The paper proposes that the curvature of the high-frequency gravitational-wave feature from core-collapse supernovae can serve as a distance-dependent diagnostic separating detector-noise uncertainty from intrinsic model variability.
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From the Early Slope to Curvature: Future Prospects and challenges for Astrophysical Parameter Estimation Using the Core-Collapse Supernova High-Frequency Feature
The paper proposes that the curvature of the high-frequency gravitational-wave feature from core-collapse supernovae can serve as a distance-dependent diagnostic separating detector-noise uncertainty from intrinsic model variability.