Molecule Types Linear Molecules | <Prev Next> |
Nucleus | Index, starting from 1, of the nuclear spin involved in perturbation; 0 (the default) for those not involving a nuclear spin. |
SymSelect | Possible values are all
(normal use), e_only
(only affect e
levels) and f_only
(only affect f
levels). Was ParitySelect in previous versions. |
ScalePrev | Scale factor with respect to preceding perturbation |
Op | Perturbation type. See below for possible values. If only
Npower and/or Srank, Scomp are
needed, use Op = Luncouple with n = 0. |
n | Power of operator in perturbation. |
Npower | Power of N (for centrifugal distortion of
perturbation). Perturbation operator is ½[N2,Op]+.
If RSquaredH
is set, N is replaced by R. |
OmegaSelect | Set to all (the default) for normal use; set to a specific value to restrict the perturbation to a specific value of Ω. Note that the current implementation applies the constraint to both connected wavefunctions, so is only useful for ΔΩ = 0 matrix elements. |
Srank | If Srank < 0: adds a
term S±Scomp and changes the power of
J or N. See the Op details below. If Srank > 0: spherical tensor operator for S with overall rank Srank and component Scomp. Note that both of these are only implemented for Op = Luncouple, Suncouple and LNuncouple. |
Scomp |
Value | Size of perturbation. |
LS |
Spin orbit coupling, with the
Ω dependence from the Wigner-Eckart theorem; see for example
Lefebvre-Brion and Field, 2nd Edition Equation 3.4.36: The perturbation parameter is the reduced matrix element arranged so that Λ' > Λ and Λ' > 0 (or S' > S if Λ' = Λ). It is perhaps more normal to quote the value including the 3j symbol, but this is ambiguous when the spin-orbit operator connects more than one component of a pair of states. Some common non-zero values of the 3j symbol are tabulated below.
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Luncouple |
J+nL-n+J-nL+n |
L uncoupling; Using the
default n = 1 this can be used to model the term omitted from the
rotational operator. The perturbation parameter is the value
of the matrix element: for Λ > 0 with the matrix element of L- derived by symmetry If Srank < 0 the operator becomes: J+n+ScompS+-ScompL-n+J-n+ScompS--ScompL+n |
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Suncouple |
J+nS-n+J-nS+n | S uncoupling. (Note that this
term with n = 1 is present in the normal Hamiltonian
within a single vibronic state; it only makes sense to add
it as a perturbation between states.) It checks for ΔΛ = 0
and |ΔΣ| = n, but does not check for ΔS = 0. S is
taken from the Ket. (Note this form is not useful with Srank
< 0). |
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Homog |
Simple homogeneous
perturbation with ΔΩ = 0 selection rule; Use only if one of
the other types is not appropriate. |
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NS |
N.S (n is ignored) |
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RS |
R.S (n is ignored) |
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LNuncouple |
N+nL-n+N-nL+n | Similar to Luncouple, but with J
replaced by N. If Srank < 0 the operator becomes: N+n+ScompS+-ScompL-n+N-n+ScompS--ScompL+n |
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aL |
aI.L |
Nuclear Spin Orbit
perturbation |
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e |
Nuclear magnetic dipole
