Constraint of the astrophysical Al 26g (p,γ) Si 27 destruction rate at stellar temperatures

Physical Review Letters

Volumn 114, Issue 21, 2015, Pages

  Pain, S D ^a   Bardayan, D W ^a,b   Blackmon, J C ^c   Brown, S M ^d   Chae, K Y ^e,f   Chipps, K A ^g   Cizewski, J A ^g   Jones, K L ^e   Kozub, R L ^h   Liang, J F ^a   Matei, C ⁱ   Matos, M ^c   Moazen, B H ^e   Nesaraja, C D ^a   Okolowicz J ^j   O'Malley, P D ^g   Peters, W A ⁱ   Pittman, S T ^e   Ploszajczak M ^k   Schmitt, K T ^e   Shriner, J F ^h   Shapira, D ^a   Smith, M S ^a   Stracener, D W ^a   Wilson, G L ^d   more..

^a OAK RIDGE NATIONAL LABORATORY   (United States)

^b UNIVERSITY OF NOTRE DAME   (United States)

^c LOUISIANA STATE UNIVERSITY   (United States)

^d UNIVERSITY OF SURREY   (United Kingdom)

^e UNIVERSITY OF TENNESSEE   (United States)

^f Sungkyunkwan University   (South Korea)

^g RUTGERS UNIVERSITY   (United States)

^h TENNESSEE TECHNOLOGICAL UNIVERSITY   (United States)

ⁱ OAK RIDGE ASSOCIATED UNIVERSITIES   (United States)

^j INSTITUTE OF NUCLEAR PHYSICS   (Poland)

^k DIF   (France)

more..

Author keywords

[No Author keywords available]

Indexed keywords

INVERSE KINEMATICS; RESONANCE; STARS;

DESTRUCTION RATES; GAMMA-RAY ASTRONOMY; MASSIVE STARS; MIRROR SYMMETRY; PROTON RESONANCES; RESONANCE STRENGTHS; SPECTROSCOPIC FACTORS; UPPER LIMITS;

GAMMA RAYS;

EID: 84931291843     PISSN: 00319007     EISSN: 10797114     Source Type: Journal    
DOI: 10.1103/PhysRevLett.114.212501     Document Type: Article

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