Impact of active-sterile neutrino mixing on supernova explosion and nucleosynthesis

TL;DR

This paper investigates how active-sterile neutrino mixing affects supernova explosions and element formation, showing that such mixing can alter neutron-richness and neutrino heating, with implications for astrophysics and particle physics.

Contribution

It demonstrates that active-sterile neutrino mixing significantly impacts supernova nucleosynthesis and explosion dynamics, providing a new way to constrain neutrino properties.

Findings

Enhanced production of elements from Sr to Cd due to neutrino conversion.

Suppressed neutrino heating affecting shock revival.

Potential to constrain neutrino mixing parameters through supernova simulations.

Abstract

We show that for the active-sterile flavor mixing parameters suggested by the reactor neutrino anomaly, substantial \\nu_e-\\nu_s and \bar \\nu_e-\bar \\nu_s conversion occurs in regions with electron fraction of \approx 1/3 near the core of an 8.8 M_sun electron-capture supernova. Compared to the case without such conversion, the neutron-richness of the ejected material is enhanced to allow production of elements from Sr, Y, and Zr up to Cd in broad agreement with observations of the metal-poor star HD 122563. Active-sterile flavor conversion also strongly suppresses neutrino heating at times when it is important for the revival of the shock. Our results suggest that simulations of supernova explosion and nucleosynthesis may be used to constrain active-sterile mixing parameters in combination with neutrino experiments and cosmological considerations.