Clebsch–Gordan coefficients

Angular momentum operators are self-adjoint operators , , and that satisfy the commutation relations \begin{align} &[\mathrm{j}_k, \mathrm{j}_l] \equiv \mathrm{j}_k \mathrm{j}_l - \mathrm{j}_l \mathrm{j}_k = i \hbar \varepsilon_{klm} \mathrm{j}_m & k, l, m &\in \{ \mathrm{x, y, z}\}, \end{align} where is the Levi-Civita symbol. Together the three operators define a vector operator, a rank one Cartesian tensor operator, \mathbf j = (\mathrm{j_x}, \mathrm{j_y}, \mathrm{j_z}). It is also known as a spherical vector, since it is also a spherical tensor operator. It is only for rank one that spherical tensor operators coincide with the Cartesian tensor operators. By developing this concept further, one can define another operator as the inner product of with itself: \mathbf j^2 = \mathrm{j_x^2} + \mathrm{j_y^2} + \mathrm{j_z^2}. This is an example of a Casimir operator. It is diagonal and its eigenvalue characterizes the particular irreducible representation of the angular momentum algebra \mathfrak{so}(3,\mathbb{R}) \cong \mathfrak{su}(2). This is physically interpreted as the square of the total angular momentum of the states on which the representation acts. One can also define raising () and lowering () operators, the so-called ladder operators, \mathrm {j_\pm} = \mathrm{j_x} \pm i \mathrm{j_y}. == Spherical basis for angular momentum eigenstates ==

It can be shown from the above definitions that commutes with , , and : \begin{align} &[\mathbf j^2, \mathrm {j}_k] = 0 & k &\in \{\mathrm x, \mathrm y, \mathrm z\}. \end{align} When two Hermitian operators commute, a common set of eigenstates exists. Conventionally, and are chosen. From the commutation relations, the possible eigenvalues can be found. These eigenstates are denoted where is the angular momentum quantum number and is the angular momentum projection onto the z-axis. They comprise the spherical basis, are complete, and satisfy the following eigenvalue equations, \begin{align} \mathbf j^2 |j \, m\rangle &= \hbar^2 j (j + 1) |j \, m\rangle, & j &\in \{0, \tfrac{1}{2}, 1, \tfrac{3}{2}, \ldots\} \\ \mathrm{j_z} |j \, m\rangle &= \hbar m |j \, m\rangle, & m &\in \{-j, -j + 1, \ldots, j\}. \end{align} The raising and lowering operators can be used to alter the value of , \mathrm j_\pm |j \, m\rangle = \hbar C_\pm(j, m) |j \, (m \pm 1)\rangle, where the ladder coefficient is given by: {{NumBlk|| C_\pm(j, m) = \sqrt{j (j + 1) - m (m \pm 1)} = \sqrt{(j \mp m)(j \pm m + 1)}. |}} In principle, one may also introduce a (possibly complex) phase factor in the definition of C_\pm(j, m). The choice made in this article is in agreement with the Condon–Shortley phase convention. The angular momentum states are orthogonal (because their eigenvalues with respect to a Hermitian operator are distinct) and are assumed to be normalized, \langle j \, m | j' \, m' \rangle = \delta_{j, j'} \delta_{m, m'}. Here the italicized and denote integer or half-integer angular momentum quantum numbers of a particle or of a system. On the other hand, the roman , , , , , and denote operators. The \delta symbols are Kronecker deltas. == Tensor product space ==