perturbation |
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eQq1 | Nuclear electric quadrupole perturbation |
Name |
Operator |
Op |
n |
Npower |
Srank |
Scomp |
Scale Factor |
Notes |
B | N2 |
(Luncouple) | 0 | 2 | 0 | 0 | 1 | N2 is replaced by R2 if RSquaredH is set |
D | N4 | (Luncouple) | 0 | 4 | 0 | 0 | -1 | N4 is replaced by R4 if RSquaredH is set |
H | N6 | (Luncouple) | 0 | 6 | 0 | 0 | 1 | N6 is replaced by R6 if RSquaredH is set |
L | N8 | (Luncouple) | 0 | 8 | 0 | 0 | 1 | N8 is replaced by R8 if RSquaredH is set |
M | N10 | (Luncouple) | 0 | 10 | 0 | 0 | 1 | N10 is replaced by R10 if RSquaredH is set |
PP | N12 | (Luncouple) | 0 | 12 | 0 | 0 | 1 | N12 is replaced by R12 if RSquaredH is set |
A | see above |
LS | 1 | 0 | 0 | 0 | Scale factor
calculated to give LzSz
operator form |
|
AD | see above |
LS | 1 | 2 | 0 | 0 | Scale factor calculated to give ½[N2,LzSz]+ operator form | |
gamma | N.S |
NS | 1 | 0 | 0 | 0 | 1 | |
gammaD | ½[N2,N.S]+ | NS | 1 | 2 | 0 | 0 | 1 | N2 (only) is replaced by R2 if RSquaredH is set |
gammaH | ½[N4,N.S]+ | NS | 1 | 4 | 0 | 0 | 1 | N4 (only) is replaced by R4 if RSquaredH is set |
gammaL | ½[N6,N.S]+ | NS | 1 | 6 | 0 | 0 | 1 | N6 (only) is replaced by R6 if RSquaredH is set |
LambdaSS | 6-½(3Sz2-S2) | (Luncouple) | 0 | 0 | 2 |
0 | (8/3)½ | |
LambdaD | ½[N2,6-½(3Sz2-S2)]+ | (Luncouple) | 0 | 2 | 2 |
0 | (8/3)½ | N2 (only) is replaced by R2 if RSquaredH is set |
LambdaH | ½[N4,6-½(3Sz2-S2)]+ | (Luncouple) | 0 | 4 | 2 |
0 | (8/3)½ | N4 (only) is replaced by R4 if RSquaredH is set |
theta | 280-½(35Sz4-20S2Sz2+25Sz2-6S2+3S4) | (Luncouple) | 0 | 0 | 4 |
0 | (35/18)½ |
For all of these operators, the N is replaced by R
if RSquaredH
is set; the N+ and N-
operators are not changed.
Name |
Operator |
Op |
n |
Npower |
Srank |
Scomp |
Scale Factor |
o | S+2L-2+S-2L+2 | LNuncouple | 2 | 0 | -1 | -4 | ½ |
oD | ½[N2,S+2L-2+S-2L+2]+ | LNuncouple | 2 | 2 | -1 | -4 | ½ |
oH | ½[N4,S+2L-2+S-2L+2]+ | LNuncouple | 2 | 4 | -1 | -4 | ½ |
oL | ½[N6,S+2L-2+S-2L+2]+ | LNuncouple | 2 | 6 | -1 | -4 | ½ |
p | N+S+L-2+N-S-L+2 | LNuncouple | 2 | 0 | -1 | -2 | -½ |
pD | ½[N2,N+S+L-2+N-S-L+2]+ | LNuncouple | 2 | 2 | -1 | -2 | -½ |
pH | ½[N4,N+S+L-2+N-S-L+2]+ | LNuncouple | 2 | 4 | -1 | -2 | -½ |
pL | ½[N6,N+S+L-2+N-S-L+2]+ | LNuncouple | 2 | 6 | -1 | -2 | -½ |
q | N+2L-2+N-2L+2 | LNuncouple | 2 | 0 | 0 | 0 | ½ |
qD | ½[N2,N+2L-2+N-2L+2]+ | LNuncouple | 2 | 2 | 0 | 0 | ½ |
qH | ½[N4,N+2L-2+N-2L+2]+ | LNuncouple | 2 | 4 | 0 | 0 | ½ |
qL | ½[N6,N+2L-2+N-2L+2]+ | LNuncouple | 2 | 6 | 0 | 0 | ½ |
A few lambda doubling operators for Δ states are built into
PGOPHER, though note that these use the form involving J
rather than N, and the name is not standard for some of
them. The form involving N can be obtained by replacing Luncouple
with LNuncouple and lambda operators for higher values
of Λ can be obtained by setting n = 2Λ.
Name |
Operator |
Op |
n |
NPower |
Srank |
Scomp |
Scale Factor |
Notes |
o | S+4L-4+S-4L+4 | Luncouple | 4 | 0 | -1 | -8 | ½ | The conventional name would be m |
oD | J+S+3L-4+J-S-3L+4 | Luncouple | 4 | 0 | -1 | -6 | -½ | The conventional name would be n |
oH | J+2S+2L-4+J-2S-2L+4 | Luncouple | 4 | 0 | -1 | -4 | ½ | The conventional name would be o |
p | J+3S+L-4+J-3S-L+4 | Luncouple | 4 | 0 | -1 | -2 | -½ | |
q | J+4L-4+J-4L+4 | Luncouple | 4 | 0 | 0 | 0 | ½ |