The reaction rate for {sup 31}S(p,{gamma}){sup 32}Cl and its influence on the SiP-cycle in hot stellar hydrogen burning

Journal Article · Sun Feb 05 04:00:00 EST 1995 · AIP Conference Proceedings

DOI:https://doi.org/10.1063/1.47409· OSTI ID:165227

Vouzoukas, S; Browne, C P; Goerres, J; Herndl, H; Iliadis, C; Meissner, J; Ross, J G; van Wormer, L; Wiescher, M ^[1]; Lefebvre, A; Aguer, P; Coc, A; Thibaud, J P ^[2]

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1. University of Notre Dame, Department of Physics, Notre Dame, Indiana 46556 (United States)
2. Centre de Spectrometrie Nucleaire et de Sprectrometrie de Masse, Orsay 91405 (France)

The {sup 31}S(p, {gamma}){sup 32}Cl reaction rate has been measured for {sup 3}He energies between 22.5 and 25 MeV at forward angles. Excitation energies and spin-parities of the observed levels in {sup 32}Cl are derived. These data are used to calculate flow patterns of nuclear reactions in the mass range A=22--26 for temperatures and densities of astrophysical interest. (AIP) {copyright} {ital 1995} {ital American} {ital Institute} {ital of} {ital Physics}. {copyright} {ital 1995} {ital American} {ital Institute} {ital of} {ital Physics}.

• Sponsoring Organization: USDOE
• OSTI ID: 165227
• Report Number(s): CONF-9407131--
• Journal Information: AIP Conference Proceedings, Journal Name: AIP Conference Proceedings Journal Issue: 1 Vol. 327; ISSN 0094-243X; ISSN APCPCS
• Country of Publication: United States
• Language: English

Related Subjects

66 PHYSICS
CAPTURE
CHLORINE 32
EXCITED STATES
HYDROGEN BURNING
MEV RANGE 10-100
NUCLEAR REACTION KINETICS
PROTON REACTIONS
SULFUR 31
TEMPERATURE DEPENDENCE