Empirical mapping between τ and progenitor-core structure metrics (compactness ξ_M and Ertl’s M4–μ4)

Calibrate an empirical mapping τ = f(ξ_M, M4, μ4) that links the spectral parameter τ derived from neutrino observations to pre-collapse progenitor metrics—compactness ξ_M and Ertl’s two-parameter criterion (M4, μ4)—by assembling a sample or simulations that jointly constrain these core metrics and post-explosion observables.

Background

The τ parameter is an observationally derived descriptor of the supernova neutrino spectrum that encodes aspects of the explosion’s energetics and transport efficiency. Theoretical progenitor metrics—compactness ξ_M and Ertl’s M4–μ4 criterion—quantify the pre-collapse core structure and are used to predict explodability and post-bounce dynamics.

The authors point out that their current dataset lacks objects with independently constrained ξ_M and (M4, μ4), and that quantitatively calibrating τ against these metrics would require matched samples or simulations. They explicitly defer this empirical mapping to future work, highlighting it as an unresolved task.

References

That said, our current dataset does not include objects with independently constrained $\xi_M$ or ($M_4, \mu_4$) parameters. A quantitative calibration of $\tau = f(\xi_M, M_4, \mu_4)$ would require a sample (or simulations) matching inferred progenitor core metrics with post-explosion observables. Therefore, we leave this direct empirical mapping for future work.

A Core-Collapse Supernova Neutrino Parameterization with Enhanced Physical Interpretability  (2511.16631 - Shi et al., 20 Nov 2025) in Discussion (Section 4)