122 research outputs found
Mode coupling evolution in arbitrary inflationary backgrounds
The evolution of high order correlation functions of a test scalar field in
arbitrary inflationary backgrounds is computed. Whenever possible, exact
results are derived from quantum field theory calculations. Taking advantage of
the fact that such calculations can be mapped, for super-horizon scales, into
those of a classical system, we express the expected correlation functions in
terms of classical quantities, power spectra, Green functions, that can be
easily computed in the long-wavelength limit. Explicit results are presented
that extend those already known for a de Sitter background. In particular the
expressions of the late time amplitude of bispectrum and trispectrum, as well
as the whole high-order correlation structure, are given in terms of the
expansion factor behavior. When compared to the case of a de Sitter background,
power law inflation and chaotic inflation induced by a massive field are found
to induce high order correlation functions the amplitudes of which are
amplified by almost one order of magnitude. These results indicate that the
dependence of the related non-Gaussian parameters - such as f_NL - on the
wave-modes is at percent level.Comment: 22 pages, 5 figures. Revised version with correction of typos and
more detailed discussions on the validity regime of the calculation
Constraints on higher-dimensional gravity from the cosmic shear three-point correlation function
With the developments of large galaxy surveys or cosmic shear surveys it is
now possible to map the dark matter distribution at truly cosmological scales.
Detailed examinations of the statistical properties of the dark matter
distribution reveal the detail of the large-scale structure growth of the
Universe. In particular it is shown here that the behavior of the density field
bi-spectrum is sensitive to departure from normal gravity in a way which
depends only weakly on the background evolution. The cosmic shear bispectrum
appears to be particularly sensitive to changes in the Poisson equation: we
show that the current cosmic shear data can already be used to infer
constraints on the scale of a possible higher-dimensional gravity, above 2
h^{-1}Mpc.Comment: 5 pages, 3 figures, submitted to PR
Cosmological Perturbation Theory for streams of relativistic particles
Motion equations describing streams of relativistic particles and their
properties are explored in detail in the framework of Cosmological Perturbation
Theory. Those equations, derived in any metric both in the linear and nonlinear
regimes, express the matter and momentum conservation. In this context we
extend the setup of adiabatic initial conditions - that was initially performed
in the Conformal Newtonian gauge - to the Synchronous gauge. The subhorizon
limit of the nonlinear motion equations written in a generic perturbed
Friedmann-Lema\^{i}tre metric is then derived and analyzed. We show in
particular that the momentum field is always potential in the linear
regime and remains so at subhorizon scales in the nonlinear regime. Finally the
equivalence principle is exploited to highlight invariance properties satisfied
by such a system of equations, extending that known for streams of
non-relativistic particles, namely the extended Galilean invariance
Describing massive neutrinos in cosmology as a collection of independent flows
A new analytical approach allowing to account for massive neutrinos in the
non-linear description of the growth of the large-scale structure of the
universe is proposed. Unlike the standard approach in which neutrinos are
described as a unique hot fluid, it is shown that the overall neutrino fluid
can be equivalently decomposed into a collection of independent flows. Starting
either from elementary conservation equations or from the evolution equation of
the phase-space distribution function, we derive the two non-linear motion
equations that each of these flows satisfies. Those fluid equations describe
the evolution of macroscopic fields. We explain in detail the connection
between the collection of flows we defined and the standard massive neutrino
fluid. Then, in the particular case of adiabatic initial conditions, we
explicitly check that, at linear order, the resolution of this new system of
equations reproduces the results obtained in the standard approach based on the
collisionless Boltzmann hierarchy. Besides, the approach advocated in this
paper allows to show how each neutrino flow settles into the cold dark matter
flow depending on initial velocities. It opens the way to a fully non-linear
treatment of the dynamical evolution of neutrinos in the framework of
large-scale structure growth.Comment: 23 pages, 4 figure
On the importance of nonlinear couplings in large-scale neutrino streams
We propose a procedure to evaluate the impact of nonlinear couplings on the
evolution of massive neutrino streams in the context of large-scale structure
growth. Such streams can be described by general nonlinear conservation
equations, derived from a multiple-flow perspective, which generalize the
conservation equations of non-relativistic pressureless fluids. The relevance
of the nonlinear couplings is quantified with the help of the eikonal
approximation applied to the subhorizon limit of this system. It highlights the
role played by the relative displacements of different cosmic streams and it
specifies, for each flow, the spatial scales at which the growth of structure
is affected by nonlinear couplings. We found that, at redshift zero, such
couplings can be significant for wavenumbers as small as /Mpc for
most of the neutrino streams.Comment: 12 pages, 1 figur
Cosmic Strings Lens Phenomenology Revisited
We present investigations of lens phenomenological properties of cosmic
strings for deep galaxy surveys. General results that have obtained for lineic
energy distribution are presented first. We stress that generically the local
convergence always vanishes in presence of strings although there might be some
significant distortions. We then propose a simplified model of strings, we call
``Poisson strings'', for which exhaustive investigations can be done either
numerically or analytically.Comment: 6 pages; To appear in the Proceedings of the XXth Moriond
Astrophysics Meeting "Cosmological Physics with Gravitational Lensing", eds.
J.-P. Kneib, Y. Mellier, M. Moniez and J. Tran Thanh Van, Les Arcs, France,
March 11th-18th 200
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