collaborators
Showing astro-ph.HEShow all

5 papers · 1 filter

astro-ph.HE2026

The Hidden Evolution of Gamma-Ray Burst Jets Revealed by Gravitational Waves

Gerardo Urrutia, Fabio De Colle, Agnieszka Janiuk +2

Gamma-ray burst (GRB) jets can propagate through massive stars, where the high opacity of the stellar envelope traps electromagnetic radiation and limits observations of the jet at…

astro-ph.HE2026

Bayesian parameter estimation for the Core-bounce phase of Rapidly Rotating Core-Collapse Supernovae in real interferometric data

Emmanuel Avila, Michele Zanolin, Javier M. Antelis +1

We present a novel methodology to estimate the ratio of kinetic to gravitational potential energy in core-collapse supernova progenitors and to assess the equation of state (EOS) u…

astro-ph.HE2026

Joint Detection and Characterization of the Standing Accretion Shock Instability for Core-Collapse Supernovae with cWB XP

Vicente Sierra, Zidu Lin, Michelle Zanolin +3

The most sensitive to-date multimessenger detection of the standing accretion shock instability in real interferometric data is presented, which quantitatively identifies the prese…

astro-ph.HE2024

Dependence of the Reconstructed Core-Collapse Supernova Gravitational Wave High-Frequency Feature on the Nuclear Equation of State, in Real Interferometric Data

R. Daniel Murphy, Alejandro Casallas-Lagos, Anthony Mezzacappa +6

We present an analysis of gravitational wave (GW) predictions from five two-dimensional Core Collapse Supernova (CCSN) simulations that varied only in the Equation of State (EOS) i…

astro-ph.HE2024

Residual neural networks to classify the high frequency emission in core-collapse supernova gravitational waves

Manuel D. Morales, Javier M. Antelis, Claudia Moreno

We present a new methodology to explore the morphology of the High Frequency Feature (HFF), i.e., the dominant, rising-frequency GW emission from a proto-neutron star in core-colla…