14 citations · 17 across the 9 of their papers we have counts for
9 papers
GRACE: An Open-Source Framework for GPU-Accelerated Numerical Relativity
Carlo Musolino, Christian Ecker, Konrad Topolski +6
We present GRACE, a new GPU-accelerated numerical-relativity framework designed to run efficiently on heterogeneous high-performance computing platforms. Developed from scratch and…
A formation scenario of black hole-envelope systems --viscous hydrodynamics simulation in general relativity--
Alan Tsz Lok Lam, Masaru Shibata, Kenta Hotokezaka +1
By performing a viscous hydrodynamics simulation in general relativity for super-Eddington accretion flows onto massive black holes of mass --, we discuss a fo…
A "Neural" Riemann solver for Relativistic Hydrodynamics
Carlo Musolino
In this paper, we present an approach to solving the Riemann problem in one-dimensional relativistic hydrodynamics, where the most computationally expensive steps of the exact solv…
Accurate muonic interactions in neutron star mergers and impact on heavy-element nucleosynthesis
Harry Ho-Yin Ng, Carlo Musolino, Samuel D. Tootle +1
The abundances resulting from -process nucleosynthesis as predicted by simulations of binary neutron star (BNS) mergers remain an open question as the current state of the art i…
On the impact of neutrinos on the launching of relativistic jets from "magnetars" produced in neutron-star mergers
Carlo Musolino, Luciano Rezzolla, Elias R. Most
A significant interest has emerged recently in assessing whether collimated and ultra-relativistic outflows can be produced by a long-lived remnant from a binary neutron-star (BNS)…
"Extended emission" from fallback accretion onto merger remnants
Carlo Musolino, Raphaël Duqué, Luciano Rezzolla
Using a set of general-relativistic magnetohydrodynamics simulations that include proper neutrino transfer, we assess for the first time the role played by the fallback accretion o…
A hybrid approach to long-term binary neutron-star simulations
Harry Ho-Yin Ng, Jin-Liang Jiang, Carlo Musolino +3
One of the main challenges in the numerical modeling of binary neutron-star (BNS) mergers is long-term simulations of the post-merger remnant over timescales of the order of second…
On the maximum mass and oblateness of rotating neutron stars with generic equations of state
Carlo Musolino, Christian Ecker, Luciano Rezzolla
A considerable effort has been dedicated recently to the construction of generic equations of state (EOSs) for matter in neutron stars. The advantage of these approaches is that th…
A practical guide to a moment approach for neutrino transport in numerical relativity
Carlo Musolino, Luciano Rezzolla
The development of a neutrino moment based radiative-transfer code to simulate binary neutron-star mergers can easily become an obstacle path because of the numerous ways in which…