activity
20152024
most citedMini-disk accretion onto spinning black hole binaries: quasi-periodicities and outflows

58 citations · 262 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.HE2024★ 10 cited

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…

gr-qc2023

Ameliorating the Courant-Friedrichs-Lewy condition in spherical coordinates: A double FFT filter method for general relativistic MHD in dynamical spacetimes

Liwei Ji, Vassilios Mewes, Yosef Zlochower +5

Numerical simulations of merging compact objects and their remnants form the theoretical foundation for gravitational wave and multi-messenger astronomy. While Cartesian-coordinate…

astro-ph.HE2022★ 18 cited

First results of the glitching pulsars monitoring program at the Argentine Institute of Radioastronomy

Ezequiel Zubieta, Ryan Missel, Valentina Sosa Fiscella +10

We report here on the first results of a systematic monitoring of southern glitching pulsars at the Argentine Institute of Radioastronomy that started in the year 2019. We detected…

gr-qc2022★ 21 cited

Addition of tabulated equation of state and neutrino leakage support to IllinoisGRMHD

Leonardo R. Werneck, Zachariah B. Etienne, Ariadna Murguia-Berthier +11

We have added support for realistic, microphysical, finite-temperature equations of state (EOS) and neutrino physics via a leakage scheme to IllinoisGRMHD, an open-source GRMHD cod…

astro-ph.HE2021★ 11 cited

Handing off the outcome of binary neutron star mergers for accurate and long-term post-merger simulations

Federico G. Lopez Armengol, Zachariah B. Etienne, Scott C. Noble +20

We perform binary neutron star (BNS) merger simulations in full dynamical general relativity with IllinoisGRMHD, on a Cartesian grid with adaptive-mesh refinement. After the remnan…

astro-ph.HE2021★ 58 cited

Electromagnetic Signatures from Supermassive Binary Black Holes Approaching Merger

Eduardo M. Gutiérrez, Luciano Combi, Scott C. Noble +4

We present fully relativistic predictions for the electromagnetic emission produced by accretion disks surrounding spinning and nonspinning supermassive binary black holes on the v…

astro-ph.HE2021★ 58 cited

Mini-disk accretion onto spinning black hole binaries: quasi-periodicities and outflows

Luciano Combi, Federico G. Lopez Armengol, Manuela Campanelli +4

We perform a full 3D general relativistic magnetohydrodynamical (GRMHD) simulation of an equal-mass, spinning, binary black hole approaching merger, surrounded by a circumbinary di…

astro-ph.HE2021★ 5 cited

Vela Pulsar: Single Pulses Analysis with Machine Learning Techniques

Carlos O. Lousto, Ryan Missel, Harsh Prajapati +12

We study individual pulses of Vela (PSR\ B0833-45\,/\,J0835-4510) from daily observations of over three hours (around 120,000 pulses per observation), performed simultaneously with…

astro-ph.HE2021★ 25 cited

HARM3D+NUC: A new method for simulating the post-merger phase of binary neutron star mergers with GRMHD, tabulated EOS and neutrino leakage

Ariadna Murguia-Berthier, Scott C. Noble, Luke F. Roberts +25

The first binary neutron star merger has already been detected in gravitational waves. The signal was accompanied by an electromagnetic counterpart including a kilonova component p…

astro-ph.HE2016★ 20 cited

Effects of Scalar-Tensor-Vector Gravity on relativistic jets

Federico G. Lopez Armengol, Gustavo E. Romero

Scalar-Tensor-Vector Gravity (STVG) is a theory that does not require dark components to describe astrophysical data. We aim at constraining the free parameters of STVG based on re…

gr-qc2016★ 35 cited

Neutron stars in Scalar-Tensor-Vector Gravity

Federico G. Lopez Armengol, Gustavo E. Romero

Scalar-Tensor-Vector Gravity (STVG), also referred as MOdified Gravity (MOG), is an alternative theory of the gravitational interaction. Its weak field approximation has been succe…

gr-qc2015★ 1 cited

Cosmological black holes and the direction of time

Gustavo E. Romero, Daniela Pérez, Federico G. Lopez Armengol

Macroscopic irreversible processes emerge from fundamental physical laws of reversible character. The source of the local irreversibility seems to be not in the laws themselves but…