Bulletin of the American Physical Society
6th Joint Meeting of the APS Division of Nuclear Physics and the Physical Society of Japan
Sunday–Friday, November 26–December 1 2023; Hawaii, the Big Island
Session 3WPB: The Origin of the Heavy Elements II
11:00 AM–12:30 PM,
Monday, November 27, 2023
Hilton Waikoloa Village
Room: Kohala 4
Chair: Hendrik Schatz, Michigan State University
Abstract: 3WPB.00002 : Better understanding of nu-p process with experimentally determined 56Ni(n,p) reaction rate via direct measurements at LANSCE*
11:30 AM–12:00 PM
Presenter:
Hye Young Lee
(Los Alamos Natl Lab)
Authors:
Hye Young Lee
(Los Alamos Natl Lab)
Sean A Kuvin
(Los Alamos National Laboratory)
Hirokazu Sasaki
(Los Alamos National Laboratory)
Christian Vermeulen
(Los Alamos National Laboratory)
Veronika Mocko
(Los Alamos National Laboratory)
Panagiotis Gastis
(Los Alamos National Laboratory)
Toshihiko Kawano
(Los Alamos National Laboratory)
Shea Mosby
(Los Alamos Natl Lab)
Georgios Perdikakis
(Central Michigan University)
Pelagia Tsintari
(Central Michigan University)
Carla Frohlich
(North Carolina State University)
For reaching out radioactive isotopes relevant for the nu-p process, a new capability of producing radioactive isotopes at Isotope Production Facility and performing direct measurements for (n,p) and (n,a) reactions has been commissioned at Los Alamos Neutron Science Center. We studied the 56Ni(n,p) reaction, which has been identified as one of critical reactions for understanding heavy element productions in core-collapse supernovae. Using the hotLENZ (radioactive Low Energy NZ) instrument, the first directly measured cross sections of 56,59Ni(n,p), 56Co(n,p), and 59Ni(n,a) reactions were obtained for deducing reaction rates. Updated 56Ni(n,p) and 56Co(n,p) reaction rates are compared with the current rates from REACLIB (Cyburt 2010), and used for hydrodynamics calculations with the parameters from Wanajo et al. (2011) and Nishimura et al. (2019) along with our parameters. The summary of this effort will be discussed in terms of potential further constrains on the nu-p process. The optimized solenoidal spectrometer development for radioisotope reaction studies at LANSCE will be presented.
*This work benefits from the LANSCE accelerator facility and is supported by the U.S. Department of Energy under contracts DE-AC52-06NA25396, the Laboratory Directed Research and Development program of Los Alamos National Laboratory under project numbers 20130758ECR and 20180228ER, and the U.S. Department of Energy Office of Science-Nuclear Physics.
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