Abstract
When a neutron star accretes hydrogen and helium from the outer layers of its companion star, thermonuclear burning enables the αp-process as a break out mechanism from the hot CNO cycle. Model calculations predict (α, p) reaction rates significantly affect both the light curves and elemental abundances in the burst ashes. The Jet Experiments in Nuclear Structure and Astrophysics (JENSA) gas jet target enables the direct measurement of previously inaccessible (α,p) reactions with radioactive beams provided by the rare isotope re-accelerator ReA3 at the National Superconducting Cyclotron Laboratory (NSCL), USA. JENSA is going to be the main target for the Recoil Separator for Capture Reactions (SECAR) at the Facility for Rare Isotope Beams (FRIB). Commissioning of JENSA and first experiments at Oak Ridge National Laboratory (ORNL) showed a highly localized, pure gas target with a density of ∼1019 atoms per square centimeter. Preliminary results are presented from the first direct cross section measurement of the 34Ar(α, p)37 K reaction at NSCL.
Original language | English |
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Title of host publication | Nuclear Physics in Astrophysics VIII, NPA8 2017 |
Editors | Marcello Lattuada, Rosario Gianluca Pizzone, Claudio Spitaleri, Marcello Lattuada, Marco La Cognata, Sara Palmerini, Claudio Spitaleri |
Publisher | EDP Sciences |
ISBN (Electronic) | 9782759890309 |
DOIs | |
State | Published - Dec 30 2017 |
Event | 8th International Conference on Nuclear Physics in Astrophysics, NPA8 2017 - Catania, Italy Duration: Jun 18 2017 → Jun 23 2017 |
Publication series
Name | EPJ Web of Conferences |
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Volume | 165 |
ISSN (Print) | 2101-6275 |
ISSN (Electronic) | 2100-014X |
Conference
Conference | 8th International Conference on Nuclear Physics in Astrophysics, NPA8 2017 |
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Country/Territory | Italy |
City | Catania |
Period | 06/18/17 → 06/23/17 |
Funding
This research is supported by the National Science Foundation in part under Grant No. PHY-1430152 (JINA Center for the Evolution of the Elements), Grant No. PHY-1419765, Grant No. PHY-1404218, by the U. S. Department of Energy (DoE), Office of Nuclear Physics and National Nuclear Security Administration, and by the Laboratory Directed Research and Development Program of Oak Ridge National Laboratory, managed by UT-Battelle, LLC, for DoE.
Funders | Funder number |
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UT-Battelle | |
National Science Foundation | 1713857, PHY-1419765, PHY-1404218 |
National Science Foundation | |
U.S. Department of Energy | |
Directorate for Mathematical and Physical Sciences | 1419765, 1404218, 1430152 |
Directorate for Mathematical and Physical Sciences | |
National Nuclear Security Administration | |
Oak Ridge National Laboratory | |
Laboratory Directed Research and Development |