High-energy cosmic rays and neutrinos from semirelativistic hypernovae

Physical Review D - Particles, Fields, Gravitation and Cosmology

Volumn 76, Issue 8, 2007, Pages

  Wang, Xiang Yu ^a,b   Razzaque, Soebur ^a   Mészáros, Peter ^a   Dai, Zi Gao ^b  

^a PENNSYLVANIA STATE UNIVERSITY   (United States)

^b NANJING UNIVERSITY   (China)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 35548979381     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.76.083009     Document Type: Article

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72. A low-metallicity host galaxy requirement for hypernovae is not yet firmly established; without this requirement, galactic hypernovae might also be potential high-energy CR sources, if the galactic rate and the CR containment time are sufficiently large.