Beta-delayed proton decay of proton-rich nuclei 23Al and 31Cl and explosive H-burning in classical novae
L. Trache, A. Banu, J. C. Hardy, V. E. Iacob, M. McCleskey, E., Simmons, G. Tabacaru, R. E. Tribble, J. Aysto, A. Jokinen, A. Saastamoinen,, M. A. Bentley, D. Jenkins, T. Davinson, P. J. Woods, N. L. Achouri, B. Roeder

TL;DR
This paper introduces a new technique for measuring beta-delayed proton decay in proton-rich nuclei, enabling detailed study of isotopes relevant to explosive hydrogen burning in novae.
Contribution
The authors developed a novel method for detecting beta-delayed protons from short-lived radioactive nuclei, improving sensitivity and selectivity for astrophysical research.
Findings
Successfully measured beta-delayed proton decay of 23Al and 31Cl.
Demonstrated the technique's high selectivity and potential for low-rate radioactive beams.
Provided data relevant to nuclear processes in classical novae.
Abstract
We have developed a technique to measure beta-delayed proton decay of proton-rich nuclei produced and separated with the MARS recoil spectrometer of Texas A&M University. The short-lived radioactive species are produced in-flight, separated, then slowed down (from about 40 MeV/u) and implanted in the middle of very thin Si detectors. The beam is pulsed and beta-p decay of the pure sources collected in beam is measured between beam pulses. Implantation avoids the problems with detector windows and allows us to measure protons with energies as low as 200 keV from nuclei with lifetimes of 100 ms or less. Using this technique, we have studied the isotopes 23Al and 31Cl, both important for understanding explosive H-burning in novae. They were produced in the reactions 24Mg(p,2n)23Al and 32S(p,2n)31Cl, respectively, in inverse kinematics, from stable beams at 48 and 40 MeV/u, respectively. We…
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Taxonomy
TopicsNuclear physics research studies · Quantum Chromodynamics and Particle Interactions · Gamma-ray bursts and supernovae
