#! /bin/sh # Spin-orbit coupled relativistic ZORA, X2C, and RA-X2C # are compared in this example for the calculation of # Core Electron Binding Energies (CEBEs). # In this case the CEBE of the 1s of Iodine in the molecule HI. # For such calculations X2C or RA-X2C is recommended. # Note, for more accurate calculations one should increase the basis set. # In this example the LDA functional is used. # Results of this example will show that for X2C the CEBE is around 33.211 keV # and for RA-X2C the CEBE is around 33.202 keV. # If one increases the basis set (especially in the core region), for example, with a QZ4P basis set, # the results obtained with X2C and RA-X2C will be much closer. # In case of ZORA, without the scaled ZORA energy correction # the CEBE in this case is around 34.515 keV, much larger than the results with X2C or RA-X2C. # If one includes the scaled ZORA energy correction (can be found in the output) # the CEBE in case of ZORA is around 33.238 keV. # NOTE: The scaled ZORA energy correction should only be used to compare two calculations # in which the only difference in the calculation is the electron configuration. # Then the difference in energy of this term should be added to the difference in energy of # the two electron configurations. # This term should not be used otherwise. # In practice it is useful only for core excitation energy calculations. for f in "ZORA" "X2C" "RA-X2C" do AMS_JOBNAME=HI_$f $AMSBIN/ams <