128 research outputs found
Possibilities for Measurement and Compensation of Stray DC Electric Fields Acting on Drag-Free Test Masses
DC electric fields can combine with test mass charging and thermal dielectric
voltage noise to create significant force noise acting on the drag-free test
masses in the LISA (Laser Interferometer Space Antenna) gravitational wave
mission. This paper proposes a simple technique to measure and compensate
average stray DC potentials at the mV level, yielding substantial reduction in
this source of force noise. We discuss the attainable resolution for both
flight and ground based experiments.Comment: To be published in Advances in Space Research, COSPAR 2002 conference
proceedings (6 pages, 3 figures
Long-term degradation of optical devices on the moon
Forty years ago, Apollo astronauts placed the first of several retroreflector
arrays on the lunar surface. Their continued usefulness for laser-ranging might
suggest that the lunar environment does not damage optical devices. However,
new laser ranging data reveal that the efficiency of the three Apollo reflector
arrays is now diminished by a factor of ten at all lunar phases and by an
additional factor of ten when the lunar phase is near full moon. These deficits
did not exist in the earliest years of lunar ranging, indicating that the lunar
environment damages optical equipment on the timescale of decades. Dust or
abrasion on the front faces of the corner-cube prisms may be responsible,
reducing their reflectivity and degrading their thermal performance when
exposed to face-on sunlight at full moon. These mechanisms can be tested using
laboratory simulations and must be understood before designing equipment
destined for the moon.Comment: 9 pages; 4 figures; accepted for publication in Icaru
A Note on the Integral Formulation of Einstein's Equations Induced on a Braneworld
We revisit the integral formulation (or Green's function approach) of
Einstein's equations in the context of braneworlds. The integral formulation
has been proposed independently by several authors in the past, based on the
assumption that it is possible to give a reinterpretation of the local metric
field in curved spacetimes as an integral expression involving sources and
boundary conditions. This allows one to separate source-generated and
source-free contributions to the metric field. As a consequence, an exact
meaning to Mach's Principle can be achieved in the sense that only
source-generated (matter fields) contributions to the metric are allowed for;
universes which do not obey this condition would be non-Machian. In this paper,
we revisit this idea concentrating on a Randall-Sundrum-type model with a
non-trivial cosmology on the brane. We argue that the role of the surface term
(the source-free contribution) in the braneworld scenario may be quite subtler
than in the 4D formulation. This may pose, for instance, an interesting issue
to the cosmological constant problem.Comment: 10 pages, no figures, accepted for publication in the General
Relativity and Gravitation Journa
Dark Energy and Extending the Geodesic Equations of Motion: Its Construction and Experimental Constraints
With the discovery of Dark Energy, , there is now a universal
length scale, , associated with the
universe that allows for an extension of the geodesic equations of motion. In
this paper, we will study a specific class of such extensions, and show that
contrary to expectations, they are not automatically ruled out by either
theoretical considerations or experimental constraints. In particular, we show
that while these extensions affect the motion of massive particles, the motion
of massless particles are not changed; such phenomena as gravitational lensing
remain unchanged. We also show that these extensions do not violate the
equivalence principal, and that because Mpc, a
specific choice of this extension can be made so that effects of this extension
are not be measurable either from terrestrial experiments, or through
observations of the motion of solar system bodies. A lower bound for the only
parameter used in this extension is set.Comment: 19 pages. This is the published version of the first half of
arXiv:0711.3124v2 with corrections include
The Collapse of Large Extra Dimensions
In models of spacetime that are the product of a four-dimensional spacetime
with an ``extra'' dimension, there is the possibility that the extra dimension
will collapse to zero size, forming a singularity. We ask whether this collapse
is likely to destroy the spacetime. We argue, by an appeal to the
four-dimensional cosmic censorship conjecture, that--at least in the case when
the extra dimension is homogeneous--such a collapse will lead to a singularity
hidden within a black string. We also construct explicit initial data for a
spacetime in which such a collapse is guaranteed to occur and show how the
formation of a naked singularity is likely avoided.Comment: Uses revtex
Vanishing of cosmological constant in nonfactorizable geometry
We generalize the results of Randall and Sundrum to a wider class of
four-dimensional space-times including the four-dimensional Schwarzschild
background and de Sitter universe. We solve the equation for graviton
propagation in a general four dimensional background and find an explicit
solution for a zero mass bound state of the graviton. We find that this zero
mass bound state is normalizable only if the cosmological constant is strictly
zero, thereby providing a dynamical reason for the vanishing of cosmological
constant within the context of this model. We also show that the results of
Randall and Sundrum can be generalized without any modification to the
Schwarzschild background.Comment: 8 Pages(expanded version), Accepted in Phys. Rev.
Charge Asymmetry in the Brane World and Formation of Charged Black Holes
In theories with an infinite extra dimension, free particles localized on the
brane can leak out to the extra space. We argue that if there were color
confinement in the bulk, electrons would be more able to escape than quarks and
than protons (which are composed states). Thus, this process generates an
electric charge asymmetry on brane matter densities. A primordial charge
asymmetry during Big Bang Nucleosynthesis era is predicted. We use current
bounds on this and on electron disappearance to constrain the parameter space
of these models. Although the generated asymmetry is generically small, it
could be particularly enhanced on large densities as in astrophysical objects,
like massive stars. We suggest the possibility that such accumulation of charge
may be linked, upon supernova collapse, to the formation of a charged Black
Hole and the generation of Gamma-Ray Bursts.Comment: Four pages, one figure. Minor changes, conclusions remai
Sub-millimeter Tests of the Gravitational Inverse-square Law
Motivated by a variety of theories that predict new effects, we tested the
gravitational 1/r^2 law at separations between 10.77 mm and 137 microns using
two different 10-fold azimuthally symmetric torsion pendulums and rotating
10-fold symmetric attractors. Our work improves upon other experiments by up to
a factor of about 100. We found no deviation from Newtonian physics at the 95%
confidence level and interpret these results as constraints on extensions of
the Standard Model that predict Yukawa or power-law forces. We set a constraint
on the largest single extra dimension (assuming toroidal compactification and
that one extra dimension is significantly larger than all the others) of R <=
160 microns, and on two equal-sized large extra dimensions of R <= 130 microns.
Yukawa interactions with |alpha| >= 1 are ruled out at 95% confidence for
lambda >= 197 microns. Extra-dimensions scenarios stabilized by radions are
restricted to unification masses M >= 3.0 TeV/c^2, regardless of the number of
large extra dimensions. We also provide new constraints on power-law potentials
V(r)\propto r^{-k} with k between 2 and 5 and on the gamma_5 couplings of
pseudoscalars with m <= 10 meV/c^2.Comment: 34 pages, 38 figure
Modified Gravity via Spontaneous Symmetry Breaking
We construct effective field theories in which gravity is modified via
spontaneous breaking of local Lorentz invariance. This is a gravitational
analogue of the Higgs mechanism. These theories possess additional graviton
modes and modified dispersion relations. They are manifestly well-behaved in
the UV and free of discontinuities of the van Dam-Veltman-Zakharov type,
ensuring compatibility with standard tests of gravity. They may have important
phenomenological effects on large distance scales, offering an alternative to
dark energy. For the case in which the symmetry is broken by a vector field
with the wrong sign mass term, we identify four massless graviton modes (all
with positive-definite norm for a suitable choice of a parameter) and show the
absence of the discontinuity.Comment: 5 pages; revised versio
- …