Supernova explosions of massive stars and cosmic rays

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F18%3A00547197" target="_blank" >RIV/68378271:_____/18:00547197 - isvavai.cz</a>
Result on the web
<a href="https://doi.org/10.1016/j.asr.2018.03.028" target="_blank" >https://doi.org/10.1016/j.asr.2018.03.028</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1016/j.asr.2018.03.028" target="_blank" >10.1016/j.asr.2018.03.028</a>

Result language
angličtina
Original language name
Supernova explosions of massive stars and cosmic rays
Original language description
Most cosmic ray particles observed derive from the explosions of massive stars. Massive stars from slightly above about 10 Me explode as supernovae via a mechanism which we do not know yet: two not mutually exclusive main ideas are an explosion driven by neutrinos, or the magneto-rotational mechanism, in which the magnetic field acts like a conveyor-belt to transport energy outwards for an explosion. Massive stars above about 25 M-circle dot, depending on their heavy element abundance, commonly produce stellar black holes in their supernova explosions. When two such black holes find themselves in a tight binary system they finally merge in a gigantic emission of gravitational waves, events that have now been detected.
Czech name
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Czech description
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Type
J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database
CEP classification
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OECD FORD branch
10303 - Particles and field physics

Publication year
2018
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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