Abstract
The implementation of π production in the Liège intranuclear cascade model (INCL4) for spallation reactions is revisited to alleviate the overestimate of the π yield. Three modifications are proposed for this purpose: a better cross section at high energy, the introduction of a π average potential, and the modification of the average mass of the Δ resonance. The π potential is determined from a global fit of a set of data bearing on π production in proton-induced reactions, on -nucleus and absorption cross sections, and on proton production in π-induced reactions. The resulting π potential is poorly determined in the nuclear interior and agrees with the phenomenological optical-model potentials in the surface region. With these modifications, the predictions of the INCL4 model concerning π production cross sections in proton-induced reactions are considerably improved. Predictions of the improved version for -nucleus reaction and absorption cross sections and for proton, residue, and fission cross sections in π-induced reactions are also presented and shown to give reasonably good agreement. Neutron production and some aspects of fission in π-induced reactions are also investigated and reasonably well predicted. Effects on the modifications on observables, which are not directly linked with π's, such as the neutron yield and the residue mass and charge spectra in proton-induced reactions are also investigated and shown to improve the description of these observable quantities. Several results on π production and the relative insentivity to the π potential in the nuclear interior are shown to be consistent with the fact that most π's are not produced in early collisions. Importance of rescattering in π absorption on nuclei is also pointed out. A comparison is made with the so-called Δ-hole model. Residual discrepancies are identified and are interpreted as due to the lack of π interaction with two nucleons at low energy, to the neglect of quantum motion effects, and to a possible underestimate of rescattering.
20 More- Received 7 June 2006
DOI:https://doi.org/10.1103/PhysRevC.74.064607
©2006 American Physical Society