output
20062025
most citedSMILEI: a collaborative, open-source, multi-purpose particle-in-cell code for plasma simulation

580 citations

Showing 2013Show all

7 papers · 1 filter

astro-ph.GA2013★ 51 cited

Pillars and globules at the edges of H ii regions, Confronting Herschel observations and numerical simulations

P. Tremblin, V. Minier, N. Schneider +24

Pillars and globules are present in many high-mass star-forming regions, such as the Eagle nebula (M16) and the Rosette molecular cloud, and understanding their origin will help ch…

hep-lat2013★ 68 cited

Lattice QCD at the physical point meets SU(2) chiral perturbation theory

Stephan Durr, Zoltan Fodor, Christian Hoelbling +9

We perform a detailed, fully-correlated study of the chiral behavior of the pion mass and decay constant, based on 2+1 flavor lattice QCD simulations. These calculations are implem…

astro-ph.SR2013★ 84 cited

Simulations of protostellar collapse using multigroup radiation hydrodynamics. II. The second collapse

N. Vaytet, G. Chabrier, E. Audit +4

Star formation begins with the gravitational collapse of a dense core inside a molecular cloud. As the collapse progresses, the centre of the core begins to heat up as it becomes o…

math.NA2013★ 25 cited

Simulation of sharp interface multi-material flows involving an arbitrary number of components through an extended five-equation model

Marie Billaud Friess, Samuel Kokh

In this paper, we present an anti-diffusive method dedicated to the simulation of interface flows on Cartesian grids involving an arbitrary number m of compress- ible components. O…

physics.geo-ph2013

Conservative Regridding When Grid Cell Edges Are Unknown -- Case of SCRIP

Joël Chavas, Édouard Audit, Laure Coquart +1

Nowadays, climate models rely on couplers. Each complete climate model is broken into different sub-models (oceanic, atmospheric,...), each one working on a different grid. The cou…

astro-ph.HE2013★ 19 cited

The influence of frequency-dependent radiative transfer on the structures of radiative shocks

N. Vaytet, M. Gonzalez, E. Audit +1

Radiative shocks are shocks in a gas where the radiative energy and flux coming from the very hot post-shock material are non-negligible in the shock's total energy budget, and are…