Computer Science – Performance
Scientific paper
Mar 2012
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012aps..aprh11004k&link_type=abstract
American Physical Society, APS April Meeting 2012, March 31-Apr 3, 2012, abstract #H11.004
Computer Science
Performance
Scientific paper
Studies of rp-process nucleosynthesis in stellar explosions show that establishing the lowest l=0 and l=1 resonances is the most important step to determine reaction rates in the astrophysical rp--process path. At the resolut facility, we have used the (d,n) reaction to populate the lowest p-- resonances in ^26Si, and demonstrated the usefulness of this approach to populate the resonances of astrophysical interest [1]. In order to establish the (d,n) reaction as a standard technique for the spectroscopy of astrophysical resonances, we have developed a compact setup of low-energy Neutron-detectors, resoneut and tested it with the stable beam reaction ^12C(d,n)^13N in inverse kinematics. Performance data from this test-experiment and future plans for this setup will be presented. [4pt] [1] P.N. Peplowski et al. Phys.Rev.C 79, 032801 (2009)
Baby Lagy T.
Baker Jessica
Ebong Imeh
Gay Dennis
Kuvin Sean
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