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Orbital angular momentum contraction

The second (indirect) relativistic effect is responsible for the expansion of outer d and f orbitals Here the relativistic contraction of the s and pi/2 shells results in a more efficient screening of the nuclear charge, and the outer high angular momentum orbitals expand and become energetically destabilized. In turn, the relativistically expanded d and f orbitals cause a small additional... [Pg.11]


See other pages where Orbital angular momentum contraction is mentioned: [Pg.83]    [Pg.232]    [Pg.540]    [Pg.205]    [Pg.116]    [Pg.116]    [Pg.546]    [Pg.167]    [Pg.167]    [Pg.320]    [Pg.6]    [Pg.228]    [Pg.214]    [Pg.357]    [Pg.540]    [Pg.100]    [Pg.100]    [Pg.469]    [Pg.18]    [Pg.19]    [Pg.9]    [Pg.39]    [Pg.292]    [Pg.69]    [Pg.3]    [Pg.205]    [Pg.705]    [Pg.321]    [Pg.270]    [Pg.126]    [Pg.90]    [Pg.121]    [Pg.149]    [Pg.101]    [Pg.11]    [Pg.11]    [Pg.16]    [Pg.281]    [Pg.291]    [Pg.97]    [Pg.502]    [Pg.55]    [Pg.208]    [Pg.278]    [Pg.257]    [Pg.151]    [Pg.96]    [Pg.52]    [Pg.53]   
See also in sourсe #XX -- [ Pg.78 , Pg.281 ]




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