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Volumn 591, Issue 1-2, 2004, Pages 61-68

Astrophysical S-factor of 14N(p,γ)15O

(32)  Formicola, A a   Imbriani, G b   Costantini, H c   Angulo, C d   Bemmerer, D e   Bonetti, R f   Broggini, C g   Corvisiero, P c   Cruz, J h   Descouvemont, P i   Fulop Z j   Gervino, G k   Guglielmetti, A f   Gustavino, C l   Gyurky G j   Jesus, A P h   Junker, M l   Lemut, A c   Menegazzo, R g   Prati, P c   more..


Author keywords

24.30. v; 24.50.+g; 26.20.+f

Indexed keywords

ANALYTIC METHOD; ARTICLE; ATOMIC PARTICLE; MEASUREMENT; NEUTRINO; NUCLEAR PHYSICS; PHASE TRANSITION;

EID: 2942572934     PISSN: 03702693     EISSN: None     Source Type: Journal    
DOI: 10.1016/j.physletb.2004.03.092     Document Type: Article
Times cited : (367)

References (23)
  • 11
    • 2942594127 scopus 로고    scopus 로고
    • Thesis, University of Genova, to be published
    • H. Costantini, Thesis, University of Genova, 2003, to be published
    • (2003)
    • Costantini, H.1
  • 12
    • 2942564212 scopus 로고    scopus 로고
    • Thesis, Ruhr-Universität Bochum
    • A. Formicola, Thesis, Ruhr-Universität Bochum, 2004
    • (2004)
    • Formicola, A.1
  • 15
    • 2942562425 scopus 로고    scopus 로고
    • Geant4 Collaboration. http://www.info.cern.ch/asd/geant4/geant4.html
  • 21
    • 2942562424 scopus 로고    scopus 로고
    • Astron. Astrophys., in press
    • Imbriani G., et al. astro-ph/0403071. Astron. Astrophys., in press
    • Imbriani, G.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.