92 research outputs found
Notes on the Two-brane Model with Variable Tension
Motivated by possible extensions of the braneworld models with two branes, we
investigate some consequences of a variable brane tension using the well
established results on consistency conditions. By a slight modification of the
usual stress-tensor used in order to derive the braneworld sum rules, we find
out some important constraints obeyed by time dependent brane tensions. In
particular it is shown that the tensions of two Randall-Sundrum like branes
obeying, at the same time, an Eotvos law, aggravate the fine tuning problem.
Also, it is shown that if the hidden brane tension obeys an Eotvos law, then
the visible brane has a mixed behavior allowing a bouncing-like period at early
times while it is dominated by an Eotvos law nowadays. To finalize, we discuss
some qualitative characteristics which may arise in the scope of dynamical
brane tensions, as anisotropic background and branons production.Comment: 7 pages, 1 figure, accepted for publication in Physical Review
Two-branes with variable tension model and the effective Newtonian constant
It is shown that, in the two brane time variation model framework, if the
hidden brane tension varies according to the phenomenological Eotvos law, the
visible brane tension behavior is such that its time derivative is negative in
the past and positive after a specific time of cosmological evolution. This
behavior is interpreted in terms of an useful mechanical system analog and its
relation with the variation of the Newtonian (effective) gravitational
`constant' is explored.Comment: 15 pages, no figure, accepted for publication in Physical Review
Friedmann branes with variable tension
We introduce brane-worlds with non-constant tension, strenghtening the
analogy with fluid membranes, which exhibit a temperature-dependence according
to the empirical law established by E\"otv\"os. This new degree of freedom
allows for evolving gravitational and cosmological constants, the latter being
a natural candidate for dark energy. We establish the covariant dynamics on a
brane with variable tension in full generality, by considering asymmetrically
embedded branes and allowing for non-standard model fields in the 5-dimensional
space-time. Then we apply the formalism for a perfect fluid on a Friedmann
brane, which is embedded in a 5-dimensional charged Vaidya-Anti de Sitter
space-time.Comment: 12 pages, to appear in Phys. Rev.
Strong quantum violation of the gravitational weak equivalence principle by a non-Gaussian wave-packet
The weak equivalence principle of gravity is examined at the quantum level in
two ways. First, the position detection probabilities of particles described by
a non-Gaussian wave-packet projected upwards against gravity around the
classical turning point and also around the point of initial projection are
calculated. These probabilities exhibit mass-dependence at both these points,
thereby reflecting the quantum violation of the weak equivalence principle.
Secondly, the mean arrival time of freely falling particles is calculated using
the quantum probability current, which also turns out to be mass dependent.
Such a mass-dependence is shown to be enhanced by increasing the
non-Gaussianity parameter of the wave packet, thus signifying a stronger
violation of the weak equivalence principle through a greater departure from
Gaussianity of the initial wave packet. The mass-dependence of both the
position detection probabilities and the mean arrival time vanish in the limit
of large mass. Thus, compatibility between the weak equivalence principle and
quantum mechanics is recovered in the macroscopic limit of the latter. A
selection of Bohm trajectories is exhibited to illustrate these features in the
free fall case.Comment: 11 pages, 7 figure
Black string corrections in variable tension braneworld scenarios
Braneworld models with variable tension are investigated, and the corrections
on the black string horizon along the extra dimension are provided. Such
corrections are encrypted in additional terms involving the covariant
derivatives of the variable tension on the brane, providing profound
consequences concerning the black string horizon variation along the extra
dimension, near the brane. The black string horizon behavior is shown to be
drastically modified by the terms corrected by the brane variable tension. In
particular, a model motivated by the phenomenological interesting case
regarding Eotvos branes is investigated. It forthwith provides further physical
features regarding variable tension braneworld scenarios, heretofore concealed
in all previous analysis in the literature. All precedent analysis considered
uniquely the expansion of the metric up to the second order along the extra
dimension, what is able to evince solely the brane variable tension absolute
value. Notwithstanding, the expansion terms aftermath, further accomplished in
this paper from the third order on, elicits the successive covariant
derivatives of the brane variable tension, and their respective coupling with
the extrinsic curvature, the Weyl tensor, and the Riemann and Ricci tensors, as
well as the scalar curvature. Such additional terms are shown to provide sudden
modifications in the black string horizon in a variable tension braneworld
scenarioComment: 12 pages, 5 figures, accepted in PR
Testing the Principle of Equivalence by Solar Neutrinos
We discuss the possibility of testing the principle of equivalence with solar
neutrinos. If there exists a violation of the equivalence principle quarks and
leptons with different flavors may not universally couple with gravity. The
method we discuss employs a quantum mechanical phenomenon of neutrino
oscillation to probe into the non-universality of the gravitational couplings
of neutrinos. We develop an appropriate formalism to deal with neutrino
propagation under the weak gravitational fields of the sun in the presence of
the flavor mixing. We point out that solar neutrino observation by the next
generation water Cherenkov detectors can improve the existing bound on
violation of the equivalence principle by 3-4 orders of magnitude if the
nonadiabatic Mikheyev-Smirnov-Wolfenstein mechanism is the solution to the
solar neutrino problem.Comment: Latex, 17 pages + 6 uuencoded postscript figures, KEK-TH-396,
TMUP-HEL-9402 (unnecessary one reference was removed
A Neutron Interferometric Method to Provide Improved Constraints on Non-Newtonian Gravity at the Nanometer Scale
In recent years, an energetic experimental program has set quite stringent
limits on a possible "non - 1/r^2" dependence on gravity at short length
scales. This effort has been largely driven by the predictions of theories
based on compactification of extra spatial dimensions. It is characteristic of
many such theories that the strength and length scales of such anomalous
gravity are not clearly determined from first principles. As a result, it is
productive to extend the current limits the range and strength of such
hypothetical interactions. As a heavy, neutral, and (almost) stable particle,
the neutron provides an ideal probe for the study of such hypothetical
interactions at very short range. In this work, we describe methods based on
neutron interferometry which have the capability to provide improved
sensitivity non-Newtonian forces down to length scales at and below an
nanometer.Comment: PDF-fil
Back reaction of a long range force on a Friedmann-Robertson-Walker background
It is possible that there may exist long-range forces in addition to gravity.
In this paper we construct a simple model for such a force based on exchange of
a massless scalar field and analyze its effect on the evolution of a
homogeneous Friedmann-Robertson-Walker cosmology. The presence of such an
interaction leads to an equation of state characterized by positive pressure
and to resonant particle production similar to that observed in preheating
scenarios.Comment: 14 pages, 6 color Postscript figures, LaTe
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