1998
DOI: 10.1103/physrevc.57.3185
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Rescattering in knockout reactions as manifested in40Ca(p,pp

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Cited by 29 publications
(24 citation statements)
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“…However, this observable does not permit us to have complete control over the number of knocked out nucleons in the collision. For this reason, in this work we use quadruple-differential cross sections of two coincident protons produced in proton-induced reactions on 40 Ca at 392 [17], and quadruple-and triple-differential cross sections of two coincident protons produced in proton-induced reactions on 197 Au at 200 MeV [88]. We have selected this set of experimental data taking into account the study of onenucleon-removal cross sections performed in Sec.…”
Section: B Quadruple-and Triple-differential Cross Sections For Coinmentioning
confidence: 99%
See 1 more Smart Citation
“…However, this observable does not permit us to have complete control over the number of knocked out nucleons in the collision. For this reason, in this work we use quadruple-differential cross sections of two coincident protons produced in proton-induced reactions on 40 Ca at 392 [17], and quadruple-and triple-differential cross sections of two coincident protons produced in proton-induced reactions on 197 Au at 200 MeV [88]. We have selected this set of experimental data taking into account the study of onenucleon-removal cross sections performed in Sec.…”
Section: B Quadruple-and Triple-differential Cross Sections For Coinmentioning
confidence: 99%
“…On the one hand, we can follow in time all the particles participating in the nuclear collision, determining their multiple-scattering probabilities and final states. In other models, such as the distorted-wave Born approximation (DWBA) or distorted-wave impulse approximation (DWIA) [14,15], the evaluation of the multiple scattering at higher energies (>300 MeV) is complicated by the possible production of pions and their propagation, which is not considered [16,17]. On the other hand, the dynamical models permit us to characterize the remnant in atomic and mass numbers, excitation energy, and angular momentum [18,19].…”
Section: Introductionmentioning
confidence: 99%
“…Garcia et al 1989, hereafter G89). The optical counterpart visible during the low state is an F8IV object (Cowley & Schmidtke 1990) whose colours were initially observed to be inconsistent with a normal star (Kaluzny 1988). However, subsequent observations failed to con®rm this abnormality in the optical colours of the F star (Deutsch et al 1996).…”
Section: U2129 47mentioning
confidence: 99%
“…In DWBA and DWIA, rescattering is modeled as absorption owing to the imaginary part of an optical potential, which seems far-fetched at the energies we are concerned with. Analyses of proton spectra from the continuum have indeed shown that, even in the 200-400 MeV incident-energy range, it is necessary to go beyond DWIA insofar as the description of rescattering is concerned [see, e.g., [29][30][31]. Finally, the evaluation of rescattering at higher energies is complicated by the possible production of pions in the knockout collision.…”
Section: B Appropriateness Of Inc/de-excitationmentioning
confidence: 99%