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Volumn 61, Issue 12, 2000, Pages

High energy cosmic rays from neutrinos

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[No Author keywords available]

Indexed keywords


EID: 17144396365     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.61.123003     Document Type: Article
Times cited : (33)

References (29)
  • 9
    • 85037200760 scopus 로고    scopus 로고
    • astro-ph/9804023
    • E. Waxman, astro-ph/9804023.
    • Waxman, E.1
  • 16
    • 4243741631 scopus 로고    scopus 로고
    • Super-Kamiokande Collaboration, Y. Fukuda, Phys. Rev. Lett. 81, 1562 (1998)
    • (1998) Phys. Rev. Lett. , vol.81 , pp. 1562
    • Fukuda, Y.1
  • 22
    • 4243611047 scopus 로고    scopus 로고
    • At the same c.m. energy, (Formula presented) interaction can have a relevant cross section [see D. Seckel, Phys. Rev. Lett. 80, 900 (1998)], but due to the much lower (Formula presented) energy, the neutrino threshold energy is four orders of magnitude higher and can be neglected.
    • (1998) Phys. Rev. Lett. , vol.80 , pp. 900
    • Seckel, D.1
  • 28
    • 85037232086 scopus 로고    scopus 로고
    • The Pierre Auger Project Design Report, Auger Collaboration, Report No. FERMILAB-PUB-96-024, 1996
    • The Pierre Auger Project Design Report, Auger Collaboration, Report No. FERMILAB-PUB-96-024, 1996.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.