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Evidence for UHECR origin in starburst galaxies
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Evidence for UHECR origin in starburst galaxies
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The quest for the origin(s) of ultra-high-energy cosmic rays (UHECRs) continues to be a far-reaching pillar of high energy astrophysics. The source scrutiny is mostly based on three observables: the energy spectrum, the nuclear composition, and the distribution of arrival directions. We show that each of these three observables can be well reproduced with UHECRs originating in starburst galaxies.
Forward citations
Cited by 1 Pith paper
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The Galactic magnetic field in the light of starburst-generated ultrahigh-energy cosmic rays
Assuming starbursts source UHECRs, arrival directions (especially a TA hot spot from M82) can constrain Galactic magnetic field models.
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