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DOE OSTI · 2484102

The Core-collapse Supernova Sensitivity Machine (Final Technical Report)

Couch, Sean M. [Michigan State Univ., East Lansing, MI (United States)] (ORCID:0000000250805996)
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Abstract

Core-collapse supernovae are vital phenomena for understanding the extreme physics of stellar evolution, nuclear interactions, and the origins of elements in the universe. This project developed high-resolution 3D simulations and innovative 1D turbulence models to study the explosion mechanisms, yielding critical insights into the role of turbulence, magnetohydrodynamics, and neutrino physics. The outcomes include enhanced sensitivity analyses connecting nuclear physics inputs to observable supernovae characteristics, tools for the broader research community, and substantial contributions to the training of future scientists.

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79 ASTRONOMY AND ASTROPHYSICSCore-collapse supernovaemagnetohydrodynamicsneutrino physicsnuclear astrophysicssensitivity studiesturbulence

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Couch, Sean M. [Michigan State Univ., East Lansing, MI (United States)] (ORCID:0000000250805996). 2024-12-31. The Core-collapse Supernova Sensitivity Machine (Final Technical Report). https://doi.org/10.2172/2484102

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