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Measurement of the (p,{gamma}) Cross Sections of {sup 46}Ti, {sup 64}Zn, {sup 114}Sn and {sup 116}Sn at Astrophysically Relevant Energies

Journal Article · · AIP Conference Proceedings
DOI:https://doi.org/10.1063/1.3120138· OSTI ID:21289632
; ; ; ;  [1]
  1. Physics Department, Western Michigan University, Everett Tower, 1903 W. Michigan Ave., Kalamazoo, MI 48009-5252 (United States)
The total cross sections for the {sup 116}Sn(p,{gamma}){sup 117}Sb, {sup 114}Sn(p,{gamma}){sup 115}Sb, {sup 64}Zn(p,{gamma}){sup 65}Ga, and {sup 46}Ti(p,{gamma}){sup 47}V reactions have been measured using an activation technique for protons with center-of-mass energies between about 1 and 4 MeV. Radiative proton captures on {sup 116}Sn and {sup 64}Zn are compared to previous measurements while extending the measured energy range. From these measurements, astrophysical S-factors have been deduced by integrating NON-SMOKER results which have been scaled to the deduced S-factors in the measured energy range. Comparisons are made to thermonuclear reaction rates from the MOST and NON-SMOKER statistical model calculations.
OSTI ID:
21289632
Journal Information:
AIP Conference Proceedings, Journal Name: AIP Conference Proceedings Journal Issue: 1 Vol. 1099; ISSN APCPCS; ISSN 0094-243X
Country of Publication:
United States
Language:
English

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