Bulletin of the American Physical Society
Fall 2022 Meeting of the APS Division of Nuclear Physics
Volume 67, Number 17
Thursday–Sunday, October 27–30, 2022; Time Zone: Central Daylight Time, USA; New Orleans, Louisiana
Session JE: Nuclear Astrophysics IV
8:30 AM–10:30 AM,
Saturday, October 29, 2022
Hyatt Regency Hotel
Room: Celestin C
Chair: Ruchi Garg, Michigan State University
Abstract: JE.00003 : The 17F(α, p)20Ne Reaction Rate in Type 1 X-Ray Bursts from the Inverse Reaction*
8:54 AM–9:06 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
(Louisiana State University)
Khang H Pham
(Louisiana State University)
Zachary M Purcell
(Louisiana State University)
Melina Avila
(Argonne National Laboratory)
Heshani Jayatissa
(Argonne National Laboratory)
Ernst Rehm
(Argonne National Laboratory)
Lauren K Callahan
(University of Notre Dame)
Thomas L Bailey
(Notre Dame Physics)
Ingo L Wiedenhoever
(Florida State University)
Lagy T Baby
(Florida State University)
Michael Paul
(Hebrew University)
Collaborations:
LSU, FSU, ANL, Notre Dame, Hebrew University
breakout from the hot-CNO cycle that can be important in some X-ray burst
scenarios. We have measured the 20Ne(p, α)17F cross section at low energies
ranging from 4.80 to 7.60 MeV using a proton beam on a neon gas cell with an
activation method and NaI detectors at the Fox Accelerator Laboratory at
Florida State University. Later, we measured the same reaction through
inverse kinematics with a 20Ne beam on a methylene target at the ATLAS
facility at Argonne National Laboratory. We used an annular Si strip detector for alpha
detection with recoiling heavy ions detected in the Enge spectrograph by the
MONICA focal plane detector. Studying the inverse kinematics reaction
allows us to distinguish alpha particles being emitted either to the ground or
first excited state of 17F. Cross sections will be compared to previous work,
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-FG02-96ER40978This 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. |
© 2024 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