collaborators

6 papers

astro-ph.HE2026

Magnetic Eruption and Nucleosynthesis in GRνMHD Simulations of Spinning Neutron Star Mergers

Allen Wen, Jay V. Kalinani, Michail Chabanov +3

We present three-dimensional general relativistic magnetohydrodynamics simulations of equal-mass binary neutron star mergers with varied neutron star spin configurations and second…

astro-ph.HE2026

Jet-environment interaction after delayed collapse in binary neutron star mergers

Jay V. Kalinani, Riccardo Ciolfi, Manuela Campanelli +4

We present general relativistic magnetohydrodynamic simulations of binary neutron star (BNS) mergers, where the collapse of the metastable massive neutron star (MNS) remnant leads…

gr-qc2026

Accelerating Numerical Relativity Simulations with New Multistep Fourth-Order Runge-Kutta Methods

Lucas Timotheo Sanches, Steven Robert Brandt, Jay Kalinani +2

Many HPC applications that solve differential equations rely on the Runge-Kutta family of methods for time integration. Among these methods, the fourth-order accurate RK4 scheme is…

astro-ph.HE2025

Relativistic gas accretion onto supermassive black Hole binaries from inspiral through merger

Lorenzo Ennoggi, Manuela Campanelli, Yosef Zlochower +8

Accreting supermassive black hole binaries are powerful multimessenger sources emitting both gravitational and EM radiation. Understanding the accretion dynamics of these systems a…

astro-ph.HE2025

Role of injection parameters in jet propagation through realistic binary neutron star merger environments

Andrea Pavan, Riccardo Ciolfi, Emma Dreas +1

After the first multi-messenger observation of a binary neutron star (BNS) merger powering a short-duration gamma-ray burst (GRB), GW170817-GRB 170817A, remarkable effort is ongoin…

astro-ph.HE2025

AsterX: a new open-source GPU-accelerated GRMHD code for dynamical spacetimes

Jay V. Kalinani, Liwei Ji, Lorenzo Ennoggi +10

We present AsterX, a novel open-source, modular, GPU-accelerated, fully general relativistic magnetohydrodynamic (GRMHD) code designed for dynamic spacetimes in 3D Cartesian coordi…