Nucleus δE$_{p}$ ( F R ) σ δE$_{p}$ ( G ) σ δE$_{sc}$ Δ$_{FR}$ Δ$_{G}$ $^{90}$Zr 1 . 59 0 . 19 1 . 88 0 . 20 1 . 44 0 . 15 0 . 44 $^{100}$Sn − 7 . 47 0 . 064 − 7 . 42 0 . 14 − 7 . 01 0 . 46 0 . 41 $^{132}$Sn − 7 . 39 0 . 068 − 6 . 04 0 . 12 − 6 . 64 0 . 75 0 . 60 $^{146}$Gd 4 . 89 0 . 10 5 . 28 0 . 24 4 . 52 0 . 37 0 . 76 $^{180}$P b − 8 . 94 0 . 15 − 7 . 78 0 . 04 − 8 . 62 0 . 32 0 . 84 $^{208}$P b 7 . 57 0 . 07 6 . 73 0 . 03 7 . 29 0 . 28 0 . 56 Nucleus δE$_{n}$ ( F R ) σ δE$_{n}$ ( G ) σ δE$_{sc}$ Δ$_{FR}$ Δ$_{G}$ $^{68}$Ni 0 . 16 0 . 12 0 . 50 0 . 07 0 . 81 0 . 65 0 . 31 $^{78}$Ni − 3 . 59 0 . 07 − 2 . 78 0 . 16 − 4 . 21 0 . 62 1 . 43 $^{90}$Zr − 7 . 42 0 . 06 − 7 . 35 0 . 17 − 6 . 82 0 . 60 0 . 53 $^{122}$Zr − 5 . 92 0 . 11 − 4 . 52 0 . 15 − 6 . 33 0 . 41 1 . 81 $^{124}$Zr − 4 . 12 0 . 12 − 3 . 25 0 . 13 − 4 . 35 0 . 23 1 . 10 $^{100}$Sn − 8 . 16 0 . 20 − 6 . 95 0 . 23 − 7 . 50 0 . 66 0 . 55 $^{132}$Sn − 9 . 85 0 . 14 − 8 . 58 0 . 10 − 8 . 87 0 . 98 0 . 29 $^{146}$Gd 10 . 26 0 . 07 10 . 33 0 . 20 9 . 79 0 . 47 0 . 54 TABLE II: Neutron shell corrections δE$_{n}$ and their variations σ calculated using the finite range weight function ( F R ) and the generalized Strutinski procedure G in comparison with the semi- classical shell correction δE$_{sc}$ = E$_{sc}$ − E n sp calculated for several nuclei. Their deviations from the semi-classical result Δ$_{FR}$ = | δE$_{sc}$ − δE$_{n}$ ( F R ) | , Δ$_{G}$ = | δE$_{sc}$ − δE$_{n}$ ( G ) | are also shown. All energies are in MeV units. TABLE III: Proton shell corrections δE$_{p}$ and their variations σ calculated using the finite range weight function ( F R ) and the generalized Strutinski procedure G in comparison with the semi- classical shell correction δE$_{sc}$ = E$_{sc}$ − E n sp calculated for several nuclei. Their deviations from the semi-classical result Δ$_{FR}$ = | δE$_{sc}$ − δE$_{p}$ ( F R ) | , Δ$_{G}$ = | δE$_{sc}$ − δE$_{p}$ ( G ) | are also shown. All energies are in MeV units. 19