We now consider systems with two physically different angular momenta and . Examples include the spin and the orbital angular momentum of a single electron, or the spins of two electrons, or the orbital angular momenta of two electrons. Mathematically, this means that the angular momentum operators act on a space V_1 of dimension 2j_1+1 and also on a space V_2 of dimension 2j_2 + 1. We are then going to define a family of "total angular momentum" operators acting on the tensor product space V_1 \otimes V_2, which has dimension (2j_1+1)(2j_2+1). The action of the total angular momentum operator on this space constitutes a representation of the SU(2) Lie algebra, but a reducible one. The reduction of this reducible representation into irreducible pieces is the goal of Clebsch–Gordan theory. Let be the -dimensional vector space spanned by the states \begin{align} &|j_1 \, m_1\rangle, & m_1 &\in \{-j_1, -j_1 + 1, \ldots, j_1\} \end{align}, and the -dimensional vector space spanned by the states \begin{align} &|j_2 \, m_2\rangle, & m_2 &\in \{-j_2, -j_2 + 1, \ldots, j_2\} \end{align}. The tensor product of these spaces, , has a -dimensional uncoupled basis |j_1 \, m_1 \, j_2 \, m_2\rangle \equiv |j_1 \, m_1\rangle \otimes |j_2 \, m_2\rangle, \quad m_1 \in \{-j_1, -j_1 + 1, \ldots, j_1\}, \quad m_2 \in \{-j_2, -j_2 + 1, \ldots, j_2\}. Angular momentum operators are defined to act on states in in the following manner: (\mathbf j_1 \otimes 1) |j_1 \, m_1 \, j_2 \, m_2\rangle \equiv \mathbf j_1 |j_1 \, m_1\rangle \otimes |j_2 \, m_2\rangle and (1 \otimes \mathrm \mathbf j_2) |j_1 \, m_1 \, j_2 \, m_2\rangle \equiv |j_1 \, m_1\rangle \otimes \mathbf j_2 |j_2 \, m_2\rangle, where denotes the identity operator. The total angular momentum operators are defined by the coproduct (or tensor product) of the two representations acting on , The total angular momentum operators can be shown to satisfy the very same commutation relations, [\mathrm{J}_k, \mathrm{J}_l] = i \hbar \varepsilon_{k l m} \mathrm{J}_m ~, where . Indeed, the preceding construction is the standard method for constructing an action of a Lie algebra on a tensor product representation. Hence, a set of coupled eigenstates exist for the total angular momentum operator as well, \begin{align} \mathbf{J}^2 |[j_1 \, j_2] \, J \, M\rangle &= \hbar^2 J (J + 1) |[j_1 \, j_2] \, J \, M\rangle \\ \mathrm{J_z} |[j_1 \, j_2] \, J \, M\rangle &= \hbar M |[j_1 \, j_2] \, J \, M\rangle \end{align} for . Note that it is common to omit the part. The total angular momentum quantum number must satisfy the triangular condition that |j_1 - j_2| \leq J \leq j_1 + j_2, such that the three nonnegative integer or half-integer values could correspond to the three sides of a triangle. The total number of total angular momentum eigenstates is necessarily equal to the dimension of : \sum_{J = |j_1 - j_2|}^{j_1 + j_2} (2 J + 1) = (2 j_1 + 1) (2 j_2 + 1) ~. As this computation suggests, the tensor product representation decomposes as the direct sum of one copy of each of the irreducible representations of dimension 2J+1, where J ranges from |j_1 - j_2| to j_1 + j_2 in increments of 1. As an example, consider the tensor product of the three-dimensional representation corresponding to j_1 = 1 with the two-dimensional representation with j_2 = 1/2. The possible values of J are then J = 1/2 and J = 3/2. Thus, the six-dimensional tensor product representation decomposes as the direct sum of a two-dimensional representation and a four-dimensional representation. The goal is now to describe the preceding decomposition explicitly, that is, to explicitly describe basis elements in the tensor product space for each of the component representations that arise. The total angular momentum states form an orthonormal basis of : \left\langle J\, M | J'\, M' \right\rangle = \delta_{J, J'}\delta_{M, M'}~. These rules may be iterated to, e.g., combine doublets (=1/2) to obtain the Clebsch-Gordan decomposition series, (Catalan's triangle), \mathbf{2}^{\otimes n} = \bigoplus_{k=0}^{\lfloor n/2 \rfloor}~ \left(\frac{n + 1 - 2k}{n + 1}{n + 1 \choose k}\right)~(\mathbf{n} + \mathbf{1} - \mathbf{2}\mathbf{k})~, where \lfloor n/2 \rfloor is the integer floor function; and the number preceding the boldface irreducible representation dimensionality () label indicates multiplicity of that representation in the representation reduction. For instance, from this formula, addition of three spin 1/2s yields a spin 3/2 and two spin 1/2s, {\mathbf 2}\otimes{\mathbf 2}\otimes{\mathbf 2} = {\mathbf 4}\oplus{\mathbf 2}\oplus{\mathbf 2}. == Formal definition of Clebsch–Gordan coefficients ==

