Nucleosynthesis of proton-rich nuclei. Experimental results on the rp-process

Nucleosynthesis of proton-rich nuclei. Experimental results on the rp-process

We report in this study the nuclear properties of proton-rich isotopes located along the rp-process path. The experiments have recently been performed at the National Superconducting Cyclotron Laboratory (NSCL) at Michigan State University. The level properties above the proton separation energy of...

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Hauptverfasser: Galaviz, D, Amthor, A M, Bazin, D, Becerril, A D, Brown, B A, Chen, A A, Cole, A, Cook, J M, Elliot, T, Estrade, A, Fülöp, Z S, Gade, A, Glasmacher, T, Heger, A, Howard, M E, Kessler, R, Lorusso, G, Matos, M, Montes, F, Müller, W, Pereira, J, Schatz, H, Sherrill, B, Schertz, F, Shimbara, Y, Smith, E, Smith, K, Tamii, A, Stolz, A, Weisshaar, D, Wallace, M, Wiescher, M, Zegers, R G T
Format: Tagungsbericht
Sprache:eng
Schlagworte:
Astrophysics
Cyclotrons
Nuclear fusion
Nuclear properties
Nuclei
Physics
Protons
Sciences of the Universe
Solar and Stellar Astrophysics
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Beschreibung
Zusammenfassung:We report in this study the nuclear properties of proton-rich isotopes located along the rp-process path. The experiments have recently been performed at the National Superconducting Cyclotron Laboratory (NSCL) at Michigan State University. The level properties above the proton separation energy of the nuclei 30S, 36K and 37Ca were measured with precision of < 10 keV. This will allow a reduction in the determination of the astrophysical (p,γ) reaction rate under rp-process conditions.
ISSN:1742-6596
1742-6588
1742-6596
DOI:10.1088/1742-6596/202/1/012009