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Volumn 4858, Issue , 2002, Pages 191-198

Monte Carlo design studies for a next generation UHE neutrino observatory located in a large rock salt formation

Author keywords

[No Author keywords available]

Indexed keywords

COMPUTER SIMULATION; COSMIC RAYS; ELECTRIC FIELD EFFECTS; HIGH ENERGY PHYSICS; MONTE CARLO METHODS; OBSERVATORIES; PARTICLE DETECTORS;

EID: 0037515719     PISSN: 0277786X     EISSN: None     Source Type: Conference Proceeding    
DOI: 10.1117/12.458024     Document Type: Conference Paper
Times cited : (4)

References (28)
  • 3
    • 85037913743 scopus 로고    scopus 로고
    • R. Engel, D. Seckel, and T. Stanev, Phys. Rev. D 64, 093010 (2001) and references therein provides a recent comprehensive summary of GZK produced neutrinos.
    • (2001) Phys. Rev. D , vol.64 , pp. 093010
    • Engel, R.1    Seckel, D.2    Stanev, T.3
  • 4
    • 0038331462 scopus 로고    scopus 로고
    • Amanda Collaboration
    • Amanda Collaboration, Annalen Phys. 10 131 (2001).
    • (2001) Annalen Phys. , vol.10 , pp. 131
  • 5
    • 0037993607 scopus 로고    scopus 로고
    • Antares Collaboration, astro-ph/9907432
    • Antares Collaboration, astro-ph/9907432.
  • 6
    • 0037655810 scopus 로고    scopus 로고
    • ICECUBE collaboration, NSF proposal
    • ICECUBE collaboration, NSF proposal, http://icecube.wisc.edu
  • 25
    • 0037655801 scopus 로고    scopus 로고
    • UCLA-HEP-02-001
    • For a review of helical antennas see J. Becker, UCLA-HEP-02-001 (2002).
    • (2002)
    • Becker, J.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.