Level structure of22Mg: Implications for the22Na(p, γ)22Mg astrophysical reaction rate and for the22Mg mass

Physical Review Letters

Volumn 94, Issue 3, 2005, Pages

  Seweryniak, D ^a   Woods, P J ^b   Carpenter, M P ^a   Davinson, T ^b   Janssens, R V F ^a   Jenkins, D G ^c   Lauritsen, T ^a   Lister, C J ^a   Ruiz, C ^d   Shergur, J ^a,e   Sinha, S ^a   Woehr, A ^f  

^a ARGONNE NATIONAL LABORATORY   (United States)

^b UNIVERSITY OF EDINBURGH   (United Kingdom)

^c UNIVERSITY OF YORK   (United Kingdom)

^d SIMON FRASER UNIVERSITY   (Canada)

^e UNIVERSITY OF MARYLAND   (United States)

^f UNIVERSITY OF NOTRE DAME   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

CONSERVED VECTOR CURRENT (CVC); LEVEL STRUCTURE; NUCLEAR SHELL MODEL; PROTON THERSHOLD;

ASTROPHYSICS; ELECTRIC EXCITATION; GAMMA RAYS; MAGNESIUM PRINTING PLATES; PROTONS; REACTION KINETICS;

SODIUM;

EID: 18044382126     PISSN: 00319007     EISSN: 10797114     Source Type: Journal    
DOI: 10.1103/PhysRevLett.94.032501     Document Type: Article

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