Technical Support Information
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Overlay 615 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30 31 32 35 36 37 38 39 40 41 42 43 44 45 46 47 48 49 51 52 53 54 55 56 57 58 59 60 61 62 63 64 65 70 71 72 73 74 75 76 77 78 79 80 81 82 IOp(6/15)SPECIFICATION OF ADDITIONAL CENTERS. IF MORE THAN ONE OF THESE IS REQUESTED, THE LISTS ARE IN SEPARATE INPUT SECTIONS IN THE ORDER LISTED BELOW. 0 NO ADDITIONAL CENTERS. EVALUATE THE PROPERTIES ONLY AT EACH ATOMIC CENTER. 1 READ ADDITIONAL CENTERS. ONE
CARD PER CENTER WITH THE X, Y AND Z 2 READ IN COORDINATES AS FOR
1. STARTING AT EACH POINT, LOCATED THE 4 Read in a set of cards specifying
a grid of points at which the electric potential will be computed. A. Evenly spaced rectangular grid. Three cards are required: KTape,XO,YO,ZO -- output unit and coordinates of one corner of grid. If KTape is 0, it defaults to 51. N1,X1,Y1,Z1 -- number of increments and vector. N2,X2,Y2,Z2 -- number of increments and vector. N1 records will be written to unit KTape, with N2 values in each record. B. An arbitrary list of points. Only one card is needed: N,NEFG,LTape,KTape The coordinates of N points in Angstroms will be read unit LTape in format (3F20.12). The potential (NEFG=3), potential and field (NEFG=2), or potential, field, and field gradient (NEFG=1) will be computed and written along with the coordinates to unit KTape in format (4F20.12). Thus if NEFG=3 for each point there will be 4 cards written per point, containing: X-coord,Y-coord,Z-coord,Potential X-field,Y-field,Z-field,XX-EFG YY-EFG,ZZ-EFG,XY-EFG,XZ-EFG YZ-EFG Note that either form of grid should be specified with respect to the standard orientation of the molecule. 8 Do potential-derived charges. 16 Constrain the dipole in fitting charges. 32 Read in centers at which to evaluate the potential from the rwf. 128 Read grid; do not default cube. IOp(6/16)Cutoffs in L602. 0 Use full accuracy in calculations at specific points, but use sleazy cutoffs in mapping a grid of points. 1 Do all points to full accuracy. IOp(6/17)DEBUGGING CONTROL (L602). 0 COMPUTE ALL CONTRIBUTIONS TO SELECTED PROPERTIES. 1 COMPUTE ONLY THE NUCLEAR CONTRIBUTION. 2 COMPUTE ONLY THE ELECTRONIC CONTRIBUTION. -N COMPUTE ONLY THE CONTRIBUTION OF SHELL N. IOp(6/18)Whether to update dipole rwf 0/1 yes/no. IOp(6/19)Whether to rotate exact polarizability before comparing with approximate (which will be calculated in the standard orientation). This is like IOp(9) in L9999. 0 Default, same as 1. 1 Exact is still in standard orientation; use as-is. 2 Exact is already in z-matrix orientation, so rotate. IOp(6/20)How to do electrostatic-potential derived charges: 0 Default (1). -1 Read a list of points at which to fit, one per line. 1 Merz-Kollman point selection 2 CHELP point selection. 3 CHELPG point selection. 00 Default radii are those defined with the selected method. 10 Force Merz-Kollman radii. 20 Force CHELP (Francl) recommended radii. 30 Force CHELPG (Breneman) recommended radii. 100 Read in replacement radii for selected atom types as pairs (IAn,Rad) or (Symbol,Rad), terminated by a blank line. 200 Read in replacment radii for selected atoms as pairs (I,Rad), terminated by a blank line. 1000 Fit united atoms (heavy atoms only) rather than all atoms. 10000 Use only active atoms in the fit. IOp(6/21)Operation of L603: 0 Default (same as 2). 1 Read in density basis functions and compute populations. 