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20052009
most citedA test of the nature of cosmic acceleration using galaxy redshift distortions

670 citations

Showing 2009Show all

6 papers · 1 filter

physics.class-ph200978 cited

Nucleation of spherical shell-like interfaces by second gradient theory: numerical simulations

Francesco Dell'Isola, Henri Gouin, Giacomo Rotoli

The theory of second gradient fluids (which are able to exert shear stresses also in equilibrium conditions) allows us: (i) to describe both the thermodynamical and the mechanical…

math-ph20093 cited

The Hamilton principle for fluid binary mixtures with two temperatures

Henri Gouin, Tommaso Ruggeri

For binary mixtures of fluids without chemical reactions, but with components having different temperatures, the Hamilton principle of least action is able to produce the equation…

astro-ph.GA200942 cited

A forming, dust enshrouded disk at z=0.43: the first example of a late type disk rebuilt after a major merger?

F. Hammer, H. Flores, Y. B. Yang +4

Abreg: By combining HST/UDF imagery with kinematics from VLT/GIRAFFE we derive a physical model of distant galaxy J033245.11-274724.0 in a way similar to what can be done in the ne…

astro-ph.GA200960 cited

Keck spectroscopic survey of strongly lensed galaxies in Abell 1703: further evidence for a relaxed, unimodal cluster

Johan Richard, Liuyi Pei, Marceau Limousin +2

Strong gravitational lensing is a unique tool to model with great accuracy the inner mass distribution of massive galaxy clusters. In particular, clusters with large Einstein radii…

math-ph20092 cited

Barriers for the reduction of transport due to the EXB drift in magnetized plasmas

Natalia Tronko, Michel Vittot, Cristel Chandre +2

We consider a 1 1/2degrees of freedom Hamiltonian dynamical system, which models the chaotic dynamics of charged test-particles in a turbulent electric field, across the confining…

astro-ph20096 cited

The MiMeS Project: Magnetism in Massive Stars

G. A. Wade, E. Alecian, D. A. Bohlender +11

The Magnetism in Massive Stars (MiMeS) Project is a consensus collaboration among the foremost international researchers of the physics of hot, massive stars, with the basic aim of…