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The Physics of Spallation Processes

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3.2. CALCULATIONS OF HADRONIC SHOWERS 33further hadronic interactions once the π ± are created. At still higher energies, well above10 GeV, other meson production channels open up which in addition deplete the cascade<strong>of</strong> energy 2 . Using Monte-Carlo methods, the spatial distribution <strong>of</strong> such hadronic showersinside a massive cylindrical Pb-target will be discussed in the following.3.2 Calculations <strong>of</strong> hadronic showersIn the case <strong>of</strong> thick targets, the reaction scenario includes secondary and higher-orderreactions induced by the reaction products themselves and, therefore, the calculationsmust include a 3-dimensional simulation <strong>of</strong> inter-nuclear cascades. Such a 3-dimensionaldescription <strong>of</strong> the propagation <strong>of</strong> the inter-nuclear cascade and the transport <strong>of</strong> particles inthick targets is a rather complex problem that involves various boundary conditions. Thisissue is addressed in the following, where the propagation <strong>of</strong> various species <strong>of</strong> particletypes (p, n) is considered separately in longitudinal and radial directions. <strong>The</strong> energylosses <strong>of</strong> high-energy particles (≥ 1 GeV) traveling through matter are mainly determinedby the production <strong>of</strong> secondary particles and not due to electronic stopping which isdominating at lower bombarding energies. Thus, the main feature <strong>of</strong> the cascade is aninitial increase <strong>of</strong> the particle intensity with depth and time. As already mentioned, ifthe energy <strong>of</strong> the produced secondary particles is high enough, they in turn knock outadditional particles. <strong>The</strong>re exists however a physical limit for the development <strong>of</strong> furthercascades, because the initial energy <strong>of</strong> the primary particle is distributed among theproduced particles. <strong>The</strong>refore, the multiplicities tend to decrease again during the cascadeprocess and fade away because the average energy <strong>of</strong> the cascade particles decreases anda greater fraction <strong>of</strong> the individual particle energy is now dissipated by ionization losses.At the end <strong>of</strong> the inter-nuclear cascade process, subsequent emission <strong>of</strong> many low energyparticles, mainly neutrons, takes place, known as evaporation process [Wei40].<strong>The</strong> development <strong>of</strong> electromagnetic showers with their principal production processes -bremsstrahlung for electrons and positrons, pair production for photons, becoming energydependent above 1 GeV - are well described by quantum electro dynamics (QED-theory)over a wide energy range. In HERMES this is taken into account by the EGS4 code aswill be discussed in section 4.3. <strong>The</strong> complexity and entanglement <strong>of</strong> all intra- and internuclearcascade processes finally causing the production <strong>of</strong> neutrons requires a complexrecord keeping <strong>of</strong> all particles actually participating in terms <strong>of</strong> energy, direction andlocation. <strong>The</strong> simulated propagation <strong>of</strong> the three-dimensional hadronic showers followingthe bombardment <strong>of</strong> cylindrical lead targets <strong>of</strong> 35 cm x 15 cm (for the length and diameter,respectively) by 0.4, 1.2 and 2.5 GeV protons is illustrated in the contour plots <strong>of</strong> Fig. 3.3.In the HETC+MORSE (cf.sect. 4.3) Monte-Carlo calculations to produce the datafor Fig. 3.3 the cylindrical target is divided into cylindrical zones <strong>of</strong> 0.5 cm in radial (r)and 1 cm (z) in longitudinal direction and the tracklength flux 3 [Clo88] is represented.<strong>The</strong> symmetry axis <strong>of</strong> the cylinder is oriented in z direction and pointing downstream theproton beam. <strong>The</strong> tracklength flux <strong>of</strong> neutrons (left) and protons (right) reflects the radialand longitudinal propagation <strong>of</strong> particles involved in the intra- and internuclear cascades2 an effect being responsible for the decrease <strong>of</strong> the number <strong>of</strong> neutrons plotted in Fig. 7.9 <strong>of</strong> sect. 7.1.13 tracklength flux as defined in equation 4.2 <strong>of</strong> sect. 4.1

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