57 research outputs found
Effective Geometry
We introduce the concept of effective geometry by studying several systems in
which it arises naturally. As an example of the power and conciseness of the
method, it is shown that a flowing dielectric medium with a linear response to
an external electric field can be used to generate an analog geometry that has
many of the formal properties of a \Sch black hole for light rays, in spite of
birefringence. The surface gravity of this analog black hole has a contribution
that depends only on the dielectric properties of the fluid (in addition to the
usual term dependent on the acceleration). This term may be give a hint to a
new mechanism to increase the temperature of Hawking radiation.Comment: 13 pages, RevTex4, Contribution to the Proceedings of the Xth
Brazilian School of Gravitation and Cosmology, to be published by AI
Evolution of Vacuum Bubbles Embeded in Inhomogeneous Spacetimes
We study the propagation of bubbles of new vacuum in a radially inhomogeneous
background filled with dust or radiation, and including a cosmological
constant, as a first step in the analysis of the influence of inhomogeneities
in the evolution of an inflating region. We also compare the cases with dust
and radiation backgrounds and show that the evolution of the bubble in
radiation environments is notably different from that in the corresponding dust
cases, both for homogeneous and inhomogeneous ambients, leading to appreciable
differences in the evolution of the proper radius of the bubble.Comment: 18 pages, 15 figures, accepted for publication in Journal of
Cosmology and Astroparticle Physics (new version with a few cosmetic changes
w.r.t. the published one
Cosmography and the redshift drift in Palatini theories
We present an application to cosmological models in theories
within the Palatini formalism of a method that combines cosmography and the
explicit form of the field equations in the calculation of the redshift drift.
The method yields a sequence of constraint equations which lead to limits on
the parameter space of a given -model. Two particular families of
-cosmologies capable of describing the current dynamics of the
universe are explored here: (i) power law theories of the type , and (ii) theories of the form . The constraints on and
, respectively, limit the values to intervals that are narrower
than the ones previously obtained. As a byproduct, we show that when applied to
General Relativity, the method yields values of the kinematic parameters with
much smaller errors that those obtained directly from observations.Comment: 7 pages, 2 figure
Cylindrically symmetric spinning Brans-Dicke spacetimes with closed timelike curves
We present here three new solutions of Brans-Dicke theory for a stationary
geometry with cylindrical symmetry in the presence of matter in rigid rotation
with . All the solutions have eternal closed timelike curves
in some region of the spacetime, the size of which depends on .
Moreover, two of them do not go over a solution of general relativity in the
limit .Comment: revtex, 10 pages, 1 figure in p
A Born-Infeld-like f(R) gravity
Several features of an theory in which there is a maximum value for
the curvature are analyzed. The theory admits the vaccuum solutions of GR, and
also the radiation evolution for the scale factor of the standard cosmological
model. Working in the Jordan frame, a complete analysis of the phase space is
performed, and its results supported with examples obtainted by numerical
integration. In particular, we showed that theory has nonsingular cosmological
solutions which after the bounce enter a phase of de Sitter expansion and
subsequently relax to a GR-like radiation-dominated evolution.Comment: Latex file, 14 pages, 7 figures (jpg format), including more detailed
discussions than previous version, accepted for publication in Physical
Review
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