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Volumn 593, Issue 1-4, 2004, Pages 42-47

Galactic point sources of TeV antineutrinos

Author keywords

13.85.Tp; 95.30.Cq; 95.85.Ry

Indexed keywords

ARTICLE; COSMIC RADIATION; COSMOS; ENERGY; FLIGHT; NEUTRON; TIME;

EID: 3242696735     PISSN: 03702693     EISSN: None     Source Type: Journal    
DOI: 10.1016/j.physletb.2004.04.054     Document Type: Article
Times cited : (117)

References (36)
  • 1
    • 0033130341 scopus 로고    scopus 로고
    • Hayashida N., et al. AGASA Collaboration. Astropart. Phys. 10:1999;303 astro-ph/9807045
    • (1999) Astropart. Phys. , vol.10 , pp. 303
    • Hayashida, N.1
  • 2
    • 0001062907 scopus 로고    scopus 로고
    • Proc. 27th International Cosmic Ray Conference
    • Teshima M., et al. Copernicus Gesellschaft. Proc. 27th International Cosmic Ray Conference :2001;341
    • (2001) Copernicus Gesellschaft , pp. 341
    • Teshima, M.1
  • 6
    • 0242467152 scopus 로고    scopus 로고
    • Butt Y., et al. Astrophys. J. 597:2003;494 astro-ph/0302342
    • (2003) Astrophys. J. , vol.597 , pp. 494
    • Butt, Y.1
  • 11
    • 3242737010 scopus 로고    scopus 로고
    • IceCube is the neutrino telescope under construction at the South Pole
    • IceCube is the neutrino telescope under construction at the South Pole http://icecube.wisc.edu/
  • 12
    • 4243270502 scopus 로고
    • The GZK or "cosmogenic" neutrinos are created as secondaries from the decay of charged pions produced in collisions between ultrahigh energy nucleons and the cosmic microwave background
    • The GZK or "cosmogenic" neutrinos are created as secondaries from the decay of charged pions produced in collisions between ultrahigh energy nucleons and the cosmic microwave background Greisen K. Phys. Rev. Lett. 16:1966;748
    • (1966) Phys. Rev. Lett. , vol.16 , pp. 748
    • Greisen, K.1
  • 15
    • 85037913743 scopus 로고    scopus 로고
    • For an update on GZK neutrinos, see e.g.
    • For an update on GZK neutrinos, see e.g. Engel R., Seckel D., Stanev T. Phys. Rev. D. 64:2001;093010 astro-ph/0101216
    • (2001) Phys. Rev. D , vol.64 , pp. 093010
    • Engel, R.1    Seckel, D.2    Stanev, T.3
  • 21
  • 28
    • 5444234270 scopus 로고    scopus 로고
    • Ahrens J. AMANDA Collaboration. Phys. Rev. Lett. 92:2004;071102 astro-ph/0309585
    • (2004) Phys. Rev. Lett. , vol.92 , pp. 071102
    • Ahrens, J.1
  • 33
    • 25344472407 scopus 로고    scopus 로고
    • CASA-MIA Collaboration
    • Borione A., et al. CASA-MIA Collaboration. Phys. Rev. D. 55:1997;1714 astro-ph/9611117
    • (1997) Phys. Rev. D , vol.55 , pp. 1714
    • Borione, A.1
  • 36
    • 3242661255 scopus 로고    scopus 로고
    • Clay R.W., et al. astro-ph/0308494
    • Clay, R.W.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.