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Failed Experiment ReportOpen accessPhysics and Astronomy· cited by 9

Neutrino heating in 1D, 2D, and 3D core-collapse supernovae: characterizing the explosion of high-compactness stars

Luca Boccioli; David Vartanyan; Evan O’Connor; Daniel Kasen · 2025 · Monthly Notices of the Royal Astronomical Society

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Abstract

ABSTRACT Massive stars can end their lives with a successful supernova explosion (leaving behind a neutron star or, more rarely, a black hole), or a failed explosion that leaves behind a black hole. The density structure of the pre-collapse progenitor star already encodes much of the information regarding the outcome and properties of the explosion. However, the complexity of the collapse and subsequent shock expansion phases prevents drawing a straightforward connection between the pre-collapse and post-explosion properties. In order to derive such a connection several explodability studies h

Abstract by Luca Boccioli; David Vartanyan; Evan O’Connor; Daniel Kasen, Monthly Notices of the Royal Astronomical Society (2025) — licensed CC BY 4.0.

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Metadata source: OpenAlex · DOI 10.1093/mnras/staf963