The coupled states can be expanded via the completeness relation (resolution of identity) in the uncoupled basis {{NumBlk|| |J \, M\rangle = \sum_{m_1 = -j_1}^{j_1} \sum_{m_2 = -j_2}^{j_2} |j_1 \, m_1 \, j_2 \, m_2\rangle \langle j_1 \, m_1 \, j_2 \, m_2 | J \, M\rangle |}} The expansion coefficients \langle j_1 \, m_1 \, j_2 \, m_2 | J \, M \rangle are the Clebsch–Gordan coefficients. Note that some authors write them in a different order such as . Another common notation is . Applying the operators \begin{align} \mathrm J&=\mathrm j \otimes 1+1\otimes\mathrm j \\ \mathrm J_{\mathrm z}&=\mathrm j_{\mathrm z}\otimes 1+1\otimes\mathrm j_{\mathrm z} \end{align} to both sides of the defining equation shows that the Clebsch–Gordan coefficients can only be nonzero when \begin{align} |j_1 - j_2| \leq J &\leq j_1 + j_2 \\ M &= m_1 + m_2. \end{align} == Recursion relations ==

The recursion relations were discovered by physicist Giulio Racah from the Hebrew University of Jerusalem in 1941. Applying the total angular momentum raising and lowering operators \mathrm J_\pm = \mathrm j_\pm \otimes 1 + 1 \otimes \mathrm j_\pm to the left hand side of the defining equation gives \begin{align} \mathrm J_\pm |[j_1 \, j_2] \, J \, M\rangle &= \hbar C_\pm(J, M) |[j_1 \, j_2] \, J \, (M \pm 1)\rangle \\ &= \hbar C_\pm(J, M) \sum_{m_1, m_2} |j_1 \, m_1 \, j_2 \, m_2\rangle \langle j_1 \, m_1 \, j_2 \, m_2 | J \, (M \pm 1)\rangle \end{align} Applying the same operators to the right hand side gives \begin{align} \mathrm J_\pm &\sum_{m_1, m_2} |j_1 \, m_1 \, j_2 \, m_2\rangle \langle j_1 \, m_1 \, j_2 \, m_2 | J \, M\rangle \\ = \hbar &\sum_{m_1, m_2} \Bigl( C_\pm(j_1, m_1) |j_1 \, (m_1 \pm 1) \, j_2 \, m_2\rangle + C_\pm(j_2, m_2) |j_1 \, m_1 \, j_2 \, (m_2 \pm 1)\rangle \Bigr) \langle j_1 \, m_1 \, j_2 \, m_2 | J \, M\rangle \\ = \hbar &\sum_{m_1, m_2} |j_1 \, m_1 \, j_2 \, m_2\rangle \Bigl( C_\pm(j_1, m_1 \mp 1) \langle j_1 \, (m_1 \mp 1) \, j_2 \, m_2 | J \, M\rangle + C_\pm(j_2, m_2 \mp 1) \langle j_1 \, m_1 \, j_2 \, (m_2 \mp 1) | J \, M\rangle \Bigr) . \end{align} Combining these results gives recursion relations for the Clebsch–Gordan coefficients, where was defined in : C_\pm(J, M) \langle j_1 \, m_1 \, j_2 \, m_2 | J \, (M \pm 1)\rangle = C_\pm(j_1, m_1 \mp 1) \langle j_1 \, (m_1 \mp 1) \, j_2 \, m_2 | J \, M\rangle + C_\pm(j_2, m_2 \mp 1) \langle j_1 \, m_1 \, j_2 \, (m_2 \mp 1) | J \, M\rangle. Taking the upper sign with the condition that gives initial recursion relation: 0 = C_+(j_1, m_1 - 1) \langle j_1 \, (m_1 - 1) \, j_2 \, m_2 | J \, J\rangle + C_+(j_2, m_2 - 1) \langle j_1 \, m_1 \, j_2 \, (m_2 - 1) | J \, J\rangle. In the Condon–Shortley phase convention, one adds the constraint that :\langle j_1 \, j_1 \, j_2 \, (J - j_1) | J \, J\rangle > 0 (and is therefore also real). The Clebsch–Gordan coefficients can then be found from these recursion relations. The normalization is fixed by the requirement that the sum of the squares, which equivalent to the requirement that the norm of the state must be one. The lower sign in the recursion relation can be used to find all the Clebsch–Gordan coefficients with . Repeated use of that equation gives all coefficients. This procedure to find the Clebsch–Gordan coefficients shows that they are all real in the Condon–Shortley phase convention. == Explicit expression ==

