73 research outputs found
More on Tachyon Cosmology in De Sitter Gravity
We aim to study rolling tachyon cosmological solutions in de Sitter gravity.
The solutions are taken to be flat FRW type and these are not time-reversal
symmetric. We find that cosmological constant of our universe has to be
fine-tuned at the level of the action itself, as in KKLT string
compactification. The rolling tachyon can give rise to required inflation with
suitable choice of the initial conditions which include nonvanishing Hubble
constant. We also determine an upper bound on the volume of the
compactification manifold.Comment: 15pp, 3 figures; references adde
Relic Gravitational Waves and Their Detection
The range of expected amplitudes and spectral slopes of relic (squeezed)
gravitational waves, predicted by theory and partially supported by
observations, is within the reach of sensitive gravity-wave detectors. In the
most favorable case, the detection of relic gravitational waves can be achieved
by the cross-correlation of outputs of the initial laser interferometers in
LIGO, VIRGO, GEO600. In the more realistic case, the sensitivity of advanced
ground-based and space-based laser interferometers will be needed. The specific
statistical signature of relic gravitational waves, associated with the
phenomenon of squeezing, is a potential reserve for further improvement of the
signal to noise ratio.Comment: 25 pages, 9 figures included, revtex. Based on a talk given at
"Gyros, Clocks, and Interferometers: Testing General Relativity in Space"
(Germany, August 99
Monopole Inflation in Brans-Dicke Theory
According to previous work, topological defects expand exponentially without
an end if the vacuum expectation value of the Higgs field is of the order of
the Planck mass. We extend the study of inflating topological defects to the
Brans-Dicke gravity. With the help of numerical simulation we investigate the
dynamics and spacetime structure of a global monopole. Contrary to the case of
the Einstein gravity, any inflating monopole eventually shrinks and takes a
stable configuration. We also discuss cosmological constraints on the model
parameters.Comment: 17 pages, revtex, including figures, discussions in more general
theories are added, to appear in Phys. Rev.
A Supersymmetric SO(10) Model with Inflation and Cosmic Strings
We have built a supersymmetric SO(10) model consistent with cosmological
observations. The model gives rise to a false vacuum hybrid inflationary
scenario which solves the monopole problem. We argue that this type of
inflationary scenario is generic in supersymmetric SO(10) model, and arises
naturally from the theory. Neither any external field nor any external symmetry
has to be added. It can just be a consequence of the theory. In our specific
model, at the end of inflation, cosmic strings form. The properties of the
strings are presented. The cosmic background radiation anisotropies induced by
the inflationary perturbations and the cosmic strings are estimated. The model
produces a stable lightest superparticle and a very light left-handed neutrino
which may serve as the cold and hot dark matter. The properties of a mixed
cosmic string-inflationary large scale structure formation scenario are
discussed.Comment: 32 pages, uses RevTex. Misprint in a referenc
Gravitational Lensing and f(R) theories in the Palatini approach
We investigate gravitational lensing in the Palatini approach to the f(R)
extended theories of gravity. Starting from an exact solution of the f(R) field
equations, which corresponds to the Schwarzschild-de Sitter metric and, on the
basis of recent studies on this metric, we focus on some lensing observables,
in order to evaluate the effects of the non linearity of the gravity
Lagrangian. We give estimates for some astrophysical events, and show that
these effects are tiny for galactic lenses, but become interesting for
extragalactic ones.Comment: 7 Pages, RevTex, 1 eps figure; references added; revised to match the
version accepted for publication in General Relativity and Gravitatio
Fabry-Perot interference and spin filtering in carbon nanotubes
We study the two-terminal transport properties of a metallic single-walled
carbon nanotube with good contacts to electrodes, which have recently been
shown [W. Liang et al, Nature 441, 665-669 (2001)] to conduct ballistically
with weak backscattering occurring mainly at the two contacts. The measured
conductance, as a function of bias and gate voltages, shows an oscillating
pattern of quantum interference. We show how such patterns can be understood
and calculated, taking into account Luttinger liquid effects resulting from
strong Coulomb interactions in the nanotube. We treat back-scattering in the
contacts perturbatively and use the Keldysh formalism to treat non-equilibrium
effects due to the non-zero bias voltage. Going beyond current experiments, we
include the effects of possible ferromagnetic polarization of the leads to
describe spin transport in carbon nanotubes. We thereby describe both
incoherent spin injection and coherent resonant spin transport between the two
leads. Spin currents can be produced in both ways, but only the latter allow
this spin current to be controlled using an external gate. In all cases, the
spin currents, charge currents, and magnetization of the nanotube exhibit
components varying quasiperiodically with bias voltage, approximately as a
superposition of periodic interference oscillations of spin- and
charge-carrying ``quasiparticles'' in the nanotube, each with its own period.
The amplitude of the higher-period signal is largest in single-mode quantum
wires, and is somewhat suppressed in metallic nanotubes due to their sub-band
degeneracy.Comment: 12 pages, 6 figure
Constraints on diffuse neutrino background from primordial black holes
We calculated the energy spectra and the fluxes of electron neutrino emitted
in the process of evaporation of primordial black holes (PBHs) in the early
universe. It was assumed that PBHs are formed by a blue power-law spectrum of
primordial density fluctuations. We obtained the bounds on the spectral index
of density fluctuations assuming validity of the standard picture of
gravitational collapse and using the available data of several experiments with
atmospheric and solar neutrinos. The comparison of our results with the
previous constraints (which had been obtained using diffuse photon background
data) shows that such bounds are quite sensitive to an assumed form of the
initial PBH mass function.Comment: 18 pages,(with 7 figures
Geometric and thermodynamic properties in Gauss-Bonnet gravity
In this paper, the generalized second law (GSL) of thermodynamics and entropy
is revisited in the context of cosmological models in Gauss-Bonnet gravity with
the boundary of the universe is assumed to be enclosed by the dynamical
apparent horizon. The model is best fitted with the observational data for
distance modulus. The best fitted geometric and thermodynamic parameters such
as equation of state parameter, deceleration parameter and entropy are derived.
To link between thermodynamic and geometric parameters, the "entropy rate of
change multiplied by the temperature" as a model independent thermodynamic
state parameter is also derived. The results show that the model is in good
agreement with the observational analysis.Comment: 13 pages, 13 figures, to be published in Astrophysics and Space Sc
Interacting entropy-corrected new agegraphic tachyon, K-essence and dilaton scalar field models of dark energy in non-flat universe
We present the new agegraphic dark energy model by introducing the quantum
corrections to the entropy-area relation in the setup of loop quantum gravity.
Employing this new form of dark energy, we investigate the model of interacting
dark energy and derive its equation of state. We study the correspondence
between the tachyon, K-essence and dilaton scalar field models with the
interacting entropy-corrected new agegraphic dark energy model in the non-flat
FRW universe. Moreover, we reconstruct the corresponding scalar potentials
which describe the dynamics of the scalar field models.Comment: 11 pages, typos fixe
Kaluza-Klein Type Robertson Walker Cosmological Model With Dynamical Cosmological Term
In this paper we have analyzed the Kaluza-Klein type Robertson Walker (RW)
cosmological models by considering three different forms of variable :
, and
. It is found that, the connecting free parameters of the
models with cosmic matter and vacuum energy density parameters are equivalent,
in the context of higher dimensional space time. The expression for the look
back time, luminosity distance and angular diameter distance are also derived.
This work has thus generalized to higher dimensions the well-known results in
four dimensional space time. It is found that there may be significant
difference in principle at least, from the analogous situation in four
dimensional space time.Comment: 16 pages, no figur
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