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 D09: Nuclear Astrophysics II
9:00 AM–12:00 PM,
Wednesday, November 29, 2023
Hilton Waikoloa Village
Room: Kohala 2
Chair: Sharon Stephenson, DOE Nuclear Physics
Abstract: D09.00007 : The 17F(α, p)20Ne Reaction Rate in Type I X-Ray Bursts from the Inverse Reaction*
10:30 AM–10:45 AM
Presenter:
William Braverman
(Louisiana State University)
Authors:
William Braverman
(Louisiana State University)
Jeffery C Blackmon
(Louisiana State University)
Catherine M Deibel
(Louisiana State University)
Gemma L Wilson
(Louisiana State University)
Sudarsan Balakrishnan
(Rutgers University)
Khang H Pham
(Louisiana State University)
Zachary M Purcell
(Louisiana State University)
Melina Avila
(Argonne National Laboratory)
Ernst Rehm
(Argonne National Laboratory)
Lauren K Callahan
(University of Notre Dame)
Thomas L Bailey
(Notre Dame Physics)
Ingo L Wiedenhover
(Florida State University)
Lagy T Baby
(Florida State University)
Michael Paul
(Hebrew University)
Heshani Jayatissa
(Los Alamos National Laboratory)
breakout from the hot-CNO cycle that can be important in some X-ray burst
scenarios. We have previously measured the 20Ne(p, α)17F cross section at low
center-of-mass energies ranging from 4.80 to 7.60 MeV via activation
measurements with a proton beam on a 20Ne gas cell at the Fox Accelerator
Laboratory at Florida State University. We subsequently measured the same
reaction through inverse kinematics with a 20Ne beam on a methylene target
at Argonne National Lab’s ATLAS facility. We used an annular Si strip
detector for alpha-particle detection with recoiling heavy ions detected in the
Enge spectrograph by the MONICA focal plane detector. Studying the
reaction in inverse kinematics allows us to distinguish alpha particles emitted
to the first-excited state of 17F which do not contribute to the reverse (α, p)
reaction on the 17F ground state. Cross section comparisons and preliminary
results from an R-matrix analysis constraining properties of states in 21Na will
be presented.
*Work supported by U.S. Dept of Energy via Award DE-FG02-96ER40978,National Science Foundation via Award NSF-PHY 2012522, and by theLouisiana Board of Regents.This research used resources of ANL’s ATLAS facility, which is a DOE Officeof Science User Facility
Follow Us |
Engage
Become an APS Member |
My APS
Renew Membership |
Information for |
About APSThe American Physical Society (APS) is a non-profit membership organization working to advance the knowledge of physics. |
© 2025 American Physical Society
| All rights reserved | Terms of Use
| Contact Us
Headquarters
1 Physics Ellipse, College Park, MD 20740-3844
(301) 209-3200
Editorial Office
100 Motor Pkwy, Suite 110, Hauppauge, NY 11788
(631) 591-4000
Office of Public Affairs
529 14th St NW, Suite 1050, Washington, D.C. 20045-2001
(202) 662-8700