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Volumn 90, Issue 13, 2003, Pages

Does the sun shine by p p or CNO fusion reactions?

Author keywords

[No Author keywords available]

Indexed keywords

ELECTRON SCATTERING; ELECTRONIC STRUCTURE; FUSION REACTIONS; LUMINESCENCE; MATHEMATICAL MODELS; SUN;

EID: 0037502768     PISSN: 00319007     EISSN: None     Source Type: Journal    
DOI: None     Document Type: Article
Times cited : (23)

References (51)
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    • KamLAND Collaboration
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    • (2003) Phys. Rev. Lett. , vol.90 , pp. 021802
    • Eguchi, K.1
  • 44
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    • (for the Super-Kamiokande Collaboration), hep-ex/0208004
    • M. B. Smy (for the Super-Kamiokande Collaboration), hep-ex/0208004.
    • Smy, M.B.1
  • 48
    • 0038525089 scopus 로고    scopus 로고
    • hep-ph/0210359 (to be published)
    • M. C. Gonzalez-Garcia, hep-ph/0210359 (to be published).
    • Gonzalez-Garcia, M.C.1
  • 49
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    • Borexino Collaboration
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    • (2002) Astropart. Phys. , vol.16 , pp. 205
    • Alimonti, G.1
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    • edited by Y. Suzuki, M. Nakahata, and S. Moriyama (World Scientific, River Edge, NJ)
    • Low Energy Solar Neutrino Detection (LowNu2), edited by Y. Suzuki, M. Nakahata, and S. Moriyama (World Scientific, River Edge, NJ, 2001)
    • (2001) Low Energy Solar Neutrino Detection (LowNu2)


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.