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Project Title:  Quantum Multiple Scattering Model of Heavy Ion Fragmentation (QMSFRG) Reduce
Fiscal Year: FY 2008 
Division: Human Research 
Research Discipline/Element:
HRP SR:Space Radiation
Start Date: 09/01/2008  
End Date: 08/31/2010  
Task Last Updated: 12/03/2009 
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Principal Investigator/Affiliation:   Cucinotta, Francis A Ph.D. / University of Nevada, Las Vegas 
Address:  Health Physics & Diagnostic Sciences / BHS-345 
4505 Maryland Parkway 
Las Vegas , NV 89154-3037 
Email: not available 
Phone: (702) 895-4320  
Congressional District:
Organization Type: NASA CENTER 
Organization Name: University of Nevada, Las Vegas 
Joint Agency:  
Comments: Formerly at NASA Johnson Space Center, until summer 2013 (Ed., Oct 2013) 
Saganti, Prem  Prairie View A&M 
Kim, Myung-Hee  Wyle Laboratories 
Project Information: Grant/Contract No. NNX07AT25A 
Responsible Center: NASA JSC 
Grant Monitor: Cucinott1a, Francis  
Center Contact: 281-483-0968 
Solicitation / Funding Source: Directed Research 
Grant/Contract No.: NNX07AT25A 
Project Type: GROUND 
Flight Program:  
TechPort: Yes 
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Human Research Program Elements: (1) SR:Space Radiation
Human Research Program Risks: (1) Cancer:Risk of Radiation Carcinogenesis
Human Research Program Gaps: (1) Cancer11:What are the most effective shielding approaches to mitigate cancer risks?
(2) Cancer12:What quantitative models, numerical methods, and experimental data are needed to accurately describe the primary space radiation environment and transport through spacecraft materials and tissue to evaluate dose composition in critical organs for mission relevant radiation environments (ISS, Free-space, Lunar, or Mars)? (IRP Rev F)
Task Description: The quantum multiple scattering model of heavy ion fragmentation (QMSFRG) is an important input to risk evaluation and radiation shielding calculations. Several areas of development in nuclear data base development and output deliverables with the QMSFRG model will be the focus of this directed research as guided by previous results.

Applications include biophysical models of biological damage as ions passed through complex tissue structures (Ponomarev and Cucinotta, 2006), radiation transport code applications (Wilson et al, 1991) including shielding evaluations (Cucinotta et al., 2006), and in comparisons of models to flight experiments (Badhwar and Cucinotta, 2000; Cucinotta et al., 2000), and space radiation risk assessments (Cucinotta et al., 2001). It is important to note that although measurements of nuclear fragmentation cross sections are a step in code development for biophysical, shielding, and risk analysis, only theoretical models can provide a complete data base for such studies.

Past nuclear fragmentation models have relied on parameterizations of experiments or semi-classical physics models. These approaches have been shown to fail badly in heavy ion radiation transport code comparisons to experiments (Wilson et al., 1986). Typical fragmentation measurements do not measure all secondary products and are usually restricted to fragments from ZP-1 to ZP/2 where ZP is the projectile charge. Lower charged fragments make important contributions to the galactic cosmic ray (GCR) transport. Parametric models include no underlying physical description and thus fail outside the range of measurements. This failure is amplified when one considers the large number of projectiles, target, and energies of interest and the lack of measurements for most of these reaction partners. Important aspects of nuclear reactions are not reproduced in Monte-Carlo models of heavy ion reactions and indicate the need for a quantum description that is capable of being implemented for GCR data bases. This features include the role of the nuclear surface, and nuclear structure effects such as shell structure and clustering. Our proposal will develop the quantum mechanical models of nuclear fragmentation based in multiple scattering theory (QMSFRG) that will substantially advance the nuclear data bases for space radiation transport applications and the ability to extrapolate away from existing experimental data sets.

The QMSFRG theory has been shown to be a robust and accurate approach to multiple types of galactic cosmic ray (GCR) computational evaluations. For the two-year period of performance we have the following Specific Aims:

Specific Aim 1: To develop Computer Subroutines from the QMSFRG model that will generate require cross section data for application within the high-charge-and energy (HZE) transport computer program (HZETRN) code in collaboration with Dr. John Wilson, NASA Langley Research Center (LaRC). A 190-ion grid for 9 projectile energies on arbitrary target materials (Hydrogen to Lead) applicable GCR shielding problems will be generated with appropriate interpolation schemes for other materials and energies. Furthermore, to prepare a data base generator for Monte-Carlo transport code applications (Dr. M.Y. Kim, Lead) and tested in the Geant4 code in collaboration with Dr. Maria Grazia Pia, INFN (Italian National Institute of Nuclear and Particle Physics), Genoa, Italy.

Specific Aim 2: To report on the extension of the light ion production cross sections in the QMSFRG model for nuclear coalescence formation of light particles (d, t, h, a), and the resulting losses to n and p production (Dr. F.A. Cucinotta, Lead). Also, data bases of light-particle production multiplicities will be generated. Comparisons to experimental data will be reported.

Specific Aim 3: To improve the model energy density formalisms used in the nuclear de-excitation process in QMSFRG Master decay-solutions (Dr. P. Saganti, Lead). Cross-comparisons of different models and to experimental data will be reported.

Specific Aim 4: To implement the NASA Johnson Space Center (JSC) Selected Core formalism for the description of pre-fragment excitation functions in nuclear abrasion for selected GCR nuclei (12C, 16O, 20Ne, and 28Si) and to extend the formalism for alpha-clusters (Dr. P. Saganti, Lead). Fragmentation cross section calculations will be compared to experimental data.

Future work will extend the quantum multiple scattering theory to explicit pion channels, to consider other light particle clusters, and to produce data bases of light and heavy particle energy spectra.

Research Impact/Earth Benefits:

Task Progress & Bibliography Information FY2008 
Task Progress: New project for FY2008.

Bibliography Type: Description: (Last Updated: 02/11/2021) 

Show Cumulative Bibliography Listing
 None in FY 2008