An Emerging Coherent Picture of Red Supergiant Supernova Explosions
Dovi Poznanski (Tel Aviv University)

TL;DR
This paper synthesizes observational data, models, and simulations to propose a unified understanding of how core collapse supernovae from red supergiants deposit energy into their ejecta, linking progenitor mass to explosion characteristics.
Contribution
It introduces a coherent framework connecting progenitor mass, explosion energy, and observable supernova features, advancing the understanding of supernova explosion mechanisms.
Findings
Energy in ejecta proportional to progenitor mass cubed
Correlation between light curve plateau duration and progenitor mass
Relationship between ejecta velocity and luminosity
Abstract
Three lines of evidence indicate that in the most common type of core collapse supernovae, the energy deposited in the ejecta by the exploding core is approximately proportional to the progenitor mass cubed. This results stems from an observed uniformity of light curve plateau duration, a correlation between mass and ejecta velocity, and the known correlation between luminosity and velocity. This result ties in analytical and numerical models together with observations, providing us with clues as to the mechanism via which the explosion of the core deposits a small fraction of its energy into the hurled envelope.
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