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                                 Abstract:We examine how the density matrix affects the Pauli corrections to the pion-nucleus optical potential in the region of the Δ33 resonance,i.e. for pion kinetic energies of 50~300MeV. Four different approaches-shell Model with harmonic oscillator wave functions, uniform, local and revised local Fermi-Gas models-are used to calculate the density matrix.
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                        References
	
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