Racah's W-coefficients were introduced by Giulio Racah in 1942.[1] These coefficients have a purely mathematical definition. In physics they are used in calculations involving the quantum mechanical description of angular momentum, for example in atomic theory. The coefficients appear when there are three sources of angular momentum in the problem. For example, consider an atom with one electron in an s orbital and one electron in a p orbital. Each electron has electron spin angular momentum and in additionthe p orbital has orbital angular momentum (an s orbital has zero orbital angular momentum). The atom may be described by LS coupling or by jj coupling as explained in the article on angular momentum coupling. The transformation between the wave functions that correspond to these two couplings involves a Racah W-coefficient.
Apart from a phase factor, Racah's W-coefficients are equal to Wigner's 6-j symbols, so any equation involving Racah's W-coefficients may be rewritten using 6-j symbols. This is often advantageous because the symmetry properties of 6-j symbols are easier to remember.
Racah coefficients are related to recoupling coefficients by
W(j1j2Jj3;J12J23)\equiv
\langle(j1,(j2j3)J23)J|((j1j2)J12,j3)J\rangle | |
\sqrt{(2J12+1)(2J23+1) |
Coupling of two angular momenta
j1
j2
J2
Jz
J=j1+j2
|(j1j2)JM\rangle=
j1 | |
\sum | |
m1=-j1 |
j2 | |
\sum | |
m2=-j2 |
|j1m1\rangle|j2m2\rangle\langlej1m1j2m2|JM\rangle,
J=|j1-j2|,\ldots,j1+j2
M=-J,\ldots,J
Coupling of three angular momenta
j1
j2
j3
j1
j2
J12
J12
j3
J
|((j1j2)J12j3)JM\rangle=
J12 | |
\sum | |
M12=-J12 |
j3 | |
\sum | |
m3=-j3 |
|(j1j2)J12M12\rangle|j3m3\rangle\langleJ12M12j3m3|JM\rangle
Alternatively, one may first couple
j2
j3
J23
j1
J23
J
|(j1,(j2j3)J23)JM\rangle=
j1 | |
\sum | |
m1=-j1 |
J23 | |
\sum | |
M23=-J23 |
|j1m1\rangle|(j2j3)J23M23\rangle\langlej1m1J23M23|JM\rangle
Both coupling schemes result in complete orthonormal bases for the
(2j1+1)(2j2+1)(2j3+1)
|j1m1\rangle|j2m2\rangle|j3m3\rangle, m1=-j1,\ldots,j1; m2=-j2,\ldots,j2; m3=-j3,\ldots,j3.
M
|((j1j2)J12j3)JM\rangle=
\sum | |
J23 |
|(j1,(j2j3)J23)JM\rangle \langle(j1,(j2j3)J23)J|((j1j2)J12j3)J\rangle.
M
M=J
J-
|((j1j2)J12j3)JM\rangle=
\sum | |
J23 |
|(j1,(j2j3)J23)JM\rangle W(j1j2Jj3;J12J23)\sqrt{(2J12+1)(2J23+1)}.
Let
\Delta(a,b,c)=[(a+b-c)!(a-b+c)!(-a+b+c)!/(a+b+c+1)!]1/2
W(abcd;ef)=\Delta(a,b,e)\Delta(c,d,e)\Delta(a,c,f)\Delta(b,d,f)w(abcd;ef)
w(abcd;ef)\equiv \sum | ||||||||||
|
\alpha1=a+b+e; \beta1=a+b+c+d;
\alpha2=c+d+e; \beta2=a+d+e+f;
\alpha3=a+c+f; \beta3=b+c+e+f;
\alpha4=b+d+f.
The sum over
z
max(\alpha1,\alpha2,\alpha3,\alpha4)\lez\lemin(\beta1,\beta2,\beta3).
Racah's W-coefficients are related to Wigner's 6-j symbols, which have even more convenient symmetry properties
W(abcd;ef)(-1)a+b+c+d= \begin{Bmatrix} a&b&e\\ d&c&f \end{Bmatrix}.
W(j1j2Jj3;J12J23)=
j1+j2+j3+J | |
(-1) |
\begin{Bmatrix} j1&j2&J12\\ j3&J&J23\end{Bmatrix}.
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