Supernova explosions of massive stars and cosmic rays

Kód výsledku v 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>

Výsledek na webu

<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>

Jazyk výsledku

angličtina

Název v původním jazyce

Supernova explosions of massive stars and cosmic rays

Popis výsledku v původním jazyce

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.

Název v anglickém jazyce

Supernova explosions of massive stars and cosmic rays

Popis výsledku anglicky

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.

Druh

J_imp - Článek v periodiku v databázi Web of Science

CEP obor

—

OECD FORD obor

10303 - Particles and field physics

Projekt

—

Návaznosti

—

Rok uplatnění

2018

Kód důvěrnosti údajů

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Název periodika

Advances in Space Research

ISSN

0273-1177

e-ISSN

1879-1948

Svazek periodika

62

Číslo periodika v rámci svazku

10

Stát vydavatele periodika

GB - Spojené království Velké Británie a Severního Irska

Počet stran výsledku

44

Strana od-do

2773-2816

Kód UT WoS článku

000449448700005

EID výsledku v databázi Scopus

2-s2.0-85053694057