2 Optimize density basis set. IOp(6/22)Selection of density matrix (currently only in L601, L602, L604): -1x Read density matrices from .chk file. +1x Read density matrices from .chk file. -5 All available transition densities. -4 Transition density between the states given by IOp(29) and IOp(30). -3 Density for the excited state given by IOp(29). -2 Use all available density matrices. -1 Use the density matrix for the current method, or the HF density if the one for the current method is not available. N.ge.0 Use the density matrix for method N (see Link 1 for the numbering scheme). IOp(6/23)Density values to evaluate over grid in L604: 0 Default (same as 3). 1 Density values. 2 Density values and gradients. 3 Density values, gradients and divergence. IOp(6/24)Frozen core: -N Freeze N orbitals. 0 Default (Yes). 1 Yes. 2 No. IOp(6/25)Whether to compute coulomb self-energy in L601: 0 No. 1 Yes, classically (including self terms - requires 2e integrals, O(N**4)). 2 Yes, quantum mechanically (no self terms - requires 2e integrals, and only available for HF. O(N**5)). IOp(6/26)Which density to use in L602 and L604: 0 Default (same as 1). 1 Total. 2 Alpha. 3 Beta. 4 Spin. IOp(6/27)Choice of population analysis: 0 Default (12). 1 Don't do Mulliken populations. 2 Do Mulliken populations. 10 Don't do bonding Mulliken Populations. 20 Do bonding Mulliken Populations. 100 Do Minimal population analysis. IOp(6/28)Mark SCF density as current density. 0 No: save SCF density, but do not mark. 1 Yes: mark as well. IOp(6/29)Excited state to use if requested by IOp(22). IOp(6/30)2nd excited state for transition density: 0 Transition denstiy between state IOp(29) and g.s. N Transition denstiy between state IOp(29) and state N. IOp(6/31)Whether to determine natural orbitals from densities: 0 No. 1 Yes, using total density. 2 Yes, using alpha and beta separately for UHF. 3 Store only alpha NOs. 4 Store only beta NOs. 5 Use spin density. IOp(6/32)CONTROL PARAMETERS FOR COVBON in L609 (NOT TO BE CHANGED UNDER MOST CIRCUMSTANCES): 10000*MItLoc+1000*ITlLoc+100*IDcInt+IPrLoc, where MItLoc MItLoc*NOrb*(NOrb-1)/2 is the
maximum number of iterations in ITlLoc 10.**(-ITlLoc) is the convergence criterion for (spin)orbital localization (1...9, default 9), IDcInt Localized (spin)orbitals
with atomic occupancies less than 0.01*IDcInt are IPrLoc 0: Print the atomic occupancies
of localized (spin)orbitals (default), L605, L606: naming of RPAC interface file. 0 Make this a scratch file. 1 Name this file 'rpac.11' IOp(6/35)WHAT TO DO: 0 Determine attractors, attractor interaction lines, ring points, and cage points. 1 Determine zero-flux surfaces (IDoZrF). 2 Compute charges of AIMs (IDoAtC). 4 Compute kinetic energies and multipole moments of AIMs (IDoPrp). 10 Compute
energies of electrostatic interactions between AIMs (IDoPot). This precludes
100 Compute atomic overlap matrices (IDoAOM). 200 Compute other atomic matrix elements (IDoAMa). 400 Include zero-flux surface relaxation terms in all atomic matrix elements (IDoSRe) 1000 Compute derivatives of
atomic properties with respect to electric field (IDoSeP). 2000 Compute derivatives of
atomic properties with respect to nuclear displacements as 10000 Compute localized orbitals and bond orders (IDoLoc). 20000 Compute atomic orbitals in molecule (IDoAOs). 100000 If necessary, augment valence electron densities with
relativistic core contributions, 200000 If necessary, augment valence electron densities with nonrelativistic core contributions (IHwAug=1). 400000 Abort if pseudopotentials have been used (IHwAug=3). 1000000 Reduce accuracy so atomic charges can be computed
