An analytical model for core-bounce gravitational waveforms estimates the rotation parameter β with 94% average fitting factor to numerical templates and derives error bounds below 0.1 via matched filtering and Cramér-Rao comparison in O4 noise at 5-50 kpc distances.
Asymmetric core collapse of rapidly rotating massive star
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
gr-qc 1years
2026 1verdicts
UNVERDICTED 1representative citing papers
citing papers explorer
-
Quantification of the parameter estimation error from Rotating Core Collapse supernovae
An analytical model for core-bounce gravitational waveforms estimates the rotation parameter β with 94% average fitting factor to numerical templates and derives error bounds below 0.1 via matched filtering and Cramér-Rao comparison in O4 noise at 5-50 kpc distances.