1,548 research outputs found
A Renormalisation Group Study of Three Dimensional Turbulence
We study the three dimensional Navier-Stokes equation with a random Gaussian
force acting on large wavelengths. Our work has been inspired by Polyakov's
analysis of steady states of two dimensional turbulence. We investigate the
time evolution of the probability law of the velocity potential. Assuming that
this probability law is initially defined by a statistical field theory in the
basin of attraction of a renormalisation fixed point, we show that its time
evolution is obtained by averaging over small scale features of the velocity
potential. The probability law of the velocity potential converges to the fixed
point in the long time regime. At the fixed point, the scaling dimension of the
velocity potential is determined to be . We give conditions for
the existence of such a fixed point of the renormalisation group describing the
long time behaviour of the velocity potential. At this fixed point, the energy
spectrum of three dimensional turbulence coincides with a Kolmogorov spectrum.Comment: 8 pages , tex fil
Screening fifth forces in k-essence and DBI models
New fifth forces have not yet been detected in the laboratory or in the solar
system, hence it is typically difficult to introduce new light scalar fields
that would mediate such forces. In recent years it has been shown that a number
of non-linear scalar field theories allow for a dynamical mechanism, such as
the Vainshtein and chameleon ones, that suppresses the strength of the scalar
fifth force in experimental environments. This is known as screening, however
it is unclear how common screening is within non-linear scalar field theories.
k-essence models are commonly studied examples of non-linear models, with DBI
as the best motivated example, and so we ask whether these non-linearities are
able to screen a scalar fifth force. We find that a Vainshtein-like screening
mechanism exists for such models although with limited applicability. For
instance, we cannot find a screening mechanism for DBI models. On the other
hand, we construct a large class of k-essence models which lead to the
acceleration of the Universe in the recent past for which the fifth force
mediated by the scalar can be screened.Comment: 26 page
Brane World Cosmology, the CMB and the Radion
Recent developments in the theory of extra dimensions have opened up avenues
to confront such theories with cosmological tests. We discuss a brane-world
model with a bulk scalar field, motivated by supergravity. The low-energy
effective action is derived and physical constraints on the parameters of the
model discussed. The cosmological evolution of the brane-world moduli is
investigated and it is shown that one of the moduli is a quintessence field.
The CMB predictions are computed. Finally, the possibility that the radion
field in brane-worlds could be a chameleon field is investigated.Comment: 11 pages, 6 figures, to appear in the proceedings of the DPU
Workshop: The Density Fluctuations in the Universe: Beyond the Inflaton
Paradigm (Athens, June 2004
An Environmental Variation of Constants
Models of modified gravity, whereby local tests of gravity are evaded thanks
to a screening mechanism of the chameleon or Damour-Polyakov types, lead to a
spatial variation of the particle masses and the fine structure constant. This
is triggered by the environmental dependence of the value of the scalar field
whose presence modifies gravity. In dense media, the field settles at a density
dependent value while in sparse environments it takes the background
cosmological value. We estimate that the maximal deviation of constants from
their present values is constrained by local tests of gravity, and must be less
than .Comment: 14 pages, 7 figures, published versio
The Supermoduli Space of Matrix String Theory
We study matrix string scattering amplitudes and matrix string instantons on
a marked Riemann surface in the limit of a vanishing string coupling constant.
We give an explicit parameterization of the moduli space of such instantons. We
also give a description of the set of fermionic supermoduli. The integration
over the supermoduli leads to the inclusion of picture changing operators at
the interaction points. Finally we investigate the large N limit of the measure
on the instanton moduli space and show its convergence to the Weil-Petersson
measure on the moduli space of marked Riemann surfaces.Comment: 30 Pages, Latex, 2 Postscript figure
Lorentz Invariance Violation in Modified Gravity
We consider an environmentally dependent violation of Lorentz invariance in
scalar-tensor models of modified gravity where General Relativity is retrieved
locally thanks to a screening mechanism. We find that fermions have a modified
dispersion relation and would go faster than light in an anisotropic and
space-dependent way along the scalar field lines of force. Phenomenologically,
these models are tightly restricted by the amount of Cerenkov radiation emitted
by the superluminal particles, a constraint which is only satisfied by
chameleons. Measuring the speed of neutrinos emitted radially from the surface
of the earth and observed on the other side of the earth would probe the scalar
field profile of modified gravity models in dense environments. We argue that
the test of the equivalence principle provided by the Lunar ranging experiment
implies that a deviation from the speed of light, for natural values of the
coupling scale between the scalar field and fermions, would be below detectable
levels, unless gravity is modified by camouflaged chameleons where the field
normalisation is environmentally dependent.Comment: 8 pages, extended discussio
On Brane Cosmology and Naked Singularities
Brane-world singularities are analysed, emphasizing the case of supergravity
in singular spaces where the singularity puzzle is naturally resolved. These
naked singularities are either time-like or null, corresponding to the finite
or infinite amount of conformal time that massless particles take in order to
reach them. Quantum mechanically we show that the brane-world naked
singularities are inconsistent. Indeed we find that time-like singularities are
not wave-regular, so the time-evolution of wave packets is not uniquely defined
in their vicinity, while null singularities absorb incoming radiation. Finally
we stress that for supergravity in singular spaces there is a topological
obstruction, whereby naked singularities are necessarily screened off by the
second boundary brane.Comment: 12 page
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