Kleinman symmetry, named after American physicist D.A. Kleinman, gives a method of reducing the number of distinct coefficients in the rank-3 second order nonlinear optical susceptibility when the applied frequencies are much smaller than any resonant frequencies.[1]
Assuming an instantaneous response we can consider the second order polarisation to be given by
P(t)=\epsilon0\chi(2)E2(t)
E
For a lossless medium with spatial indices
i,j,k
(2) | |
\chi | |
ijk |
(\omega3;\omega1+\omega2)=
(2) | |
\chi | |
jki |
(\omega1;-\omega2+\omega3)=
(2) | |
\chi | |
kij |
(\omega2;\omega3-\omega1) =
(2) | |
\chi | |
ikj |
(\omega3;\omega2+\omega1)=
(2) | |
\chi | |
kji |
(\omega2;-\omega1+\omega3) =
(2) | |
\chi | |
jik |
(\omega1;\omega3-\omega2)
In the regime where all frequencies
\omegai\ll\omega0
\omega0
This is the Kleinman symmetry condition.
Kleinman symmetry in general is too strong a condition to impose, however it is useful for certain cases like in second harmonic generation (SHG). Here, it is always possible to permute the last two indices, meaning it is convenient to use the contracted notation
dil=
1 | |
2 |
(2) | |
\chi | |
ijk |
(\omega3;\omega1,\omega2)
which is a 3x6 rank-2 tensor where the index
l
Note that for processes other than SHG there may be further, or fewer reduction of the number of terms required to fully describe the second order polarisation response.