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Download Thesis in Pdf Format - Theoretical Nuclear Physics and ...

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Chapter 2. Relativistic Eikonal A(p, pN) Formalism 23with βNN 2 the slope parameter. This Gaussian parametrization is based on the diffractive pattern,with broad maxima <strong>and</strong> diffractive dips, observed <strong>in</strong> elastic NN collisions at GeV energies.Similar to Fraunhofer diffraction <strong>in</strong> optics, the diffraction phenomenon occurs when thewavelength of the projectile is short compared to the size of the <strong>in</strong>teraction region. The differentialcross section dσ/dt, with t ≡ (k µ f − kµ i )2 the M<strong>and</strong>elstam variable, is extremely forwardpeaked <strong>and</strong> drops exponentially over many orders. The slope parameter βNN 2 describes the tdependence of the elastic NN differential cross section at forward angles:dσ elNNdt≈ dσel NNdt∣ exp ( −βNN 2 |t| ) . (2.62)t=0Us<strong>in</strong>g the optical theorem Im F (θ = 0, φ = 0) = k σtot4π, one f<strong>in</strong>dsA( ∆) ⃗ = k )σtot NN4π(ɛ NN + i) exp(− β2 NN ∆2, (2.63)2with ɛ NN the ratio of the real to the imag<strong>in</strong>ary part of the scatter<strong>in</strong>g amplitude.The <strong>in</strong>verse Fourier transform of Eq. (2.57) br<strong>in</strong>gs about the follow<strong>in</strong>g expression for theprofile function:Γ NN(k, ⃗ )b = σtot NN (k) (1 − iɛ NN (k))4πβNN 2 (k)( )⃗ b2exp −2βNN 2 (k) . (2.64)The profile function for central elastic NN scatter<strong>in</strong>g depends on the momentum k throughthree parameters: the total NN cross sections σNN tot (k), the slope parameters β2 NN(k), <strong>and</strong> theratios of the real to the imag<strong>in</strong>ary part of the scatter<strong>in</strong>g amplitude ɛ NN (k). These parameterscan be determ<strong>in</strong>ed directly from the elementary proton-proton <strong>and</strong> proton-neutron scatter<strong>in</strong>gdata, <strong>and</strong> will be discussed <strong>in</strong> Section 2.3.4.At lower energies, that part of the profile function proportional to ɛ NN (k) is non-Gaussian<strong>and</strong> makes significant contributions to nuclear scatter<strong>in</strong>g. Rather than Eq. (2.64), a parametrization<strong>in</strong> terms of the Arndt NN phases [12,13] is appropriate at lower energies. For the Glaubercalculations presented here, which address higher energies, the Gaussian-like real part ofΓ NN(k, ⃗ )b is the dom<strong>in</strong>ant contributor, <strong>and</strong> the use of Eq. (2.64) is justified.2.3.2 Glauber Multiple-Scatter<strong>in</strong>g Extension of the EAAssum<strong>in</strong>g that the sequential scatter<strong>in</strong>gs are <strong>in</strong>dependent, the eikonal method can easily beextended to multiple scatter<strong>in</strong>g. This constitutes the basis of Glauber theory [62–64]. The scatter<strong>in</strong>goff a composite system (the IFSI <strong>in</strong> A(p, pN) reactions) is modeled as the scatter<strong>in</strong>g ofa fast particle (the <strong>in</strong>cident, scattered, or ejected nucleon) with the scatter<strong>in</strong>g centers of thecomposite system (the spectator nucleons <strong>in</strong> the residual nucleus). We assume that the fastparticle’s momentum is much larger than that of the spectator nucleons. Then, the particle undergoesa negligible deflection <strong>and</strong> its trajectory can be approximated by a straight l<strong>in</strong>e (thisis the EA). In addition, because the time it takes the particle to traverse the nucleus is very

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