The following approaches to treat relativistic effects are available in DALTON:
rsp_ecp
example in the test-suite. The corresponding spin-orbit
operators are not implemented.
.DOUGLAS-KROLL
keyword
**DALTON INPUT .DOUGLAS-KROLL .RUN WAVE FUNCTIONS ....
See also the energy_douglaskroll
example in the test suite.
NOTE: Exact analytical gradients and Hessians are not available at the moment, the approximate gradient and Hessians does, however, give fairly accurate geometries. For this approach, only basis sets should be used where the contraction coefficients were optimized including the Douglas-Kroll operators. DALTON currently provides: DK-Pol (relativistic version of Sadlej's POL basis sets), raf-r for some heavy elements, and the relativistically recontracted correlation-consistent basis sets of Dunning (cc-pVXZ-DK, X=D,T,Q,5). The combination with property operators should be done with care, e.g. the standard magnetic property operators are not suitable in this case.
..... **INTEGRALS .MNF-SO replaces .SPIN-ORBIT .....
For properties, the same substitution should be made, in the case of special
components, X1SPNORB
labels are replaced by X1MNF-SO
and so on, whereas the
two-electron terms will be skipped completely. For calculating phosphorescence with
the quadratic response scheme, .PHOSPHORESENCE
should be just replaced by
.MNFPHO
which takes care of choosing the appropriate integrals.
NOTE:
The choice between the Breit-Pauli or Douglas-Kroll mean-field operator is done by (not) providing the .DOUGLAS-KROLL keyword. It is therefore not possible to combine e.g. non-relativistic wave-functions with the Douglas-Kroll spin-orbit integrals.
In the present implementation, the mean-field approach works only for basis sets with a generalized contraction scheme such as the ANO basis sets, raf-r, or cc-pVXZ(-DK). For other types of basis sets, the program might work without a crash, but it will most likely provide erroneous results.