Sample directory: adf/e_RelTS_CH4_HgCl2/
A Transition State calculation, including scalar relativistic terms in the Hamiltonian.
First the relativistic core potentials are generated.
$ADFBIN/dirac -n1 < $ADFRESOURCES/Dirac/Hg.4d $ADFBIN/dirac -n1 < $ADFRESOURCES/Dirac/Cl.2p $ADFBIN/dirac -n1 < $ADFRESOURCES/Dirac/C.1s $ADFBIN/dirac -n1 < $ADFRESOURCES/Dirac/H mv TAPE12 t12.rel
Then the (relativistic) Create runs.
$ADFBIN/adf << eor create Hg $ADFRESOURCES/TZP/Hg.4d relativistic corepotentials t12.rel & Hg 1 end end input eor mv TAPE21 t21.Hg $ADFBIN/adf << eor create Cl $ADFRESOURCES/TZP/Cl.2p relativistic corepotentials t12.rel & Cl 2 end end input eor mv TAPE21 t21.Cl $ADFBIN/adf << eor create C $ADFRESOURCES/TZP/C.1s relativistic corepotentials t12.rel & C 3 end end input eor mv TAPE21 t21.C $ADFBIN/adf << eor create H $ADFRESOURCES/TZP/H relativistic corepotentials t12.rel & H 4 end end input eor mv TAPE21 t21.H
In the first Create run (Hg) the CorePotentials key could have been used in its simple form, but in the second (and third and fourth, omitted here) the block form is required to identify the appropriate section on TAPE12 for the atom at hand. In the first case we could have relied on the default: the first section on TAPE12 for the first (in this case: only) atom type.
Note that even for H, which obviously has no frozen core at all, we specify the TAPE12 corepotentials file and indicate the appropriate section for H. The reason is that TAPE12 contains not only the (frozen) core, but also the total atomic (relativistic) potential.
Finally the TS run.
$ADFBIN/adf << eor TITLE Transition State: CH4 + HgCl2 <===> CH3HgCl + HCl noprint sfo,frag print atdist GEOMETRY TransitionState END relativistic corepotentials t12.rel & C 3 Hg 1 Cl 2 H 4 end XC lda VWN Stoll END DEFINE rHg = 2.30 rX1 = 2.35 rX2 = 2.90 rH1 = 1.10 rH2 = 1.10 rH3 = 1.40 aX1 = 160 aX2 = 70 aH1 = 100 aH2 = 140 aH3 = 65 dH = 60 END ATOMS Z-Matrix 1. C 0 0 0 0. 0. 0. 2. Hg 1 0 0 rHg 0. 0. 3. Cl 2 1 0 rX1 aX1 0. 4. H 1 2 3 rH1 aH1 dH 5. H 1 2 3 rH1 aH1 -dH 6. H 1 2 3 rH2 aH2 180. 7. H 1 2 3 rH3 aH3 180. 8. Cl 2 1 3 rX2 aX2 180. END FRAGMENTS Hg t21.Hg C t21.C H t21.H Cl t21.Cl END endinput eor
For the density-functional the Local Density approximation is used (no GGA corrections), with a correlation correction term due to Stoll (see the User's Guide).
At each geometry cycle the interatomic distance matrix is printed (print atdist).
The initial geometry is a reasonable but not very accuracte estimate of the Transition State. The program needs quite a few cycles to converge, which is rather typical for ts searches: they are a lot more tricky and fail more often than a simple minimization.




