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Supernovae are Nature's high-energy, high density laboratory experiments,reaching densities in excess of nuclear densities and temperatures above 10MeV.Astronomers have built up a suite of diagnostics to study these supernovae. Ifwe can utilize these diagnostics, and tie them together with a theoreticalunderstanding of supernova physics, we can use these cosmic explosions to studythe nature of matter at these extreme densities and temperatures. Capitalizingon these diagnostics will require understanding a wide range of additionalphysics. Here we review the diagnostics and the physics needed to use them tolearn about the supernova engine, and ultimate nuclear physics.

Observational Constraints of Stellar Collapse: Diagnostic Probes of Nature's Extreme Matter Experiment