Simulating Turbulence-aided Neutrino-driven Core-collapse Supernova Explosions in One Dimension [electronic resource]
The core-collapse supernova (CCSN) mechanism is fundamentally 3D, with instabilities, convection, and turbulence playing crucial roles in aiding neutrino-driven explosions. Simulations of CCNSe including accurate treatments of neutrino transport and sufficient resolution to capture key instabilities...
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Full Text (via OSTI) |
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| Format: | Government Document Electronic eBook |
| Language: | English |
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Washington, D.C. : Oak Ridge, Tenn. :
United States. Department of Energy. Office of Science ; Distributed by the Office of Scientific and Technical Information, U.S. Department of Energy,
2020.
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Internet
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| Call Number: |
E 1.99:1802777
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| E 1.99:1802777 | Available |