From the Early Slope to Curvature: Future Prospects and challenges for Astrophysical Parameter Estimation Using the Core-Collapse Supernova High-Frequency Feature

arXiv:2607.21925 · gr-qc, astro-ph.HE · Submitted 2026-07-24 · Read on arXiv

Alejandro Casallas-Lagos, Marek Szczepańczyk, Michele Zanolin, Anthony Mezzacappa

gr-qc, astro-ph.HE

Submitted: 2026-07-24

Comments: 11 pages, 3 figures

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

Core — 45× in this paper · explained in 2 episodes
High-Frequency Feature — 7× in this paper
Equation of State (EoS) — 3× in this paper · explained in 4 episodes
Fidelity — 3× in this paper · explained in 2 episodes
Adam — 2× in this paper · explained in 2 episodes
Accretion Shock — 1× in this paper · explained in 1 episode
Accuracy — 1× in this paper · explained in 1 episode
Clustering — 1× in this paper · explained in 2 episodes
Consistency — 1× in this paper · explained in 3 episodes
Degeneracy — 1× in this paper · explained in 3 episodes
Gravitational Wave Emission — 1× in this paper · explained in 2 episodes
Metallicity — 1× in this paper · explained in 3 episodes
Signal-to-noise ratio (SNR) — 1× in this paper · explained in 2 episodes

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