output
19922026
most citedThe SIESTA method for ab initio order-N materials simulation

12k citations

Showing 2012Show all

179 papers · 1 filter

astro-ph.CO2012★ 2 cited

An expanding universe without dark matter and dark energy

Pierre Magain

Assuming that observers located inside the Universe measure a time flow which is different from the time appearing in the Friedmann-Lemaitre equation, and determining this time flo…

hep-ph2012★ 128 cited

First extraction of valence transversities in a collinear framework

Alessandro Bacchetta, A. Courtoy, Marco Radici

We present an extraction of the valence transversity parton distributions based on an analysis of pion-pair production in deep-inelastic scattering off transversely polarized targe…

hep-ph2012★ 2 cited

Scalar triplet leptogenesis without right-handed neutrino decoupling

D. Aristizabal Sierra

We discuss leptogenesis in the context of type-II seesaw in the case in which in addition to the scalar electroweak triplet decays the lepton asymmetry is also induced by right-han…

cs.AI2012★ 17 cited

On the Construction of the Inclusion Boundary Neighbourhood for Markov Equivalence Classes of Bayesian Network Structures

Vincent Auvray, Louis Wehenkel

The problem of learning Markov equivalence classes of Bayesian network structures may be solved by searching for the maximum of a scoring metric in a space of these classes. This p…

astro-ph.SR2012★ 48 cited

Mode visibilities in rapidly rotating stars

D. R. Reese, V. Prat, C. Barban +2

Context: Mode identification is a crucial step to comparing observed frequencies with theoretical ones, but has proven to be difficult in rapidly rotating stars. Aims: To further c…

astro-ph.SR2012★ 25 cited

The 2.35 year itch of Cyg OB2 #9. II. Radio monitoring

R. Blomme, Y. Naze, D. Volpi +5

Cyg OB2 #9 is one of a small set of non-thermal radio emitting massive O-star binaries. The non-thermal radiation is due to synchrotron emission in the colliding-wind region. Cyg O…