These are most clearly written down by introducing the alternative notation \langle J \, M | j_1 \, m_1 \, j_2 \, m_2 \rangle \equiv \langle j_1 \, m_1 \, j_2 \, m_2 | J \, M \rangle The first orthogonality relation is \sum_{J = |j_1 - j_2|}^{j_1 + j_2} \sum_{M = -J}^J \langle j_1 \, m_1 \, j_2 \, m_2 | J \, M \rangle \langle J \, M | j_1 \, m_1' \, j_2 \, m_2' \rangle = \langle j_1 \, m_1 \, j_2 \, m_2 | j_1 \, m_1' \, j_2 \, m_2' \rangle = \delta_{m_1, m_1'} \delta_{m_2, m_2'} (derived from the fact that \mathbf 1 = \sum_x |x\rangle \langle x|) and the second one is \sum_{m_1, m_2} \langle J \, M | j_1 \, m_1 \, j_2 \, m_2 \rangle \langle j_1 \, m_1 \, j_2 \, m_2 | J' \, M' \rangle = \langle J \, M | J' \, M' \rangle = \delta_{J, J'} \delta_{M, M'}. == Special cases ==

For the Clebsch–Gordan coefficients are given by \langle j_1 \, m_1 \, j_2 \, m_2 | 0 \, 0 \rangle = \delta_{j_1, j_2} \delta_{m_1, -m_2} \frac{(-1)^{j_1 - m_1}}{\sqrt{2 j_1 + 1}}. For and we have \langle j_1 \, j_1 \, j_2 \, j_2 | (j_1 + j_2) \, (j_1 + j_2) \rangle = 1. For and we have \langle j_1 \, m_1 \, j_1 \, (-m_1) | (2 j_1) \, 0 \rangle = \frac{(2 j_1)!^2}{(j_1 - m_1)! (j_1 + m_1)! \sqrt{(4 j_1)!}}. For we have \langle j_1 \, j_1 \, j_1 \, (-j_1) | J \, 0 \rangle = (2 j_1)! \sqrt{\frac{2 J + 1}{(J + 2 j_1 + 1)! (2 j_1 - J)!}}. For , we have \begin{align} \langle j_1 \, m \, 1 \, 0 | (j_1 + 1) \, m \rangle &= \sqrt{\frac{(j_1 - m + 1) (j_1 + m + 1)}{(2 j_1 + 1) (j_1 + 1)}} \\ \langle j_1 \, m \, 1 \, 0 | j_1 \, m \rangle &= \frac{m}{\sqrt{j_1 (j_1 + 1)}} \\ \langle j_1 \, m \, 1 \, 0 | (j_1 - 1) \, m \rangle &= -\sqrt{\frac{(j_1 - m) (j_1 + m)}{j_1 (2 j_1 + 1)}} \end{align} For we have \begin{align} \left\langle j_1 \, \left( M - \frac{1}{2} \right) \, \frac{1}{2} \, \frac{1}{2} \Bigg| \left( j_1 \pm \frac{1}{2} \right) \, M \right\rangle &= \pm \sqrt{\frac{1}{2} \left( 1 \pm \frac{M}{j_1 + \frac{1}{2}} \right)} \\ \left\langle j_1 \, \left( M + \frac{1}{2} \right) \, \frac{1}{2} \, \left( -\frac{1}{2} \right) \Bigg| \left( j_1 \pm \frac{1}{2} \right) \, M \right\rangle &= \sqrt{\frac{1}{2} \left( 1 \mp \frac{M}{j_1 + \frac{1}{2}} \right)} \end{align} == Symmetry properties ==

