roll
conditions are satisfied. The scalar perturbation exhibits the corrections to
the chaotic inflation model in general relativity. We find that the
tensor-to-scalar ratio becomes smaller than that of the usual chaotic
inflation.Comment: 9 pages. revised version to appear in EPJC, with minor typo
corrections. arXiv admin note: text overlap with arXiv:1404.608
Generation of large-scale magnetic fields due to fluctuating in shearing systems
We explore the growth of large-scale magnetic fields in a shear flow, due to
helicity fluctuations with a finite correlation time, through a study of the
Kraichnan-Moffatt model of zero-mean stochastic fluctuations of the
parameter of dynamo theory. We derive a linear integro-differential equation
for the evolution of large-scale magnetic field, using the first-order
smoothing approximation and the Galilean invariance of the -statistics.
This enables construction of a model that is non-perturbative in the shearing
rate and the -correlation time . After a brief review
of the salient features of the exactly solvable white-noise limit, we consider
the case of small but non-zero . When the large-scale magnetic
field varies slowly, the evolution is governed by a partial differential
equation. We present modal solutions and conditions for the exponential growth
rate of the large-scale magnetic field, whose drivers are the Kraichnan
diffusivity, Moffatt drift, Shear and a non-zero correlation time. Of
particular interest is dynamo action when the -fluctuations are weak;
i.e. when the Kraichnan diffusivity is positive. We show that in the absence of
Moffatt drift, shear does not give rise to growing solutions. But shear and
Moffatt drift acting together can drive large scale dynamo action with growth
rate .Comment: 19 pages, 4 figures, Accepted in Journal of Plasma Physic
Quintessential Inflation in a thawing realization
We study quintessential inflation with an inverse hyperbolic type potential
, where ,
and "n" are parameters of the theory. We obtain a bound on
for different values of the parameter n. The spectral index and the
tensor-to-scalar-ratio fall in the bound given by the Planck 2015
data for for certain values of . However for
there exist values of for which the spectral index and the
tensor-to-scalar-ratio fall only within the bound of the Planck
data. Furthermore, we show that the scalar field with the given potential can
also give rise to late time acceleration if we invoke the coupling to massive
neutrino matter. We also consider the instant preheating mechanism with Yukawa
interaction and put bounds on the coupling constants for our model using the
nucleosynthesis constraint on relic gravity waves produced during inflation.Comment: 11 page
Weak Lensing Effect on CMB in the Presence of a Dipole Anisotropy
We investigate weak lensing effect on cosmic microwave background (CMB) in
the presence of dipole anisotropy. The approach of flat-sky approximation is
considered. We determine the functions and that
appear in expressions of the lensed CMB power spectrum in the presence of a
dipole anisotropy. We determine the correction to B-mode power spectrum which
is found to be appreciable at low multipoles (). However, the temperature
and E-mode power spectrum are not altered significantly.Comment: 9 page
Scale Invariance as a Solution to the Cosmological Constant Problem
We show that scale invariance provides a solution to the fine tuning problem
of the cosmological constant. We construct a generalization of the standard
model of particle physics which displays exact quantum scale invariance. The
matter action is invariant under global scale transformations in arbitrary
dimensions. However the gravitational action breaks scale invariance
explicitly. The scale symmetry is broken spontaneously in the matter sector of
the theory. We show that the contribution to the vacuum energy and hence the
cosmological constant is identically zero from the matter sector within the
full quantum theory. However the gravitational sector may give non-zero
contributions to the cosmological constant at loop orders. No fine tuning may
be required at loop orders since the matter sector gives zero contribution to
the cosmological constant. We also show that we do not require full scale
invariance in order to constrain the vacuum energy from the matter sector. We
only require invariance under pseudoscale transformations. Using this idea and
motivated by the concept of unimodular gravity we propose an alternative model.
In this case also we show that matter sector gives exactly zero contribution to
the vacuum energy.Comment: 12 pages, no figure
Scalar Perturbation Produced at the Pre-inflationary Stage in Eddington-inspired Born-Infeld Gravity
We investigate the scalar perturbation produced at the pre-inflationary stage
driven by a massive scalar field in Eddington-inspired Born-Infeld gravity. The
scalar power spectrum exhibits a peculiar rise for low -modes. The
tensor-to-scalar ratio can be significantly lowered compared with that in the
standard chaotic inflation model in general relativity. This result is very
affirmative considering the recent dispute on the detection of the
gravitational wave radiation between PLANCK and BICEP2.Comment: 12 pages, 1 figure, version to appear in EPJ
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