activity
20182026
most citedRevival of the Fittest: Exploding Core-Collapse Supernovae from 12 to 25 M

96 citations · 335 across the 37 of their papers we have counts for

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Showing 2024Show all

17 papers · 1 filter

astro-ph.HE2024

Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars

Rosalba Perna, Ore Gottlieb, Estuti Shukla +1

The fate of the binary neutron star (NS) merger remnants hinges sensitively upon the NS equation of state and the threshold mass, , that separates a long-lived from a s…

astro-ph.HE2024★ 7 cited

Open-source library for performance-portable neutrino reaction rates: Application to neutron star mergers

Leonardo Chiesa, Maitraya Bhattacharyya, Filippo Mazzini +3

A realistic and detailed description of neutrinos in binary neutron star (BNS) mergers is essential to build reliable models of such systems. To this end, we present BNS_NURATES, a…

gr-qc2024★ 8 cited

Binary Black Hole Waveforms from High-Resolution GR-Athena++ Simulations

Alireza Rashti, Rossella Gamba, Koustav Chandra +4

The detection and subsequent inference of binary black hole signals rely heavily on the accuracy of the waveform model employed. In the highly non-linear, dynamic, and strong-field…

astro-ph.HE2024★ 21 cited

Gamma-ray bursts and kilonovae from the accretion-induced collapse of white dwarfs

Patrick Chi-Kit Cheong, Tetyana Pitik, Luís Felipe Longo Micchi +1

We present the first seconds-long 2D general relativistic neutrino magnetohydrodynamic simulations of accretion-induced collapse (AIC) in rapidly rotating, strongly magnetized whit…

gr-qc2024★ 1 cited

Performance-Portable Numerical Relativity with AthenaK

Hengrui Zhu, Jacob Fields, Francesco Zappa +6

We present the numerical relativity module within AthenaK, an open source performance-portable astrophysics code designed for exascale computing applications. This module employs t…

astro-ph.HE2024★ 13 cited

Long-lived neutron-star remnants from asymmetric binary neutron star mergers: element formation, kilonova signals and gravitational waves

Sebastiano Bernuzzi, Fabio Magistrelli, Maximilian Jacobi +3

We present 3D general-relativistic neutrino-radiation hydrodynamics simulations of two asymmetric binary neutron star mergers producing long-lived neutron stars remnants and spanni…

astro-ph.HE2024★ 15 cited

Performance-Portable Binary Neutron Star Mergers with AthenaK

Jacob Fields, Hengrui Zhu, David Radice +4

We introduce an extension to the AthenaK code for general-relativistic magnetohydrodynamics (GRMHD) in dynamical spacetimes using a 3+1 conservative Eulerian formulation. Like the…

astro-ph.HE2024★ 6 cited

Tight bound on neutron-star radius with quasiperiodic oscillations in short gamma-ray bursts

Victor Guedes, David Radice, Cecilia Chirenti +1

Quasiperiodic oscillations (QPOs) have been recently discovered in the short gamma-ray bursts (GRBs) 910711 and 931101B. Their frequencies are consistent with those of the quasirad…

astro-ph.HE2024★ 7 cited

Cocoon shock breakout emission from binary neutron star mergers

Eduardo M. Gutiérrez, Mukul Bhattacharya, David Radice +2

Shock breakout emission is among the first observable signals in a wide variety of astrophysical phenomena, including neutron star (NS) mergers, and it can be the dominant componen…

nucl-th2024★ 35 cited

Neutron stars and the dense matter equation of state: from microscopic theory to macroscopic observations

Katerina Chatziioannou, H. Thankful Cromartie, Stefano Gandolfi +4

The past years have witnessed tremendous progress in understanding the properties of neutron stars and of the dense matter in their cores, made possible by electromagnetic observat…

astro-ph.HE2024★ 2 cited

General relativistic hydrodynamic simulations of binary strange star mergers

Francesco Grippa, Aviral Prakash, Domenico Logoteta +2

We perform fully general-relativistic simulations of binary strange star mergers considering two different approaches for thermal effects. The first uses a cold equation of state (…

gr-qc2024

Numerical relativity simulations of compact binaries: comparison of cell- and vertex-centered adaptive meshes

Boris Daszuta, William Cook, Peter Hammond +4

Given the compact binary evolution problem of numerical relativity, in the finite-difference, block-based, adaptive mesh refinement context, choices must be made on how evolved fie…

gr-qc2024★ 26 cited

Scattering and dynamical capture of two black holes: synergies between numerical and analytical methods

Simone Albanesi, Alireza Rashti, Francesco Zappa +6

We study initially unbound systems of two black holes using numerical relativity (NR) simulations performed with GR-Athena++. We focus on regions of the parameter space close to th…

astro-ph.HE2024★ 9 cited

Element formation in radiation-hydrodynamics simulations of kilonovae

Fabio Magistrelli, Sebastiano Bernuzzi, Albino Perego +1

Understanding the details of -process nucleosynthesis in binary neutron star mergers (BNSM) ejecta is key to interpreting kilonova observations and identifying the role of BNSMs…

astro-ph.HE2024★ 18 cited

Turbulence modelling in neutron star merger simulations

David Radice, Ian Hawke

Observations of neutron star mergers have the potential to unveil detailed physics of matter and gravity in regimes inaccessible by other experiments. Quantitative comparisons to t…

astro-ph.HE2024★ 13 cited

Geometric and thermodynamic characterization of binary neutron star accretion discs

Alessandro Camilletti, Albino Perego, Federico Maria Guercilena +2

Accretion disks formed in binary neutron star mergers play a central role in many astrophysical processes of interest, including the launching of relativistic jets or the ejection…

astro-ph.HE2024★ 25 cited

Bayesian inference of multimessenger astrophysical data: Joint and coherent inference of gravitational waves and kilonovae

Matteo Breschi, Rossella Gamba, Gregorio Carullo +4

We present a Bayesian framework for joint and coherent analyses of multimessenger binary neutron star signals. The method, implemented in our bajes infrastructure, incorporates a j…