High-precision (p, t) Reactions to Determine Reaction Rates in the Stellar rp-process

Details High-precision (p, t) Reactions to Determine Reaction Rates in the Stellar rp-process High-precision (p, t) Reactions to Determine Reaction Rates in the Stellar rp-process

Aug 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1269..460b&link_type=abstract

THE 10TH INTERNATIONAL SYMPOSIUM ON ORIGIN OF MATTER AND EVOLUTION OF GALAXIES: OMEG-2010. AIP Conference Proceedings, Volume 1

Other

Stellar Evolution, White Dwarfs, Neutron Stars, Isotopes, Black Holes, Faint Blue Stars, White Dwarfs, Degenerate Stars, Nuclei Of Planetary Nebulae, Neutron Stars, Origin, Formation, And Abundances Of The Elements

Scientific paper

The main source of uncertainties in stellar rate calculations of the rp-process and the competing αp-process is often the lack of knowledge of the resonance states above the p- and α-thresholds and their precise energies. We have started a program to study these resonances in proton-rich unstable nuclei via the (p, t) and other neutron-pickup reactions using the high resolution spectrometer Grand Raiden. Here, we are presenting the status of the project and recent results of the 25Al(P, γ) reaction rates based on the analysis of measured 28Si(p, t)26Si spectra.

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