1974
DOI: 10.1016/0029-554x(74)90113-x
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A method for energy-loss and range calculations based on empirical approximations

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Cited by 43 publications
(22 citation statements)
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“…The agreement with the StM calculation is good for the 48 Ti(α,p) 51 V reaction although the experimental results are slightly overestimated at the upper and lower end of the measured energy interval. It is interesting to note that the NON-SMOKER calculation for the 48 Ti(α,p) 51 Cr reaction deviates from the TALYS calculation, leading to better agreement at higher and lower energies, but underestimation in the middle.…”
Section: Timentioning
confidence: 97%
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“…The agreement with the StM calculation is good for the 48 Ti(α,p) 51 V reaction although the experimental results are slightly overestimated at the upper and lower end of the measured energy interval. It is interesting to note that the NON-SMOKER calculation for the 48 Ti(α,p) 51 Cr reaction deviates from the TALYS calculation, leading to better agreement at higher and lower energies, but underestimation in the middle.…”
Section: Timentioning
confidence: 97%
“…In the mass range under study the Gamow window is found at E red ≈ 0.29 MeV for T 9 = 1 (where T 9 is the temperature in Giga-Kelvin); the variation between 21 Ne (E red = 0.293 MeV) and 51 V (E red = 0.279 MeV) is practically negligible (and even for heavy nuclei like 208 Pb a close value of E red = 0.264 MeV is found for T 9 = 1). T 9 = 2 corresponds to E red ≈ 0.45 MeV, and T 9 = 3 corresponds to E red ≈ 0.59 MeV for all nuclei under study in this work.…”
Section: Introductionmentioning
confidence: 95%
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