most cited: A GPU-accelerated relativistic Monte Carlo radiative transfer code

1 citations · 1 across the 2 of their papers we have counts for

collaborators

8 papers

astro-ph.HE20261 cited

: A GPU-accelerated relativistic Monte Carlo radiative transfer code

Pedro Naethe Motta, Rodrigo Nemmen, Abhishek V. Joshi

We introduce , a CUDA/C-based Monte Carlo radiative transfer code accelerated using graphics processing units (GPUs). derives from the CPU-ba…

astro-ph.HE2026

Chasing Gamma-Ray Signals from Binary Neutron Star Coalescences with the Cherenkov Telescope Array: Prospects and Observing Strategies

S. Abe, J. Abhir, A. Abhishek +457

The detection of gravitational waves (GWs) from a binary neutron star (BNS) merger by Advanced LIGO and Advanced Virgo (GW170817), together with its electromagnetic counterpart, th…

astro-ph.HE2025

Prospects for dark matter observations in dwarf spheroidal galaxies with the Cherenkov Telescope Array Observatory

K. Abe, S. Abe, J. Abhir +491

The dwarf spheroidal galaxies (dSphs) orbiting the Milky Way are widely regarded as systems supported by velocity dispersion against self-gravity, and as prime targets for the sear…

astro-ph.HE2025

Spectral Learning of Magnetized Plasma Dynamics: A Neural Operator Application

Roberta Duarte, Rodrigo Nemmen, Reinaldo Santos-Lima

Fourier neural operators (FNOs) provide a mesh-independent way to learn solution operators for partial differential equations, yet their efficacy for magnetized turbulence is large…

astro-ph.HE2025

Galactic transient sources with the Cherenkov Telescope Array Observatory

Cherenkov Telescope Array Observatory Consortium

A wide variety of Galactic sources show transient emission at soft and hard X-ray energies: low- and high-mass X-ray binaries containing compact objects, isolated neutron stars exh…

astro-ph.HE2025

Black hole spectral states revealed in GRMHD simulations with texture memory accelerated cooling

Pedro Naethe Motta, Jonatan Jacquemin-Ide, Rodrigo Nemmen +2

X-ray binaries (XRBs) display spectral state transitions that are accompanied by substantial changes in the hardness, luminosity, and structure of the accretion flow. We developed…