more rapidly (IQuick). No other 2000000 Use numerical instead of analtyic integration. 3000000 Use numerical instead of analtyic integration and use reduced cutoffs. IOp(6/36)CONTROL PARAMETERS FOR NEGLECT OF ORBITALS AND PRIMITIVES in L609: 10000*INoZer+100*IPrNDe+IPrNAt, where INoZer 0: Ignore (spin)orbitals with zero occupancies (default), 1: Do not ignore (spin)orbitals with zero occupancies, IPrNDe Neglect primitive contributions
below 10.**(-IPrNDe) in evaluations of electron IPrNAt Neglect primitive contributions below 10.**(-IPrNAt) in integrations over atomic basins (099, default 7). IOp(6/37)CONTROL PARAMETERS FOR ATINLI, RNGPNT, AND CAGPNT in L609 (NOT TO BE CHANGED UNDER MOST CIRCUMSTANCES): 1000000*MxBpIt+100000*SBpMax+1000*NGrd+LookUp, where MxBpIt Maximum number of iterations in trial path determination (1...99, default 10), SBpMax Maximum value of the control sum (1...9, default 2), NGrd Length of Fourier expansion for the trial path (1...99, default 20), LookUp Number of grid points in critical point search (1...999, default 100). IOp(6/38)CONTROL PARAMETERS FOR ZRFLUX AND OIGAPI in L609 (NOT TO BE CHANGED UNDER MOST CIRCUMSTANCES): 100000*INStRK+10000*IHowFa+1000*IGueDi+100*IPraIn+10*IRScal+IRtFSe INStRK 10*INStRK is the number of steps in the Runge-Kutta integrations along gradient paths (1...9, default 2), IHowFa IHowFa is the maximum distance in the Runge-Kutta integrations along gradient paths (1...9, default 5), IGueDi 10.**(-IGueDi)
is the initial displacement from the critical point in the Runge-Kutta
IPraIn 10.*IPraIn is the cut-off for zero-flux surfaces (1...9, default 2), IRScal IRScal is the scaling factor in the nonlinear transformation used in the intersection search (1...9, default 2), IRtFSe 10.*IRtFSe is the safety factor used in the intersection search (1...9, default 2). IOp(6/39)More CONTROL PARAMETERS FOR ZRFLUX AND OIGAPI in L609 (NOT TO BE CHANGED UNDER MOST CIRCUMSTANCES): 1000000*IToler+100000*INInGr+10000*INInCh+1000*IEpsSf+10*IEpsIn+INTrig IToler 10.**(-5-IToler) is the tolerance for the intersection search (1...9, default 5), INInGr 10*INInGr is the initial
number of grid points in theta and phi in the adaptive integration INInCh 5+INInCh is the initial number of sampling points in the intersection search (1...9, default 2), IEpsSf IEpsSf
is the safety factor used for patches with surface faults in the adaptive
integration IEpsIn 0.0001*IEpsIn is the target for integration error (1...99, default 2), INTrig 10*INTrig is the number of sine and cosine functions in the trial function for surface sheets (1...9, default 2). IOp(6/40)Control of link 607. 0 Default NBO analysis - don't read input. 1 Read input data to control NBO analysis. 2 Delete selected elements of
NBO Fock matrix and form a new density, whose energy can 3 Read the deletion energy produced by a previous run with IOp(40)=2 and print it. IOp(6/41)Number of layers in esp charge fit. 0 Default (4). N N layers, must be >=4. IOp(6/42)Density of points per unit area in esp fit. 0 Default (1). N points per unit area. IOp(6/43)Increment between layers in MK charge fit. 0 Default (0.4/Sqrt(#layers)) N 0.01*N. IOp(6/44)Type of calculation in L604: 0 Default, same as 2. 1 Compute the molar volume 2 Evaluate the density over a cube of points 3 Evaluate MO's over a cube of points 10 Skip header information in cube file. IOp(6/45)Number of points per bohr**3 for Monte-Carlo calaulation of molar volume -1 Read from input 0 Default (20) N N points - for tight accuracy, 50 is recommended. IOp(6/46)Threshold for molecular volume integration. 