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Volumn 60, Issue 7, 1999, Pages

Is there a 4.5 PeV neutron line in the cosmic ray spectrum?

Author keywords

[No Author keywords available]

Indexed keywords


EID: 18044375446     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.60.073005     Document Type: Article
Times cited : (14)

References (33)
  • 11
    • 85037180151 scopus 로고    scopus 로고
    • Were it not for the assumption that the neutron mean decay length greatly exceeds that of protons, the magnetic deflection of protons would eliminate directional correlations, and make the detection of neutrons based on their directionality highly problemmatic for all but nearby sources
    • Were it not for the assumption that the neutron mean decay length greatly exceeds that of protons, the magnetic deflection of protons would eliminate directional correlations, and make the detection of neutrons based on their directionality highly problemmatic for all but nearby sources.
  • 21
    • 85037246030 scopus 로고    scopus 로고
    • N. Hayashida et al., Proceedings of the International Conference on Cosmic Rays, Paris, 1981, pages XG 1.1-4
    • N. Hayashida et al., Proceedings of the International Conference on Cosmic Rays, Paris, 1981, pages XG 1.1-4.
  • 25
    • 85037192050 scopus 로고    scopus 로고
    • Jeremy Lloyd-Evans (private communication)
    • Jeremy Lloyd-Evans (private communication).
  • 33
    • 85037184581 scopus 로고    scopus 로고
    • Informal communications with AKENO Collaboration, M. Nagano (private communication);, Fly’s Eye Collaboration, Paul Sommers (private communication)
    • Informal communications with AKENO Collaboration, M. Nagano (private communication);Fly’s Eye Collaboration, Paul Sommers (private communication).


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.