2017
DOI: 10.1166/jap.2017.1283
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(n, p) Reaction Cross Sections Calculations of Some Stellar Iron Group Fusion Materials

Abstract: The excitation functions for (n, p) reactions from reaction threshold to 24 MeV on some important iron (Fe) group target elements (20 ≤ Z ≤ 28) for astrophysical (n, p) reactions such as Si, Ca, Sc, Ti, Cr, Fe, Co and Ni were calculated using TALYS-1.0 nuclear model code. The new calculations on the excitation functions of 28Si(n, p)28Al, 29Si(n, p)29Al, 42Ca(n, p) Show more

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Cited by 5 publications
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“…(1). When looping over all possible residual configurations, the multiple preequilibrium contribution is obtained [7][8][9][10][11][12][13][14][15][16][17][18][19][20]. In TALYS, multiple preequilibrium emission is followed up to arbitrary order; though for 96 MeV, only the secondary preequilibrium emission is significant.…”
Section: Tesnat 2016mentioning
confidence: 99%
“…(1). When looping over all possible residual configurations, the multiple preequilibrium contribution is obtained [7][8][9][10][11][12][13][14][15][16][17][18][19][20]. In TALYS, multiple preequilibrium emission is followed up to arbitrary order; though for 96 MeV, only the secondary preequilibrium emission is significant.…”
Section: Tesnat 2016mentioning
confidence: 99%