0 Default - 10**-3 -1 Read from input. N N*10**-4. IOp(6/47)Scale factor to apply to van der Waals radii for the box size during volume integration: 0 Default. N N*0.01 - for debugging. IOp(6/48)Use of cutoffs 0 Default (10**-6 accuracy for cubes, 1 digit better than desired acuracy for volumes). N 10**-N IOp(6/49)Approximate number of points per side in cube in l602/l604: 0 Default (80) N N points -1 Read from cards. -2 Coarse grid, 3 points/Bohr. -3 Medium grid, 6 points/Bohr. -4 Fine grid, 12 points/Bohr. -N>4 Grid using 1000 / N points/Bohr. IOp(6/51)Whether to apply Extended Koopman's Theorem (EKT): 0 Default (No). N Yes, on non-SCF densities, up to N IPs and EAs. -1 Yes, on non-SCF densities, all possible IPs and EAs. -2 No. IOp(6/52)Number of radial integration points in L609: 0 Default (100). N N. IOp(6/53)Distribution of radial points in L609: 0 Default (cubic) N Polynomial of order N. IOp(6/54)Maximum number of domains. 0 Default (100000). N N. IOp(6/55)Number of inner angular points in numerical integration in L609: -1 0 (no inner sphere) 0 302 N N point Lebedev grid (see AngQad). IOp(6/56)Whether to read in density matrix from input stream in L608. 0 No. 1 Yes. IOp(6/57)Whether to generate data over a grid using the total SCF density: 0 No. 1 Yes, read in name for output file. 2 Yes, also read in name for input file with a different grid and compare. 3 Output in the form of data statements. IOp(6/58)Grid to use in generating tables of density and potential. Must be an unpruned grid. 0 Default (99001). IOp(6/59)Approximations to Exc -1 Test superposition of atomic densities using L608: 0 Do correct energies. 1 Do correct energies and 0th order approximation 2 Do correct energies and 0th-1st order approximations 3 Do correct energies and 0th-2nd order approximations IOp(6/60-62)Over-ride standard values of IRadAn, IRanWt, and IRanGd. IOp(6/63)Suppress number of electrons test in XC quadrature in L608 (for debugging with small grids): 0 Default (do test). 1 Suppress test. 2 Do test as usual. IOp(6/64)Natural Chemical Shielding Analysis: 0 No. 1 Yes, of isotropic value. 2 Yes, of diagonal tensor elements and isotropic value. 3 Yes, of all tensor components. IOp(6/65)Threshold for printing of NCS contributions. -1 Zero. 0 Default (1 pmm). N N/1000 ppm IOp(6/70)Control of L610. IOp(6/71)XC functional in L610. IOp(6/72)Whether to read isotopes for hyperfine interractions and do hyperfine terms in L602: 0 Default (1). 1 Yes, if open-shell, NMR data is available, and other terms are being computed 2 No. 3 Yes, regardless of other terms. 4 Yes, reading isotopes IOp(6/73)Whether to save orbitals from NBO: 0 Default (No). 1 Save NBOs in place of regular MOs. 2 Save NLMOs in place of regular MOs. 3 Save NLMO occupieds and NBO virtuals. 10 Suppress re-orthogonalization. IOp(6/74)Whether to use Gaussian connectivity in choosing Lewis structure for NBO. 0 Default (use if present and choose is selected in NBO input). 1 Use. 2 Don't use. IOp(6/75)model for CM2 charges. IOp(6/76)Threshold for linear dependence in L607. 0 Default (1.D-6). N 10**(-N). IOp(6/77)Restraint in charge fitting in L602: 0 None. -1 2.d-4 N N * 10^-5. IOp(6/78)Use MOs instead of density in AtmTab. 0 Default (2). 1 Use density. 2 Use MOs. IOp(6/79)Whether to calculate Hirshfeld charges. 0 Default (No). 1 Yes. 2 No. IOp(6/80)Whether to calculate Lowdin charges and Mayer bond orders. 0 Default (No). 1 Yes. 2 No. IOp(6/81)Print kinetic energy of orbitals? 0 Default (yes, if doing other orbital results). 1 Yes, for the top 5 occupieds and lowest 5 virtuals. 2 No. 3 Yes, for all orbitals. IOp(6/82)Tensors for hyperfine spectra. 0 Default, compute if there are 100 or fewer atoms 1 Compute QEq tensors and for open-shell systems compute isotropic and anisotropic splitting tensors. 2 Do not compute tensors. |