331 research outputs found
G\"{o}del-type universes in f(R) gravity
The gravity theories provide an alternative way to explain the current
cosmic acceleration without a dark energy matter component. If gravity is
governed by a theory a number of issues should be reexamined in this
framework, including the violation of causality problem on nonlocal scale. We
examine the question as to whether the gravity theories permit
space-times in which the causality is violated. We show that the field
equations of these gravity theories do not exclude solutions with
breakdown of causality for a physically well-motivated perfect-fluid matter
content. We demonstrate that every perfect-fluid G\"{o}del-type solution of a
generic gravity satisfying the condition is necessarily
isometric to the G\"odel geometry, and therefore presents violation of
causality. This result extends a theorem on G\"{o}del-type models, which has
been established in the context of general relativity. We also derive an
expression for the critical radius (beyond which the causality is
violated) for an arbitrary theory, making apparent that the violation of
causality depends on both the gravity theory and the matter content. As
an illustration, we concretely take a recent gravity theory that is free
from singularities of the Ricci scalar and is cosmologically viable, and show
that this theory accommodates noncausal as well as causal G\"odel-type
solutions.Comment: 7 pages, V3: Version to appear in Phys. Rev. D (2009), typos
corrected, the generality of our main results is emphasized. The illustrative
character of a particular theory is also made explici
Gravitational Rainbow
It is shown that unlike Einstein's gravity quadratic gravity produces dispersive photon propagation. The energy-dependent contribution to the deflection of photons passing by the Sun is computed and subsequently the angle at which the visible spectrum would be spread over is plotted as a function of the sector mass
Constraints on non-minimally coupled curved space electrodynamics from astrophysical observations
We study interactions of electro-magnetic fields with the curvature tensor of
the form . Such
coupling terms though are invariant under general coordinate transformation and
CPT, however violate the Einstein equivalence principle. These couplings do not
cause any energy dependent dispersion of photons but they exhibit
birefringence. We put constraints on the coupling constant using
results from solar system radar ranging experiments and millisecond-pulsar
observations. We find that the most stringent constraint comes from pulsar
observations and is given by obtained from the
timing of binary pulsar PSR B1534+12.Comment: 9 pages latex, accepted in CQ
Metric-scalar gravity with torsion and the measurability of the non-minimal coupling
The "measurability" of the non-minimal coupling is discussed by considering
the correction to the Newtonian static potential in the semi-classical
approach. The coefficient of the "gravitational Darwin term" (GDT) gets
redefined by the non-minimal torsion-scalar couplings. Based on a similar
analysis of the GDT in the effective field theory approach to non-minimal
scalar we conclude that for reasonable values of the couplings the correction
is very small.Comment: 10 pages, LaTex. Accepted for publication in Mod. Phys. Lett.
Godel-type Universes in String-inspired Charged Gravity
We consider a string-inspired, gravitational theory of scalar and
electromagnetic fields and we investigate the existence of axially-symmetric,
G\"{o}del-type cosmological solutions. The neutral case is studied first and an
"extreme" G\"{o}del-type rotating solution, that respects the causality, is
determined. The charged case is considered next and two new configurations for
the, minimally-coupled to gravity, electromagnetic field are presented. Another
configuration motivated by the expected distribution of currents and charges in
a rotating universe is studied and shown to lead to a G\"{o}del-type solution
for a space-dependent coupling function. Finally, we investigate the existence
of G\"{o}del-type cosmological solutions in the framework of the one-loop
corrected superstring effective action and we determine the sole configuration
of the electromagnetic field that leads to such a solution. It turns out that,
in all the charged cases considered, Closed Timelike Curves do appear and the
causality is always violated.Comment: 26 pages, LaTex file, a few comments and references added, version to
appear in Physical Review
Closed timelike curves and geodesics of Godel-type metrics
It is shown explicitly that when the characteristic vector field that defines
a Godel-type metric is also a Killing vector, there always exist closed
timelike or null curves in spacetimes described by such a metric. For these
geometries, the geodesic curves are also shown to be characterized by a lower
dimensional Lorentz force equation for a charged point particle in the relevant
Riemannian background. Moreover, two explicit examples are given for which
timelike and null geodesics can never be closed.Comment: REVTeX 4, 12 pages, no figures; the Introduction has been rewritten,
some minor mistakes corrected, many references adde
Identificação, espacialização e caracterização dos principais solos do municĂpio de Feliz Deserto, Alagoas.
bitstream/item/64257/1/ComTec-62-Feliz-Deserto.pd
Effective Lagrangian from Higher Curvature Terms: Absence of vDVZ Discontinuity in AdS Space
We argue that the van Dam-Veltman-Zakharov discontinuity arising in the limit of the massive graviton through an explicit Pauli-Fierz mass term
could be absent in anti de Sitter space. This is possible if the graviton can
acquire mass spontaneously from the higher curvature terms or/and the massless
limit is attained faster than the cosmological constant . We discuss the effects of higher-curvature couplings and of an explicit
cosmological term () on stability of such continuity and of massive
excitations.Comment: 23 pages, Latex, the version to appear in Class. Quant. Gra
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