LightGBM and other regressors achieve R^{2}≈0.6–0.7 under random CV on CCSN GW catalogues but collapse to worse-than-mean performance under Leave-One-EoS-Out validation, exposing a generalisation gap for unseen EoS families.
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2026 2representative citing papers
Collapse of a rotating 300 solar mass star produces a strong, characteristic deci-Hz gravitational wave signal potentially detectable to 200 Mpc at a rate of 0.5 per year.
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The Generalization Gap in Machine Learning EoS Inference from Core-Collapse Supernova Gravitational Waves
LightGBM and other regressors achieve R^{2}≈0.6–0.7 under random CV on CCSN GW catalogues but collapse to worse-than-mean performance under Leave-One-EoS-Out validation, exposing a generalisation gap for unseen EoS families.
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The deci-Hz gravitational wave signal from the collapse of rotating very massive stars
Collapse of a rotating 300 solar mass star produces a strong, characteristic deci-Hz gravitational wave signal potentially detectable to 200 Mpc at a rate of 0.5 per year.