Very Low Energy Supernovae from Neutrino Mass Loss

TL;DR

This paper explores how the sudden loss of neutrino mass during core-collapse can cause very low energy supernovae, producing observable transients with distinct red, slow, and luminous characteristics.

Contribution

It provides a hydrodynamical analysis of low-energy supernovae triggered by neutrino mass loss, highlighting their potential observability and unique features.

Findings

Results show ejected mass of hydrogen envelope with speeds ~100 km/s.

Total kinetic energy of explosions is around 10^47 erg.

Events resemble luminous red novae but with lower velocities.

Abstract

The continuing difficulty of achieving a reliable explosion in simulations of core-collapse supernovae, especially for more massive stars, has led to speculation concerning the observable transients that might be produced if such a supernova fails. Even if a prompt outgoing shock fails to form in a collapsing presupernova star, one must still consider the hydrodynamic response of the star to the abrupt loss of mass via neutrinos as the core forms a protoneutron star. Following a suggestion by Nadezhin (1980), we calculate the hydrodynamical responses of typical supernova progenitor stars to the rapid loss of approximately 0.2 to 0.5 M_sun of gravitational mass from their centers. In a red supergiant star, a very weak supernova with total kinetic energy ~ 10^47 erg results. The binding energy of a large fraction of the hydrogen envelope before the explosion is of the same order and, depending upon assumptions regarding the neutrino loss rates, most of it is ejected. Ejection speeds are ~ 100 km/s and luminosities ~ 10^39 erg/s are maintained for about a year. A significant part of the energy comes from the recombination of hydrogen. The color of the explosion is extremely red and the events bear some similarity to "luminous red novae," but have much lower speeds.