activity
20242026
collaborators

6 papers

astro-ph.IM2026

STORM: RDMA-based Monte Carlo Transport Scheme for Distributed-Memory Particle Simulations

Maor Mizrachi, Barak Raveh, Elad Steinberg

Monte Carlo particle transport enables high-fidelity astrophysical radiation and neutrino simulations - from core-collapse supernovae and neutron-star mergers to accretion flows -…

astro-ph.HE2026

Multigroup Radiation Diffusion on a Moving Mesh: Implementation in RICH and Application to Tidal Disruption Events

Itamar Giron, Menahem Krief, Nicholas C. Stone +1

Radiation-hydrodynamics (RHD) determines the bulk evolution and observable emission in a wide variety of high-energy astrophysical phenomena. Due to their complexity, RHD problems…

astro-ph.HE2025

Wind-mediated Eddington-limited emission in a Black Hole Tidal Disruption Event

Paola Martire, Elena Maria Rossi, Nicholas Chamberlain Stone +3

Observations of tidal disruption events (TDEs) have already produced tens of strong candidate flares, and their number will greatly increase with upcoming wide field surveys. Never…

astro-ph.IM2025

MadVoro: Parallel Construction of Voronoi Diagrams in Distributed Memory Systems

Maor Mizrachi, Barak Raveh, Elad Steinberg

Voronoi diagrams are essential geometrical structures with numerous applications, particularly astrophysics-driven finite volume methods. While serial algorithms for constructing t…

astro-ph.HE2024

The non-equilibrium Marshak wave problem in non-homogeneous media

Nitay Derei, Shmuel Balberg, Shay I. Heizler +3

We derive a family of similarity solutions to the nonlinear non-equilibrium Marshak wave problem for an inhomogeneous planar medium which is coupled to a time dependent radiation d…

astro-ph.HE2024

The Primary Flare Following a Stellar Collision in a Galactic Nucleus

Yuval Brutman, Elad Steinberg, Shmuel Balberg

High-velocity stellar collisions near supermassive black holes may result in a complete disruption of the stars. The initial disruption can have energies on par with supernovae and…