output
20022013
most citedA direct empirical proof of the existence of dark matter

2.4k citations

Showing 2005Show all

18 papers · 1 filter

astro-ph2005

GALEX Detection of Lyman Break Galaxies at z=1 in the CDFS

D. Burgarella, P. Perez-Gonzalez, V. Buat +5

The first large sample of Lyman Break Galaxies (LBGs) at z~1 is selected from GALEX Far-UV and Near-UV images of the Chandra Deep Field South. This multi-wavelength study is based…

math-ph200519 cited

Mott transition in lattice boson models

Roberto Fernandez, Juerg Froehlich, Daniel Ueltschi

We use mathematically rigorous perturbation theory to study the transition between the Mott insulator and the conjectured Bose-Einstein condensate in a hard-core Bose-Hubbard model…

cond-mat.mtrl-sci200511 cited

Microstructure and velocity of field-driven solid-on-solid interfaces moving under stochastic dynamics with local energy barriers

G. M. Buendia, P. A. Rikvold, M. Kolesik

We study the microscopic structure and the stationary propagation velocity of (1+1)-dimensional solid-on-solid interfaces in an Ising lattice-gas model, which are driven far from e…

cond-mat.mes-hall200555 cited

Quantum-to-classical correspondence in open chaotic systems

Henning Schomerus, Philippe Jacquod

We review properties of open chaotic mesoscopic systems with a finite Ehrenfest time tau_E. The Ehrenfest time separates a short-time regime of the quantum dynamics, where wave pac…

cond-mat.other200517 cited

Full counting statistics of heteronuclear molecules from Feshbach-assisted photo association

A. Nunnenkamp, D. Meiser, P. Meystre

We study the effects of quantum statistics on the counting statistics of ultracold heteronuclear molecules formed by Feshbach-assisted photoassociation [Phys. Rev. Lett. {\bf 93},…

astro-ph2005

Effects of mass loss for highly-irradiated giant planets

W. B. Hubbard, M. F. Hattori, A. Burrows +2

We present calculations for the evolution and surviving mass of highly-irradiated extrasolar giant planets (EGPs) at orbital semimajor axes ranging from 0.023 to 0.057 AU using a g…