Hints on Using the Orca Program

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Computational Chemistry Workshops West Ridge Research Building-UAF Campus 9:00am-4:00pm, Room 009 Electronic Structure - July 19-21, 2016 Molecular Dynamics - July 26-28, 2016 Hints on Using the Orca Program

In order to run the Orca program, an input file (e.g. myinp.inp) is created and the executed in the following manner: orca myinp.inp > myinp.log & One of the ways to determine the progress of the job is tail -f myinp.log The general form of the input file for Orca is the following where Cartesian coordinates (xyz), or internal coordinates (int) can be used. The multiplicty is defined as 2S + 1, where S is the total spin of the state of the molecule, and is the the number of unpaired electrons +1. Here is an example for formaldehyde (H 2 C O), where Cartesian coordinates are used: 2

Internal Coordinates: The Z-Matrix If the molecule under investigation is not too large, the most convenient route for building molecules is to manually input bond distances, bond angles and dihedral angles. A definition of the molecular structure in this way is called a Z-Matrix. In order to specify the position of a given atom, one needs six numbers: R, A, and D are the bond distance, the bond angle, and dihedral angle. NA, NB, NC are the numbers atom numbers to which the new atom is connected. The integers NA, NB, and NC are used in the following manner: NA: the new atom connects to a previously defined atom (NA), and with distance, R in Å. NA, NB: the new atom forms an angle with two previously defined atoms (NA and NB), and with angle, A in degrees. NA, NB, NC: the new atom forms a dihedral angle with three previously defined atoms (NA, NB, and NC), and with dihedral angle, D in degrees. This is defined as the angle between the new atom and previously defined atom NC when looking down the NA-NB axis. 1. The first atom is always placed at the origin. 2. The second atom is placed at a distance, R, from the first atom, in Å, along one of the coordinate axes (e.g. x-axis). 3. The third atom is placed in a plane (e.g the xz-plane). 4. Any additional atoms require all six parameters (NA, NB, NC, R, A, D) as discussed above. 3

Constrained Optimization In the following input example, a constrained optimization is performed on the formaldehyde molecule (H 2 C O), but which also illustrates how to use the Z-Matrix formalism for the use of internal coordinates: The following points should be noted with respect to constraining coordinates: It is optional to assign a value for the constraint parameter. If a value is not given, the value in the Z-matrix is constrained. For Cartesian coordinates, the initial position of the atom is constrained. It is recommended to use a value close to the initial structure. It is possible to constrain whole sets of coordinates. 4

Rigid Potential Energy Surface (PES) Scan A rigid potential energy surface scan can be performed as in the following input example. # Scan the H-O-H angle! RHF SVP %paras R_OH = 0.950 # O-H distance A_HOH = 180,90,19 # H-O-H angle (180 to 90 in 19 steps) end * int 0 1 O 0 0 0 0.00 0.00 0.00 H 1 0 0 {R_OH} 0.00 0.00 H 1 2 0 {R_OH} {A_HOH} 0.00 * In the above example, the H O H bond angle will be modified in 18 equidistant 5 steps, ((180 90 )/5 + 1 = 19), and, at each step, a constrained geometry optimization will be carried out to yield a rigid potential energy surface scan of the H O H bond angle. Relaxed Potential Energy Surface (PES) Scan A relaxed potential energy surface scan can be performed as in the following Orca input example. In the above example, the C O bond length will be modified in 12 equidistant steps (1.35 Å - 1.10 Å), and, at each step, a constrained geometry optimization will be carried out to yield a potential energy surface scan of the C O bond stretch. 5

Transition States In order to find transition states, it is necessary to start with a structure that is reasonably close to the transition state. Structures close to a transition state can be obtained by either a relaxed or rigid potential energy surface scan of the principal reaction coordinate. In addition, chemical intuition can also play an important role. Below is the Orca input for the linear H H H molecule, where the coordinates are given n Z-Matrix format: Localized Orbitals (LOCs) Localized orbitals can be obtained by using the %loc end block command, which also creates a file called MyJob.loc. Analyze the composition of Localized Orbitals (LOCs) by running a second calculation and re-reading them with the %moinp Myjob.loc keyword so that these MOs are read and! NoIter keyword, so that no SCF interations are performed. The resulting orbitals can be processed for visualization programs such as VMD, Molden, Gabedit, and others, using the command: orca plot MyJob.loc -i. 6

