New experimental study of low-energy (p,γ) resonances in magnesium isotopes
Creators
- Limata, B.1
- Imbriani, G.1
- DiLeva, A.1
- Roca, V.1
- Strieder, F.2
- Best, A.2
- Rolfs, C.2
- Trautvetter, H.-P.2
- Formicola, A.3
- Junker, M.3
- Gustavino, C.3
- Salvo, C.3
- Becker, H. W.4
- Bemmerer, D.5
- Marta, M.5
- Bonetti, R.6
- Broggini, C.7
- Menegazzo, R.7
- Rossi Alvarez, C.7
- Caciolli, A.8, 7
- and others
- LUNA Collaboration
- 1. Dipartimento di Scienze Fisiche, Universita di Napoli 'Federico II', and INFN Sezione di Napoli, I-80126 Napoli (Italy)
- 2. Institut fuer Experimentalphysik, Ruhr-Universitaet Bochum, D-44780 Bochum (Germany)
- 3. INFN, Laboratori Nazionali del Gran Sasso (LNGS), I-67010 Assergi (Italy)
- 4. Fakultaet fuer Physik und Astronomie, Ruhr-Universitaet Bochum, D-44780 Bochum (Germany)
- 5. Forschungszentrum Dresden Rossendorf, Bautzner Landstr. 128, D-01328 Dresden (Germany)
- 6. Istituto di Fisica Generale Applicata, Universita degli Studi di Milano and INFN Sezione di Milano, I-20133 Milano (Italy)
- 7. Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Padova, via Marzolo 8, I-35131 Padova (Italy)
- 8. Dipartimento di Fisica, Universita di Padova, I-35122 Padova (Italy)
Description
Proton captures on Mg isotopes play an important role in the Mg-Al cycle active in stellar H-shell burning. In particular, the strengths of low-energy resonances with E<200 keV in 25Mg(p,γ)26Al determine the production of 26Al and a precise knowledge of these nuclear data is highly desirable. Absolute measurements at such low energies are often very difficult and hampered by γ-ray background as well as changing target stoichiometry during the measurements. The latter problem can be partly avoided using higher-energy resonances of the same reaction as a normalization reference. Hence the parameters of suitable resonances have to be studied with adequate precision. In the present work we report on new measurements of the resonance strengths ωγ of the E=214, 304, and 326 keV resonances in the reactions 24Mg(p,γ)25Al, 25Mg(p,γ)26Al, and 26Mg(p,γ)27Al, respectively. These studies were performed at the LUNA facility in the Gran Sasso underground laboratory using multiple experimental techniques and provided results with a higher accuracy than previously achieved.
Additional details
Identifiers
- DOI
- 10.1103/PhysRevC.82.015801;
- arXiv
- arXiv:1006.5281v1;
Publishing Information
- Journal Title
- Physical Review. C, Nuclear Physics
- Journal Volume
- 82
- Journal Issue
- 1
- Journal Page Range
- p. 015801-015801.14
- ISSN
- 0556-2813
- CODEN
- PRVCAN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 41117972
- Subject category
- S73: NUCLEAR PHYSICS AND RADIATION PHYSICS;
- Descriptors DEI
- ALUMINIUM 25; ALUMINIUM 26; ALUMINIUM 27; CAPTURE; GAMMA DECAY; GAMMA RADIATION; HYDROGEN BURNING; ION-ATOM COLLISIONS; KEV RANGE 100-1000; MAGNESIUM 24 TARGET; MAGNESIUM 25 TARGET; MAGNESIUM 26 TARGET; PROTON REACTIONS; PROTONS; RESONANCE; STOICHIOMETRY; UNDERGROUND
- Descriptors DEC
- ALUMINIUM ISOTOPES; ATOM COLLISIONS; BARYON REACTIONS; BARYONS; BETA DECAY RADIOISOTOPES; BETA-PLUS DECAY RADIOISOTOPES; CHARGED-PARTICLE REACTIONS; COLLISIONS; DECAY; ELECTROMAGNETIC RADIATION; ELEMENTARY PARTICLES; ENERGY RANGE; FERMIONS; HADRON REACTIONS; HADRONS; ION COLLISIONS; IONIZING RADIATIONS; ISOTOPES; KEV RANGE; LEVELS; LIGHT NUCLEI; NUCLEAR DECAY; NUCLEAR REACTIONS; NUCLEI; NUCLEON REACTIONS; NUCLEONS; ODD-EVEN NUCLEI; ODD-ODD NUCLEI; RADIATIONS; RADIOISOTOPES; SECONDS LIVING RADIOISOTOPES; STABLE ISOTOPES; STAR BURNING; TARGETS; YEARS LIVING RADIOISOTOPES
Optional Information
- Notes
- (c) 2010 The American Physical Society
- Collaborations
- LUNA Collaboration