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- W2960996910 abstract "Background: The phenomenological optical model has been extensively used to study the nucleon-nucleus scattering process. However, its use in describing the observables for nucleon scattering off light $1p$-shell nuclei has been somewhat limited and less successful. This is a result of their diffuse edges and deformations that complicate fitting the experimental data. Therefore, global optical models usually exclude light nuclei and only consider intermediate and heavy nuclei with mass number $Aensuremath{ge}24$.Purpose: We test the effectiveness of a semimicroscopic optical model with channel coupling in describing observables for neutron scattering off nuclei covering a wide mass range from $^{12}mathrm{C}$ to $^{208}mathrm{Pb}$ corresponding to neutron incident energies in the range $E=10--30phantom{rule{0.28em}{0ex}}mathrm{MeV}$.Method: The real central part of the optical model is constructed by single folding the density-independent M3Y-Paris bare nucleon-nucleon interaction over the density of the target nucleus. The rest of the potential terms are of Woods-Saxon form or its derivative. The potential parameters are determined by fitting the elastic and inelastic angular distributions in addition to polarization data for neutron scattering from $^{12}mathrm{C}, ^{16}mathrm{O}, ^{54}mathrm{Fe}, ^{58}mathrm{Ni}, ^{120}mathrm{Sn}$, and $^{208}mathrm{Pb}$. In doing so the ground state is coupled to few, low-lying rotational and vibrational excitation channels.Results: Despite considering a wide mass range of nuclei, the model resulted in good descriptions for the elastic data and, at least, the overall features of the inelastic angular distributions and polarization data are reproduced. Our potential depths are expressed as linear functions of energy while, for each target nucleus, the geometric parameters are fixed. This is unlike purely phenomenological optical models which, in many cases, resulted in best-fit parameters that show unclear energy-dependence trends. In addition, the total cross sections predicted using our parameters are in good overall agreement with experiment.Conclusions: The semimicroscopic model based on the M3Y-Paris bare $NN$ interaction succeeded in, at least, reproducing the overall features of the inelastic experimental data. However, the predicted elastic angular distributions are in good agreement with experiment and progressively improved with increasing mass number of the target. Furthermore, the weak energy dependence, introduced into the M3Y-Paris interaction via the knock-on exchange term, led to improving our data fits. Finally, other density-dependent bare $NN$ interactions resulted in potential parameters that showed less systematic behaviors with energy." @default.
- W2960996910 created "2019-07-23" @default.
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- W2960996910 date "2019-07-10" @default.
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- W2960996910 title "Semimicroscopic optical model with coupled-channel analysis for neutron scattering off nuclei with mass numbers <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML><mml:mrow><mml:mn>12</mml:mn><mml:mo>≤</mml:mo><mml:mi>A</mml:mi><mml:mo>≤</mml:mo><mml:mn>208</mml:mn></mml:mrow></mml:math>" @default.
- W2960996910 cites W1964382392 @default.
- W2960996910 cites W1966168690 @default.
- W2960996910 cites W1968490984 @default.
- W2960996910 cites W1969023993 @default.
- W2960996910 cites W1969042594 @default.
- W2960996910 cites W1971067051 @default.
- W2960996910 cites W1978852609 @default.
- W2960996910 cites W1980978683 @default.
- W2960996910 cites W1986772294 @default.
- W2960996910 cites W1987636510 @default.
- W2960996910 cites W1990502432 @default.
- W2960996910 cites W1997664190 @default.
- W2960996910 cites W2002118102 @default.
- W2960996910 cites W2002580335 @default.
- W2960996910 cites W2014479698 @default.
- W2960996910 cites W2018207959 @default.
- W2960996910 cites W2023192969 @default.
- W2960996910 cites W2026536084 @default.
- W2960996910 cites W2032643470 @default.
- W2960996910 cites W2038785435 @default.
- W2960996910 cites W2040856230 @default.
- W2960996910 cites W2041497910 @default.
- W2960996910 cites W2048182732 @default.
- W2960996910 cites W2049041673 @default.
- W2960996910 cites W2049373495 @default.
- W2960996910 cites W2054845836 @default.
- W2960996910 cites W2058854293 @default.
- W2960996910 cites W2067561843 @default.
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- W2960996910 cites W2070473564 @default.
- W2960996910 cites W2073833483 @default.
- W2960996910 cites W2078061422 @default.
- W2960996910 cites W2082290039 @default.
- W2960996910 cites W2088055560 @default.
- W2960996910 cites W2090623714 @default.
- W2960996910 cites W2090829571 @default.
- W2960996910 cites W2109415008 @default.
- W2960996910 cites W2116083525 @default.
- W2960996910 cites W2128671143 @default.
- W2960996910 cites W2240737721 @default.
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- W2960996910 cites W2596424079 @default.
- W2960996910 cites W2602566472 @default.
- W2960996910 cites W2769337279 @default.
- W2960996910 cites W2792416760 @default.
- W2960996910 cites W282371158 @default.
- W2960996910 cites W2885864202 @default.
- W2960996910 cites W2986932994 @default.
- W2960996910 cites W3098615902 @default.
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- W2960996910 doi "https://doi.org/10.1103/physrevc.100.014603" @default.
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