2007
DOI: 10.1016/j.nuclphysa.2007.04.024
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Analysis of emission mechanisms in nucleon-induced reactions around the Fermi energy

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Cited by 7 publications
(4 citation statements)
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“…In contrast to the scattering of neutrons, which is taken as isotropic, those between neutron and proton σ np and between protons σ pp are anisotropic in accordance with the fit of Ref. [26], which is given in detail in the Appendix. Similarly to above, the corresponding values of R sim NN on the evolving nuclear density [27],…”
Section: A a Density-dependent N N Cross Sectionmentioning
confidence: 63%
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“…In contrast to the scattering of neutrons, which is taken as isotropic, those between neutron and proton σ np and between protons σ pp are anisotropic in accordance with the fit of Ref. [26], which is given in detail in the Appendix. Similarly to above, the corresponding values of R sim NN on the evolving nuclear density [27],…”
Section: A a Density-dependent N N Cross Sectionmentioning
confidence: 63%
“…The dimensionless weighting factor f (E, θ) is equal to unity for the scattering between neutrons (f nn ≡ 1) and is increasingly anisotropic as energy increases for neutron-proton scattering (the f np case), and especially becomes strongly forward-backward peaked for the scattering between protons (f pp ). The parametrization of the angular dependence of σ np is defined as [26] f (E, θ) np = A 1 cos 4 θ − A 2 cos 3 θ + A 3…”
Section: Appendixmentioning
confidence: 99%
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“…[4] a preliminary resolution scheme of the ETDHF equation was proposed and different aspects of the description were analyzed. Applications to HIC at intermediate energies [10] and to nucleon induced collisions [11] have been performed. An extension of the model adapted to the description of the outer layers of neutron star crusts has also been developed [12].…”
Section: The Dissipative Behaviormentioning
confidence: 99%