2.3. Relativistic Multiple-Scatter<strong>in</strong>g Glauber Approximation 26Contrary to ROMEA, the Glauber IFSI operators of Eq. (2.73) are genu<strong>in</strong>e A-body operators,so the <strong>in</strong>tegration over the coord<strong>in</strong>ates of the spectator nucleons <strong>in</strong> Eq. (2.36) has to be carriedout explicitly:Ŝ RMSGAIFSI (⃗r) ={A∏ ∫∣d⃗r j φ αj (⃗r j ) ∣ [ (2 1 − Γ pN p 1 , ⃗ b − ⃗ )b jj=2×( [1 − Γ pN k 1 , ⃗ b ′ − ⃗ )b ′ j[ (× 1 − Γ Nk2 N k 2 , ⃗ b ′′ − ⃗ )b ′′jθ ( z ′ j − z ′)]]θ (z − z j )θ ( z ′′j − z ′′)]} . (2.74)This makes the numerical evaluation of the Glauber IFSI factor very challeng<strong>in</strong>g. St<strong>and</strong>ardnumerical <strong>in</strong>tegration techniques were adopted to evaluate the IFSI factor <strong>and</strong> no additionalapproximations, such as the commonly used thickness-function approximation, were <strong>in</strong>troduced.Henceforth, we refer to calculations based on Eq. (2.74) as the relativistic multiple-scatter<strong>in</strong>gGlauber approximation (RMSGA).2.3.4 Glauber ParametersIn contrast to the DWIA <strong>and</strong> ROMEA models, all parameters enter<strong>in</strong>g the RMSGA model canbe obta<strong>in</strong>ed directly from elementary nucleon-nucleon scatter<strong>in</strong>g experiments. When calculat<strong>in</strong>gthe Glauber scatter<strong>in</strong>g wave function for a given momentum k, the follow<strong>in</strong>g <strong>in</strong>put isneeded: the total nucleon-nucleon cross section σNN tot , the slope parameter β2 NN, <strong>and</strong> the ratioof the real to the imag<strong>in</strong>ary part of the scatter<strong>in</strong>g amplitude ɛ NN . We obta<strong>in</strong> the proton-proton<strong>and</strong> proton-neutron parameters through <strong>in</strong>terpolation of the database available from the ParticleData Group [94, 95], while the neutron-neutron scatter<strong>in</strong>g parameters are assumed to beidentical to the proton-proton ones because of isosp<strong>in</strong> symmetry.The measured total (σ tot ) <strong>and</strong> elastic (σ el ) cross sections for proton-proton <strong>and</strong> protonneutronscatter<strong>in</strong>g are shown <strong>in</strong> Fig. 2.4. The nature of the NN <strong>in</strong>teraction changes drastically<strong>in</strong> go<strong>in</strong>g from low to high energies. At proton momenta p ≤ 1 GeV/c, the scatter<strong>in</strong>g of nucleonsis completely elastic; while at higher momenta, the <strong>in</strong>teraction becomes <strong>in</strong>elastic <strong>and</strong>absorptive, as new particles are produced. From 1 GeV/c upward, the total reaction cross sectionrema<strong>in</strong>s almost constant, even though the NN <strong>in</strong>teraction leaves the elastic regime <strong>and</strong>becomes more <strong>and</strong> more <strong>in</strong>elastic.The slope parameters β 2 pp <strong>and</strong> β 2 pn can be found by analyz<strong>in</strong>g the t dependence of the differentialcross sections with the aid of expression (2.62). Here, the sp<strong>in</strong>-dependent terms areassumed to be negligible. For proton k<strong>in</strong>etic energies smaller than 1 GeV, the slope parametersextracted <strong>in</strong> this way differ significantly from the values found directly from experiment<strong>and</strong> phase-shift analysis. This can be attributed to a large contribution of the sp<strong>in</strong>-dependentscatter<strong>in</strong>g amplitude [68]. At higher energies, this difference decreases quickly demonstrat<strong>in</strong>gthat the sp<strong>in</strong> terms are small. Below 1 GeV, values for the slope parameters obta<strong>in</strong>ed through
Chapter 2. Relativistic Eikonal A(p, pN) Formalism 27Cross section (mb)10 210σ totσ elppCross section (mb)10 210σ totσ elpn10 -1 1 10Proton momentum (GeV/c)Figure 2.4 Total <strong>and</strong> elastic cross sections for proton-proton <strong>and</strong> proton-neutron scatter<strong>in</strong>g as a functionof the proton lab momentum. The data were taken from Ref. [95]. The solid (dashed) curve is our globalfit to the elastic (total) cross section.Eq. (2.62) are scarce <strong>and</strong> not free of ambiguities due to sp<strong>in</strong> effects. Therefore, <strong>in</strong> our calculations,the slope parameters are determ<strong>in</strong>ed through the follow<strong>in</strong>g relation( ) 2 ( )σpNtot 1 + ɛ 2 pNβ 2 pN =16π σ elpN. (2.75)This parametrization can be derived from the theoretical shape of the elastic pN cross sectionas follows. Expression (2.63) for the elastic scatter<strong>in</strong>g amplitude leads to( ) 2 ( )dσpNeld(∆ 2 ) = π ∣ ∣ ∣∣A( ∆) ⃗ ∣∣2 σpNtot 1 + ɛ 2 pN=k 2 exp ( −β 216πpN∆ 2) . (2.76)Integrat<strong>in</strong>g this st<strong>and</strong>ard high-energy approximation of the elastic differential cross sectionresults <strong>in</strong>∫σpN el =(dσelpNd(∆ 2 ) d(∆2 ) =σ totpN) 2 ( )1 + ɛ 2 pN16πβ 2 pN, (2.77)so that the slope parameter is given by Eq. (2.75). In Fig. 2.5, the slope parameters obta<strong>in</strong>edthrough this expression are compared with those determ<strong>in</strong>ed directly through Eq. (2.62).
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