期刊
NATURE
卷 589, 期 7840, 页码 29-39出版社
NATURE RESEARCH
DOI: 10.1038/s41586-020-03059-w
关键词
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资金
- US Department of Energy (DOE) Office of Science
- US Department of Energy (DOE) Office of Advanced Scientific Computing Research via the Scientific Discovery through Advanced Computing (SciDAC4) programme
- US Department of Energy (DOE) Office of Advanced Scientific Computing Research via the Scientific Discovery [DE-SC0018297, 00009650]
- US NSF [AST-1714267, PHY-1804048]
- DOE Office of Science User Facility [DE-AC02-06CH11357]
- National Science Foundation [OCI-0725070, ACI-1238993]
- state of Illinois, under a PRAC allocation from the National Science Foundation [OAC-1809073]
- state of Illinois [TG-AST170045, ACI-1548562]
- Princeton Institute for Computational Science and Engineering (PICSciE)
- Princeton University Office of Information Technology
- DOE Office of Science [DE-AC03-76SF00098]
Supernova explosions result from the death of massive stars, giving birth to neutron stars and black holes while ejecting solar masses of heavy elements. The delayed neutrino-heating mechanism is emerging as the key driver, but there are still many issues to address, such as the chaotic dynamics involved.
Most supernova explosions accompany the death of a massive star. These explosions give birth to neutron stars and black holes, and eject solar masses of heavy elements. However, determining the mechanism of explosion has been a half-century journey of great numerical and physical complexity. Here we present the status of this theoretical quest and the physics and astrophysics upon which its resolution seems to depend. The delayed neutrino-heating mechanism is emerging as the key driver of supernova explosions, but there remain many issues to address, such as the chaos of the involved dynamics.
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