Forbidden Transitions in Linear Molecules
    Strictly the spherical transition
      moments T(k,q) should have selection rules ΔS = ΔΣ = 0, but as an
      extension PGOPHER
      relaxes this requirement and only enforces the |ΔΩ| = q rule for
      ΔS ≠ 0 transitions. This will give some intensity to an otherwise
      forbidden transition but does not give enough flexibility in all
      cases, as several transition moments may be needed. (For exact
      simulations give intensity to the spin forbidden transition by
      using perturbations to mix in transitions to spin allowed states.)
      
    
     For one photon 1Σ - 3Σ
      transitions PGOPHER
      has enough flexibility as only one parallel (q=0) and one perpendicular (q=1) component is required.
      The relative signs of these two are significant and direct
      comparison with the results in the literature requires care; there
      are two definitions for the perpendicular component in use:
    
     J.K.G.Watson, Can J Phys 46, 1637 (1968), equation
      [23]:
    
     μ(1) = 1/√2 < S=0 +- | μ(x) + i μ(y) | S=1, -+, Σ=-1 >
    
    
     μ(perp) = 1/√2 < S=1, -+, Σ=-1 | μ(x) + i μ(y)
      | S=0 +- >
    
    The only difference here is the order, but this is essential to the
    definition. The two are related as follows:
     μ(1) = 1/√2 < 
S=0 +- | μ(x) + i μ(y) | 
S=1, -+, Σ=-1 >
      
 = 1/√2 { < S=0 +- | μ(x) | S=1, -+, Σ=-1 > + i <
        S=0 +- | μ(y) | S=1, -+, Σ=-1 > }
        = 1/√2 { < S=1, -+,
        Σ=-1 | μ(x) | S=0 +-
        >*+ i < S=1, -+,
        Σ=-1 | μ(y) | S=0 +-
        >* }
        = 1/√2 < S=1, -+,
        Σ=-1 | μ(x) - i μ(y) | S=0
        +- >*
        = -1/√2 < S=1, -+,
        Σ=+1 | μ(x) + i μ(y) | S=0
        +- >*
        = -μ(perp)*
      
    
     T(1,1) = -1/√2 < stateA, Ω+1 |
      μ(x) + i μ(y) | stateB, Ω >
    
    with stateA being the state in the bra as shown in the constants
    window. If this is 3Σ we have:
     T(1,1) = -μ(perp) = μ(1)
    
    but if the bra is 1Σ (reversing the states) the
    definition of μ(1) and μ(⊥) does not change but the definition of
    T(1,1) does, giving:
     T(1,1) = μ(perp) = -μ(1)
    
     The difference is because with PGOPHER you can select
      which state is on the left but e.g. Watson's definition always has
      the singlet state on the
      left, and swapping the states over introduces a minus sign. There
      is no such problem with T(1,0) = μ(0) = μ(//).
    
    Note on the definition of the strength parameter.
      For normal transitions, the strength is defined as the value of
      the matrix element:
     <stateA, Λ+q|
      μ | stateB, Λ>
     with the value of the  <stateA, Λ-q| μ | stateB, Λ> matrix
      element derived by symmetry. For forbidden transtions there are
      two symmetry related q = 0 matrix elements; the strength
      parameter is then the value of the matrix element:
    
    <stateA, Λ' Σ'|
      μ | stateB, Λ Σ>
    
    with Λ > 0, or Σ > 0 if Λ = 0. This definition was introduced
    in version 7.1.450, and versions before this gave incorrect values
    for some q = 0 matrix elements.