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By C. Pajares and Yu.M. Shabelski
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Extra resources for Relativistic Nuclear Interactions
Sample text
Shadowing corrections to Eq. 10) can be calculated in a similar manner with the result given in Eq. 35), where the factors (J el/(J come from the separation of elastic intermediate states in the cut hN interaction blobs and the numerical coefficients can be recognized as the AGK prescription in Eq. 35). hese calculations to the interested readers as a useful and instructive exercise. It is worth noting that final state interactions of nucleons do not change the sum of integrated cross sections for the elastic and quasi-elast ic scattering (Jhdat , see Eq.
10) can be calculated in a similar manner with the result given in Eq. 35), where the factors (J el/(J come from the separation of elastic intermediate states in the cut hN interaction blobs and the numerical coefficients can be recognized as the AGK prescription in Eq. 35). hese calculations to the interested readers as a useful and instructive exercise. It is worth noting that final state interactions of nucleons do not change the sum of integrated cross sections for the elastic and quasi-elast ic scattering (Jhdat , see Eq.
38) relu rn to the usual Glauber theory with only elastic rescattering. 79) are parametrically dill! lf' lll III Ille cClse of heavy nuclear targets both O"~~ and 0"~'1 are of the order 10 1 ,, /I \ IlIld dl' Pl:lld only slightly on the theoretical approach and its parameters. 5. 0 F rr) "N « ~ 50 ~ D 2 Q. c b 40 - -- -: :~: : :~~ 30 ... J" ... ", ... '" p p T\ ± K± -l-< 20 10 o 10 A Fig. 7. Cross sections of secondary hadron production on nuclear targets for different incident beams at 200 GeV/ c [125] a = 2/3 is not sufficiently well satisfied, as one can see in Fig.