12,827 research outputs found
Boundary terms for eleven-dimensional supergravity and M-theory
A new action for eleven dimensional supergravity on a manifold with boundary
is presented. The action is a possible low energy limit of -theory. Previous
problems with infinite constants in the action are overcome and a new set of
boundary conditions relating the behaviour of the supergravity fields to matter
fields are obtained. One effect of these boundary conditions is that matter
fields generate gravitational torsion.Comment: 4 pages;with reference
Inflating Intersecting Branes and Remarks on the Hierarchy Problem
We generalize solutions of Einstein's equations for intersecting branes in
higher dimensional spacetimes to the nonstatic case, modeling an expanding
universe. The relation between the Hubble rate, the brane tensions, and the
bulk cosmological constant is similar to the case of a single 3-brane in a
5-dimensional spacetime. However, because the bulk inflates as well as the
branes, this class of solutions suffers from Newton's constant tending toward
zero on the TeV brane, where the Randall-Sundrum mechanism should solve the
weak scale hierarchy problem. The strength of gravity remains constant on the
Planck brane, however.Comment: 10 pages, LaTeX. v2:Misprint in eq. (23) corrected; citations fixed
and clarified relationship of our work to hep-th/9909053 and hep-th/9909076
v3: final version to appear in PLB. Corrected discussion of the time
dependance of the 4-D Planck mass on the TeV brane. Some references added to
earlier works on warped Kaluza-Klein compactification
One loop effective potential in heterotic M-theory
We have calculated the one loop effective potential of the vector multiplets
arising from the compactification to five dimensions of heterotic M-theory on a
Calabi-Yau manifold with h^{1,1}>1. We find that extensive cancellations
between the fermionic and bosonic sectors of the theory cause the effective
potential to vanish, with the exception of a higher order curvature term of the
type which might arise from string corrections.Comment: Latex, 28 pages, 1 figur
Balancing the vacuum energy in heterotic -theory
Moduli stabilisation is explored in the context of low-energy heterotic
-theory to show that a small value of the cosmological constant can result
from a balance between the negative potential energy left over from stabilising
the moduli and a positive Casimir energy from the higher dimensions.
Supersymmetry breaking is induced by the fermion boundary conditions on the two
branes in the theory. An explicit calculation of the Casimir energy for the
gravitino reveals that the energy has the correct sign, although the size of
the contribution is close to the edge of the parameter range for which the
calculation is valid.Comment: 15 pages, 4figures, ReVTeX, v3 stresses some point
Entropy considerations in constraining the mSUGRA parameter space
We explore the use of two criteria to constraint the allowed parameter space
in mSUGRA models. Both criteria are based in the calculation of the present
density of neutralinos as dark matter in the Universe. The first one is the
usual ``abundance'' criterion which is used to calculate the relic density
after the ``freeze-out'' era. To compute the relic density we used the
numerical public code micrOMEGAs. The second criterion applies the
microcanonical definition of entropy to a weakly interacting and
self-gravitating gas evaluating then the change in the entropy per particle of
this gas between the ``freeze-out'' era and present day virialized structures.
An ``entropy-consistency'' criterion emerges by comparing theoretical and
empirical estimates of this entropy. The main objective of our work is to
determine for which regions of the parameter space in the mSUGRA model are both
criteria consistent with the 2 bounds according to WMAP for the relic
density: . As a first result, we found that for
, sgn, small values of tan are not favored; only for
tan are both criteria significantly consistent.Comment: 5 pages, 1 figure. To appear in the Proceedings of X Mexican Workshop
on Particles and Fields, Morelia Michoac\'an, M\'exico, November 7-12, 200
Optimal Planar Electric Dipole Antenna
Considerable time is often spent optimizing antennas to meet specific design
metrics. Rarely, however, are the resulting antenna designs compared to
rigorous physical bounds on those metrics. Here we study the performance of
optimized planar meander line antennas with respect to such bounds. Results
show that these simple structures meet the lower bound on radiation Q-factor
(maximizing single resonance fractional bandwidth), but are far from reaching
the associated physical bounds on efficiency. The relative performance of other
canonical antenna designs is compared in similar ways, and the quantitative
results are connected to intuitions from small antenna design, physical bounds,
and matching network design.Comment: 10 pages, 15 figures, 2 tables, 4 boxe
Dynamics of a trapped Brownian particle in shear flows
The Brownian motion of a particle in a harmonic potential, which is
simultaneously exposed either to a linear shear flow or to a plane Poiseuille
flow is investigated. In the shear plane of both flows the probability
distribution of the particle becomes anisotropic and the dynamics is changed in
a characteristic manner compared to a trapped particle in a quiescent fluid.
The particle distribution takes either an elliptical or a parachute shape or a
superposition of both depending on the mean particle position in the shear
plane. Simultaneously, shear-induced cross-correlations between particle
fluctuations along orthogonal directions in the shear plane are found. They are
asymmetric in time. In Poiseuille flow thermal particle fluctuations
perpendicular to the flow direction in the shear plane induce a shift of the
particle's mean position away from the potential minimum. Two complementary
methods are suggested to measure shear-induced cross-correlations between
particle fluctuations along orthogonal directions.Comment: 14 pages, 7 figure
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