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19972026
most citedProspects for Fundamental Physics with LISA

401 citations · 3.6k across the 126 of their papers we have counts for

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40 papers · 1 filter

astro-ph2008★ 36 cited

Propagators in Lagrangian space

Francis Bernardeau, Patrick Valageas

It has been found recently that propagators, e.g. the cross-correlation spectra of the cosmic fields with the initial density field, decay exponentially at large-k in an Eulerian d…

astro-ph2007★ 32 cited

Expansion schemes for gravitational clustering: computing two-point and three-point functions

P. Valageas

We describe various expansion schemes that can be used to study gravitational clustering. Obtained from the equations of motion or their path-integral formulation, they provide sev…

astro-ph2007★ 37 cited

Using the Zeldovich dynamics to test expansion schemes

Patrick Valageas

We apply various expansion schemes that may be used to study gravitational clustering to the simple case of the Zeldovich dynamics. Using the well-known exact solution of the Zeldo…

astro-ph2006★ 304 cited

Cosmology with Weak Lensing Surveys

D. Munshi, P. Valageas, L. Van Waerbeke +1

Weak gravitational lensing is responsible for the shearing and magnification of the images of high-redshift sources due to the presence of intervening matter. The distortions are d…

astro-ph2006★ 88 cited

Large-N expansions applied to gravitational clustering

Patrick Valageas

We develop a path-integral formalism to study the formation of large-scale structures in the universe. Starting from the equations of motion of hydrodynamics (single-stream approxi…

astro-ph2006★ 35 cited

Relaxation of a 1-D gravitational system

Patrick Valageas

We study the relaxation towards thermodynamical equilibrium of a 1-D gravitational system. This OSC model shows a series of critical energies where new equilibria appear a…

astro-ph2006

How many SNeIa do we need to detect the effect of weak lensing ?

Dipak Munshi, Patrick Valageas

We show that as many as 4000 SNeIa may be required to detect the effect of weak lensing on their flux distribution with a high level of significance. However, if the intrinsic SNeI…

astro-ph2006★ 44 cited

Thermodynamics and dynamics of a 1-D gravitational system

Patrick Valageas

We describe a one-dimensional self-gravitating system derived from the problem of large-scale structure formation in cosmology. Considering small times so that the expansion can be…

astro-ph2005

Do measurements of the one-point distribution of aperture-mass improve constraints on cosmology ?

Dipak Munshi, Patrick Valageas

We study the possibility of using the entire probability distribution function (PDF) of the aperture mass Map and its related cumulative probability distribution function (CPDF) to…

astro-ph2005

Cosmological Constraints from Weak Lensing Surveys

Dipak Munshi, Patrick Valageas

Focusing on the well motivated aperture mass statistics $\Map$, we study the possibility of constraining cosmological parameters using future space based SNAP class weak lensing mi…

astro-ph2005★ 9 cited

Cosmology with Weak Lensing Surveys

Dipak Munshi, Patrick Valageas

Weak gravitational lensing surveys measure the distortion of the image of distant sources due to the deflections of light rays by the fluctuations of the gravitational potential al…

astro-ph2004★ 6 cited

Covariance of Weak Lensing Observables

Dipak Munshi, Patrick Valageas

Analytical expressions for covariances of weak lensing statistics related to the aperture mass $\Map$ are derived for realistic survey geometries such as SNAP for a range of smooth…

astro-ph2004★ 5 cited

On Cross-correlating Weak Lensing Surveys

Dipak Munshi, Patrick Valageas

The present generation of weak lensing surveys will be superseded by surveys run from space with much better sky coverage and high level of signal to noise ratio, such as SNAP. How…

astro-ph2004★ 18 cited

Evolution of the Cosmological Density Distribution Function: A New Analytical Model

Patrick Valageas, Dipak Munshi

The one-point probability distribution function (pdf) of the large-scale density field is an important tool to follow the evolution of cosmological structures. In this paper we pre…

astro-ph2004★ 17 cited

On the estimation of gravity-induced non-Gaussianities from weak lensing surveys

Patrick Valageas, Dipak Munshi, Andrew J. Barber

We study various measures of weak lensing distortions in future surveys, taking into account the noise arising from the finite survey size and the intrinsic ellipticity of galaxies…

astro-ph2003★ 31 cited

Weak lensing shear and aperture-mass from linear to non-linear scales

Dipak Munshi, Patrick Valageas, Andrew J. Barber

In this paper we describe the predictions for the smoothed weak lensing shear and aperture-mass of two simple analytical models of the density field: the minimal tree-model and the…

astro-ph2003★ 64 cited

A new approach to gravitational clustering: a path-integral formalism and large-N expansions

P. Valageas

We show that the formation of large-scale structures through gravitational instability in the expanding universe can be fully described through a path-integral formalism. We derive…

astro-ph2003★ 23 cited

From linear to non-linear scales: analytical and numerical predictions for the weak lensing convergence

Andrew J. Barber, Dipak Munshi, Patrick Valageas

Weak lensing convergence can be used directly to map and probe the dark mass distribution in the universe. Building on earlier studies, we recall how the statistics of the converge…

astro-ph2003★ 22 cited

Analytical Predictions for Statistics of Cosmic Shear: Tests Against Simulations

Patrick Valageas, Andrew J. Barber, Dipak Munshi

Weak gravitational lensing surveys are rapidly becoming important tools to probe directly the mass density fluctuations in the universe and its background dynamics. Earlier studies…

astro-ph2002★ 16 cited

The phase-diagram of the IGM and the entropy floor of groups and clusters: are clusters born warm?

P. Valageas, R. Schaeffer, J. Silk

We point out that two problems of observational cosmology, the facts i) that > 60% of the baryonic content of the universe is not observed at z=0 and ii) that the properties of sma…

astro-ph2001★ 16 cited

Transients from Zel'dovich initial conditions

P. Valageas

We investigate the error implied by the use of the Zel'dovich approximation to set up the initial conditions at a finite redshift zi in numerical simulations. Using a steepest-desc…

astro-ph2001★ 28 cited

Dynamics of gravitational clustering V. Subleading corrections in the quasi-linear regime

P. Valageas

We investigate the properties of the standard perturbative expansions which describe the early stages of the dynamics of gravitational clustering. We show that for hierarchical sce…

astro-ph2001★ 23 cited

Dynamics of gravitational clustering IV. The probability distribution of rare events

P. Valageas

Using a non-perturbative method developed in a previous article (paper II) we investigate the tails of the probability distribution of the overdensity within spherical cel…

astro-ph2001★ 12 cited

Dynamics of gravitational clustering III. The quasi-linear regime for some non-Gaussian initial conditions

P. Valageas

Using a non-perturbative method developed in a previous work (paper II), we derive the probability distribution of the density contrast within spherical cells in the quasi…