Ultra High Energy Cosmic Rays, radio galaxies

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F17%3A00551299" target="_blank" >RIV/68378271:_____/17:00551299 - isvavai.cz</a>
Result on the web
<a href="http://www.lnf.infn.it/sis/frascatiseries/Volume64/Volume64.pdf" target="_blank" >http://www.lnf.infn.it/sis/frascatiseries/Volume64/Volume64.pdf</a>
DOI - Digital Object Identifier
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Result language
angličtina
Original language name
Ultra High Energy Cosmic Rays, radio galaxies
Original language description
We outline two concepts to explain Ultra High Energy Cosmic Rays (UHECRs), one based on radio galaxies and their relativistic jets and terminal hot spots, and one based on relativistic Super-Novae (SNe) or Gamma Ray Bursts (GRBs) in starburst galaxies, one matching the arrival direction data in the South (the radio galaxy Cen A) and one in the North (the starburst galaxy M82). The most likely identification of the origin of observed Gravitational Wave (GW) events is stellar binary black hole (BH) mergers in starburst galaxies such as M82 with the highest rate of star formation, so the highest far-infrared (FIR) luminosity, at the edge of the universe visible in 10-300 Hz GWs at low heavy element abundance Z ch the formation of stellar BHs extends to a larger massrange.n
Czech name
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Czech description
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Publication year
2017
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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