Unrestricted Corresponding Orbitals (UCOs) An additional analysis tool that can be used here involves unrestricted corresponding orbitals (UCOs). In order to obtain them, use! UCO in the input file. This will produce a file called MyJob.uco and additional output, which consists of spatial overlaps of spin-up and spin-down orbitals. Analyze the composition of these orbitals by running a second calculation and re-reading them with the %moinp Myjob.uco keyword, so that these MOs are read, and! NoIter keyword, so that no SCF interations are performed. Quasi Restricted Orbitals (QROs) A set of Quasi Restricted Orbitals (QROs) can be obtained by employing the keyword, which also creates a file called MyJob.qro.! UNO Analyze the composition of Quasi Restricted Orbitals (QROs) by running a second calculation and re-reading them with the %moinp Myjob.qro keyword so that these MOs are read and! NoIter keyword, so that no SCF interations are performed. The resulting orbitals can be processed for visualization programs such as VMD, Molden, Gabedit, and others, using the command: orca plot MyJob.qro -i. Unrestricted Natural Orbitals (UNOs) A set of Unrestricted Natural Orbitals (UNOs) can be obtained by employing the! UNO keyword, which also creates a file called MyJob.uno. Analyze the composition of Unrestricted Natural Orbitals (UNOs) by running a second calculation and re-reading them with the %moinp Myjob.uno keyword so that these MOs are read and! NoIter keyword, so that no SCF interations are performed. The resulting orbitals can be processed for visualization programs such as VMD, Molden, Gabedit, and others, using the command: orca plot MyJob.uno -i. Broken Symmetry Calculations Together with some approximate formalisms, it is possible to extract a value for J from a high-spin and a broken symmetry calculation. It is possible to specifically ask for such solutions. One of the ways to study antiferromagnetic coupling employs the command %scf BrokenSym 1,1 end. In the output can be found the J(3) value, which is the predicted exchange coupling constant. 7

Example Calculation on the [Cr(H 2 O) 6 ] 3+ Complex Spin-Up Orbitals In spin-unrestricted calculations, there are separate spin-up and spin-down MOs. In the present case of a d 3 system, one would expect that the three spin-up HOMOs are mainly metal t 2g in character, and the two spin-up LUMOs will have metal e g character, which can be verified, by observing the spin-up HOMO/LUMO gap: It can be seen that the three highest occupied and two lowest unoccupied spin-up orbitals are all degenerate, as shown by their composition: The result above is the one that is quite reasonable, as can be seen from the compositions of the orbitals. However, they are not pure d xy, d xz, and d yz orbitals because degenerate orbitals can arbitrarily mix among themselves without changing anything in the physics. These three orbitals simply span the three components of the t 2g representation. 8

Spin-Down Orbitals In addition, the five spin-down LUMOs are expected to represent the spin-down counterparts of the metal t 2g and metal e g orbitals which are shown below: The compositions of the LUMOs are given below: Interestingly, the orbital splittings of the spin-up and spin-down levels are quite different. In general DFT without admixture of Hartree-Fock exchange, as is the case with the BP functional used here, orbital energy difference between occupied and virtual orbitals is a 0th order approximation to the excitation energy. 9

Excited States In the present case, a ligand field transiton energy is predicted around 2.8 ev ( 23000 cm 1 ). This can be checked by running a TD-DFT calculation for only six excited states, corresponding to the six ways of taking an electron out of a t 2g orbital, and placing it into the e g orbital. It can be seen that two excited states that are triply degenerate each and correspond to the singly excited 4 T 1g and 4 T 2g terms expected from Table 1. The splitting between the two states is one of the characterisitics of electron-electron repulsion leading to different multiplets. Despite the small basis set, the result compares favorably with experiment, where transitions are observed at 17,400 cm 1 and 24,700 cm 1. Furthermore, the average of the two transition energies correspond well with the orbital energy difference. It is possible to determine which state corresponds to each symmetry by using a group theoretical table and working out the allowed transitions for a CD spectrum. The magnetic dipole components R x, R y, R z transform as the molecular rotations and belong to the T 1g representation for O h symmetry. Thus, the 4 A 2g 4 T 1g is magnetic-dipole allowed because the direct product A 2g T 1g T 1g yields the totally symmetric representation, A 2g which leads to an allowed transition in the CD spectrum for [Cr(H 2 O) 6 ] 3+. It is not always the case that TD-DFT calculations agree with experiment, and there is every reason to be critical about the calculational results. Very carefully compare the TD-DFT calculations with experiment. In many cases, artifacts will arise: charge transfer states tend to appear much too low in the spectrum; double excitations are entirely missing; neutral-toionic transitions are poorly predicted; and spin-flip transitions cannot be predicted. 10

Excited States The compositions of these transition shows that they indeed correspond to the expected excitations: 11

Keywords for the Orca Program Below is a summary for some of the keywords for the Orca program. 12