1,091 research outputs found
Dynamical classicalization
We integrate numerically the nonlinear equation of motion for a collapsing
spherical wavepacket in the context of theories that are expected to display
behavior characteristic of classicalization. The classicalization radius sets
the scale for the onset of significant deformations of the collapsing
configuration, which result in the formation of shock fronts. A characteristic
observable feature of the classicalization process is the creation of an
outgoing field configuration that extends far beyond the classicalization
radius. This feature develops before the deformed wavepacket reaches distances
of the order of the fundamental scale. We find that in some models the
scattering problem may not have real solutions over the whole space at late
times. We determine the origin of this behavior and discuss the consistency of
the underlying models.Comment: 16 pages, 6 figures, published versio
On the dynamics of classicalization
We discuss the mechanism through which classicalization may occur during the
collapse of a spherical field configuration modelled as a wavepacket. We
demonstrate that the phenomenon is associated with the dynamical change of the
equation of motion from a second-order partial differential equation of
hyperbolic to one of elliptic type. Within this approach, we rederive the known
expression for the classicalization radius. We also find indications that
classicalization is associated with the absence of wave propagation at
distances below the classicalization radius and the generation of shock fronts.
The full quantitative picture can be obtained only through the numerical
integration of a partial differential equation of mixed type.Comment: enhanced version, 6 pages, 2 figure
Black Hole Entropy and Gravity Cutoff
We study the black hole entropy as entanglement entropy and propose a
resolution to the species puzzle. This resolution comes out naturally due to
the fact that in the presence of species the universal gravitational cutoff
is , as opposed to . We
demonstrate consistency of our solution by showing the equality of the two
entropies in explicit examples in which the relation between
and is known from the fundamental theory.Comment: 11 pages, no figure
Consistency of Relevant Cosmological Deformations on all Scales
Using cosmological perturbation theory we show that the most relevant defor-
mation of gravity is consistent at the linear level. In particular, we prove
the absence of uni- tarity violating negative norm states in the weak coupling
regime from sub- to super-Hubble scales. This demonstrates that the recently
proposed classical self-protection mechanism of deformed gravity extends to the
entire kinematical domain.Comment: 22 pages, 4 figure
Infinitely Large New Dimensions
We construct intersecting brane configurations in Anti-de-Sitter space
localizing gravity to the intersection region, with any number of extra
dimensions. This allows us to construct two kinds of theories with infinitely
large new dimensions, TeV scale quantum gravity and sub-millimeter deviations
from Newton's Law. The effective 4D Planck scale is determined in
terms of the fundamental Planck scale and the radius of curvature
via the familiar relation ; acts as an
effective radius of compactification for gravity on the intersection. Taking
TeV and sub-mm reproduces the phenomenology of theories
with large extra dimensions. Alternately, taking ,
and placing our 3-brane a distance away from the
intersection gives us a theory with an exponential determination of the
Weak/Planck hierarchy.Comment: 4 pages, revtex, no figure
Braneworld Flattening by a Cosmological Constant
We present a model with an infinite volume bulk in which a braneworld with a
cosmological constant evolves to a static, 4-dimensional Minkowski spacetime.
This evolution occurs for a generic class of initial conditions with positive
energy densities. The metric everywhere outside the brane is that of a
5-dimensional Minkowski spacetime, where the effect of the brane is the
creation of a frame with a varying speed of light. This fact is encoded in the
structure of the 4-dimensional graviton propagator on the braneworld, which may
lead to some interesting Lorentz symmetry violating effects. In our framework
the cosmological constant problem takes a different meaning since the flatness
of the Universe is guaranteed for an arbitrary negative cosmological constant.
Instead constraints on the model come from different concerns which we discuss
in detail.Comment: 18 pages, 3 figures RevTe
Regularization of Brane Induced Gravity
We study the regularization of theories of ``brane induced'' gravity in
codimension . The brane can be interpreted as a thin dielectric with a
large dielectric constant, embedded in a higher dimensional space. The kinetic
term for the higher dimensional graviton is enhanced over the brane. A four
dimensional gravitation is found on the brane at distances smaller than a
critical distance , and is due to the exchange of a massive resonant
graviton. The crossover scale is determined by the mass of the resonance.
The suppression of the couplings of light Kaluza-Klein modes to brane matter
results in a higher dimensional force law at large distances. We show that the
resulting theory is free of ghosts or tachyons.Comment: One reference added. To appear in PRD. 20 pages, 3 figure
On Sub-Millimeter Forces From Extra Dimensions
We show that in theories with large extra dimensions forces mediated by a
bulk dilaton and bulk gauge fields may be parametrically (exponentially) weaker
than gravity due to the suppression of their wave-functions on a brane. This is
the case when dilaton gets stabilized by certain strongly coupled dynamics on
the brane, or the bulk gauge symmetries are spontaneously broken by the Higgs
mechanism on the worldvolume. At distances smaller than the size of a largest
extra dimension these particles produce the force-law which decreases with
distance faster than high-dimensional gravity. For a millimeter size extra
dimensions predicted deviations are in the range which may be detected in
sub-millimeter gravity measurements.Comment: 11 page
New Dimensions at a Millimeter to a Fermi and Superstrings at a TeV
Recently, a new framework for solving the hierarchy problem has been proposed
which does not rely on low energy supersymmetry or technicolor. The
gravitational and gauge interactions unite at the electroweak scale, and the
observed weakness of gravity at long distances is due the existence of large
new spatial dimensions. In this letter, we show that this framework can be
embedded in string theory. These models have a perturbative description in the
context of type I string theory. The gravitational sector consists of closed
strings propagating in the higher-dimensional bulk, while ordinary matter
consists of open strings living on D3-branes. This scenario raises the exciting
possibility that the LHC and NLC will experimentally study both ordinary
aspects of string physics such as the production of narrow Regge-excitations of
all standard model particles, as well more exotic phenomena involving strong
gravity such as the production of black holes. The new dimensions can be probed
by events with large missing energy carried off by gravitons escaping into the
bulk. We finally discuss some important issues of model building, such as
proton stability, gauge coupling unification and supersymmetry breaking.Comment: 12 pages, late
On the long-range gravity in warped backgrounds
In this paper the Randall-Sundrum model with brane-localized curvature terms
is considered. Within some range of parameters a compact extra dimension in
this model can be astronomically large. In this case the model predicts small
deviation from Newton's law at astronomical scales, caused by the massive
modes. The existence of this deviation can result in a slight affection on the
planetary motion trajectories.Comment: LaTeX, 9 pages, typos corrected, reference adde
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