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NUCFRG3: Light ion Improvements to the Nuclear Fragmentation ModelLight ion improvements to the nuclear fragmentation model NUCFRG are reported. Improvements include the replacement of the simple light ion production model with a light ion coalescence model and an improved electromagnetic dissociation (EMD) formalism. Prior versions of the model provide reasonable overall agreement with measured data; however, those versions lack a physics-based description for coalescence and EMD. The NUCFRG3 model has improved theoretical descriptions of these mechanisms and offers additional benefits. Previous work established the improved EMD formalism to be more accurate than the predecessor. The predictive capability of NUCFRG has been improved and strengthened by the light ion physics-based changes. Based on increased capability and better theoretical grounding of NUCFRG3, it is recommended that it replace NUCFRG2 for space radiation assessments and other applications.
Document ID
20200005597
Acquisition Source
Langley Research Center
Document Type
Presentation
Authors
A Adamczyk
(University of Tennessee at Knoxville Knoxville, Tennessee, United States)
R Norman ORCID
(Langley Research Center Hampton, Virginia, United States)
S Sriprisan
(Prairie View A&M University Prairie View, Texas, United States)
L Townsend ORCID
(University of Tennessee at Knoxville Knoxville, Tennessee, United States)
J Norbury
(Langley Research Center Hampton, Virginia, United States)
S Blattnig
(Langley Research Center Hampton, Virginia, United States)
T Slaba ORCID
(Langley Research Center Hampton, Virginia, United States)
Date Acquired
May 13, 2020
Publication Date
October 29, 2011
Publication Information
Publication: Bulletin of the American Physical Society
Publisher: American Physical Society
Volume: 56
Issue: 12
ISSN: 0003-0503
Subject Category
Space Radiation
Report/Patent Number
NF1676L-13036
Meeting Information
Meeting: Fall Meeting of the APS Division of Nuclear Physics
Location: East Lansing, MI
Country: US
Start Date: October 26, 2011
End Date: October 29, 2011
Sponsors: American Physical Society
Funding Number(s)
WBS: 651549.02.07.01
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
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