1,142 research outputs found
The matter Lagrangian and the energy-momentum tensor in modified gravity with non-minimal coupling between matter and geometry
We show that in modified type gravity models with non-minimal coupling
between matter and geometry, both the matter Lagrangian, and the
energy-momentum tensor, are completely and uniquely determined by the form of
the coupling. This result is obtained by using the variational formulation for
the derivation of the equations of motion in the modified gravity models with
geometry-matter coupling, and the Newtonian limit for a fluid obeying a
barotropic equation of state. The corresponding energy-momentum tensor of the
matter in modified gravity models with non-minimal coupling is more general
than the usual general-relativistic energy-momentum tensor for perfect fluids,
and it contains a supplementary, equation of state dependent term, which could
be related to the elastic stresses in the body, or to other forms of internal
energy. Therefore, the extra-force induced by the coupling between matter and
geometry never vanishes as a consequence of the thermodynamic properties of the
system, or for a specific choice of the matter Lagrangian, and it is non-zero
in the case of a fluid of dust particles.Comment: 6 pages, accepted for publication in PRD; references adde
Cosmic strings in gravity
We consider Kasner-type static, cylindrically symmetric interior string
solutions in the theory of modified gravity. The physical
properties of the string are described by an anisotropic energy-momentum tensor
satisfying the condition ; that is, the energy density of the
string along the -axis is equal to minus the string tension. As a first step
in our study we obtain the gravitational field equations in the
theory for a general static, cylindrically symmetric
metric, and then for a Kasner-type metric, in which the metric tensor
components have a power law dependence on the radial coordinate . String
solutions in two particular modified gravity models are investigated in detail.
The first is the so-called "exponential" modified gravity, in which the
gravitational action is proportional to the exponential of the sum of the Ricci
scalar and matter Lagrangian, and the second is the "self-consistent model",
obtained by explicitly determining the gravitational action from the field
equations under the assumption of a power law dependent matter Lagrangian. In
each case, the thermodynamic parameters of the string, as well as the precise
form of the matter Lagrangian, are explicitly obtained.Comment: 20 pages, no figures. Published versio
New derivation of the Lagrangian of a perfect fluid with a barotropic equation of state
In this paper we give a simple proof that when the particle number is
conserved, the Lagrangian of a barotropic perfect fluid is , where is the \textit{rest mass}
density and is the pressure. To prove this result nor additional
fields neither Lagrange multipliers are needed. Besides, the result is
applicable to a wide range of theories of gravitation. The only assumptions
used in the derivation are: 1) the matter part of the Lagrangian does not
depend on the derivatives of the metric, and 2) the particle number of the
fluid is conserved ()
Cosmological evolution of finite temperature Bose-Einstein Condensate dark matter
Once the temperature of a bosonic gas is smaller than the critical, density
dependent, transition temperature, a Bose - Einstein Condensation process can
take place during the cosmological evolution of the Universe. Bose - Einstein
Condensates are very strong candidates for dark matter, since they can solve
some major issues in observational astrophysics, like, for example, the
galactic core/cusp problem. The presence of the dark matter condensates also
drastically affects the cosmic history of the Universe. In the present paper we
analyze the effects of the finite dark matter temperature on the cosmological
evolution of the Bose-Einstein Condensate dark matter systems. We formulate the
basic equations describing the finite temperature condensate, representing a
generalized Gross-Pitaevskii equation that takes into account the presence of
the thermal cloud in thermodynamic equilibrium with the condensate. The
temperature dependent equations of state of the thermal cloud and of the
condensate are explicitly obtained in an analytical form. By assuming a flat
Friedmann-Robertson-Walker (FRW) geometry, the cosmological evolution of the
finite temperature dark matter filled Universe is considered in detail in the
framework of a two interacting fluid dark matter model, describing the
transition from the initial thermal cloud to the low temperature condensate
state. The dynamics of the cosmological parameters during the finite
temperature dominated phase of the dark matter evolution are investigated in
detail, and it is shown that the presence of the thermal excitations leads to
an overall increase in the expansion rate of the Universe.Comment: 14 pages, 11 figures, accepted for publication in PR
Dynamical behavior and Jacobi stability analysis of wound strings
We numerically solve the equations of motion (EOM) for two models of circular
cosmic string loops with windings in a simply connected internal space. Since
the windings cannot be topologically stabilized, stability must be achieved (if
at all) dynamically. As toy models for realistic compactifications, we consider
windings on a small section of , which is valid as an
approximation to any simply connected internal manifold if the winding radius
is sufficiently small, and windings on an of constant radius
. We then use Kosambi-Cartan-Chern (KCC) theory to analyze the
Jacobi stability of the string equations and determine bounds on the physical
parameters that ensure dynamical stability of the windings. We find that, for
the same initial conditions, the curvature and topology of the internal space
have nontrivial effects on the microscopic behavior of the string in the higher
dimensions, but that the macroscopic behavior is remarkably insensitive to the
details of the motion in the compact space. This suggests that
higher-dimensional signatures may be extremely difficult to detect in the
effective -dimensional dynamics of strings compactified on an internal
space, even if configurations with nontrivial windings persist over long time
periods.Comment: 46 pages, 26 figures, accepted for publication in EPJC; matches the
published version. Updated references (v3
On Einstein clusters as galactic dark matter halos
We consider global and gravitational lensing properties of the recently
suggested Einstein clusters of WIMPs as galactic dark matter halos. Being
tangential pressure dominated, Einstein clusters are strongly anisotropic
systems which can describe any galactic rotation curve by specifying the
anisotropy. Due to this property, Einstein clusters may be considered as dark
matter candidates. We analyse the stability of the Einstein clusters against
both radial and non-radial pulsations, and we show that the Einstein clusters
are dynamically stable. With the use of the Buchdahl type inequalities for
anisotropic bodies, we derive upper limits on the velocity of the particles
defining the cluster. These limits are consistent with those obtained from
stability considerations. The study of light deflection shows that the
gravitational lensing effect is slightly smaller for the Einstein clusters, as
compared to the singular isothermal density sphere model for dark matter.
Therefore lensing observations may discriminate, at least in principle, between
Einstein cluster and other dark matter models.Comment: MNRAS LaTeX, 7 pages, accepted by MNRAS; reference adde
Constraints on extra-dimensions and variable constants from cosmological gamma ray bursts
The observation of the time delay between the soft emission and the
high-energy radiation from cosmological gamma ray bursts can be used as an
important observational test of multi-dimensional physical theories. The main
source of the time delay is the variation of the electromagnetic coupling, due
to dimensional reduction, which induces an energy dependence of the speed of
light. For photons with energies around 1 TeV, the time delay could range from
a few seconds in the case of Kaluza-Klein models to a few days for models with
large extra-dimensions. Based on these results we suggest that the detection of
the 18-GeV photon 4500 s after the keV/MeV burst in GRB 940217 provides
a strong evidence for the existence of extra-dimensions. The time delay of
photons, if observed by the next generation of high energy detectors, like, for
example, the SWIFT and GLAST satellite based detectors, or the VERITAS
ground-based TeV gamma-ray instrument, could differentiate between the
different models with extra-dimensions.Comment: 8 pages, 4 figures, contribution to the proceedings of the II
Workshop on Unidentified Gamma-Ray Sources, Hong Kong, June 1-4, 200
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