\begin{align} \langle j_1 \, m_1 \, j_2 \, m_2 | J \, M \rangle &= (-1)^{j_1 + j_2 - J} \langle j_1 \, (-m_1) \, j_2 \, (-m_2) | J \, (-M)\rangle \\ &= (-1)^{j_1 + j_2 - J} \langle j_2 \, m_2 \, j_1 \, m_1 | J \, M \rangle \\ &= (-1)^{j_1 - m_1} \sqrt{\frac{2 J + 1}{2 j_2 + 1}} \langle j_1 \, m_1 \, J \, (-M)| j_2 \, (-m_2) \rangle \\ &= (-1)^{j_2 + m_2} \sqrt{\frac{2 J + 1}{2 j_1 + 1}} \langle J \, (-M) \, j_2 \, m_2| j_1 \, (-m_1) \rangle \\ &= (-1)^{j_1 - m_1} \sqrt{\frac{2 J + 1}{2 j_2 + 1}} \langle J \, M \, j_1 \, (-m_1) | j_2 \, m_2 \rangle \\ &= (-1)^{j_2 + m_2} \sqrt{\frac{2 J + 1}{2 j_1 + 1}} \langle j_2 \, (-m_2) \, J \, M | j_1 \, m_1 \rangle \end{align} A convenient way to derive these relations is by converting the Clebsch–Gordan coefficients to Wigner 3-j symbols using . The symmetry properties of Wigner 3-j symbols are much simpler. Rules for phase factors Care is needed when simplifying phase factors: a quantum number may be a half-integer rather than an integer, therefore is not necessarily for a given quantum number unless it can be proven to be an integer. Instead, it is replaced by the following weaker rule: (-1)^{4 k} = 1 for any angular-momentum-like quantum number . Nonetheless, a combination of and is always an integer, so the stronger rule applies for these combinations: (-1)^{2 (j_i - m_i)} = 1 This identity also holds if the sign of either or or both is reversed. It is useful to observe that any phase factor for a given pair can be reduced to the canonical form: (-1)^{a j_i + b (j_i - m_i)} where {{math|a ∈ {0, 1, 2, 3}}} and {{math|b ∈ {0, 1}}} (other conventions are possible too). Converting phase factors into this form makes it easy to tell whether two phase factors are equivalent. (Note that this form is only locally canonical: it fails to take into account the rules that govern combinations of pairs such as the one described in the next paragraph.) An additional rule holds for combinations of , , and that are related by a Clebsch-Gordan coefficient or Wigner 3-j symbol: (-1)^{2 (j_1 + j_2 + j_3)} = 1 This identity also holds if the sign of any is reversed, or if any of them are substituted with an instead. == Relation to Wigner 3-j symbols ==

Clebsch–Gordan coefficients are related to Wigner 3-j symbols which have more convenient symmetry relations. {{NumBlk||\begin{align} \langle j_1 \, m_1 \, j_2 \, m_2 | J \, M \rangle &= (-1)^{-j_1 + j_2 - M} \sqrt{2 J + 1} \begin{pmatrix} j_1 & j_2 & J \\ m_1 & m_2 & -M \end{pmatrix} \\ &= (-1)^{2 j_2} (-1)^{J - M} \sqrt{2 J + 1} \begin{pmatrix} j_1 & J & j_2 \\ m_1 & -M & m_2 \end{pmatrix} \end{align}|}} The factor is due to the Condon–Shortley constraint that , while is due to the time-reversed nature of . This allows to reach the general expression: : \begin{align} \langle j_1 \, m_1 \, j_2 \, m_2 | J \, M \rangle & \equiv \delta(m_1+m_2,M) \sqrt{\frac{(2J+1)(j_1+j_2-J)!(j_1-j_2+J)!(-j_1+j_2+J)!}{(j_1+j_2+J+1)!}}\ \times {} \\[6pt] &\times\sqrt{(j_1-m_1)!(j_1+m_1)!(j_2-m_2)!(j_2+m_2)!(J-M)!(J+M)!}\ \times {} \\[6pt] &\times\sum_{k=K}^N \frac{(-1)^k}{k!(j_1+j_2-J-k)!(j_1-m_1-k)!(j_2+m_2-k)!(J-j_2+m_1+k)!(J-j_1-m_2+k)!}, \end{align}. The summation is performed over those integer values for which the argument of each factorial in the denominator is non-negative, i.e. summation limits and are taken equal: the lower one K=\max(0, j_2-J-m_1, j_1-J+m_2), the upper one N=\min(j_1+j_2-J, j_1-m_1, j_2+m_2). Factorials of negative numbers are conventionally taken equal to zero, so that the values of the 3j symbol at, for example, j_3>j_1+j_2 or j_1 are automatically set to zero. == Relation to Wigner D-matrices ==

\begin{align} &\int_0^{2 \pi} d \alpha \int_0^\pi \sin \beta \, d\beta \int_0^{2 \pi} d \gamma \, D^J_{M, K}(\alpha, \beta, \gamma)^* D^{j_1}_{m_1, k_1}(\alpha, \beta, \gamma) D^{j_2}_{m_2, k_2}(\alpha, \beta, \gamma) \\ {}={} &\frac{8 \pi^2}{2 J + 1} \langle j_1 \, m_1 \, j_2 \, m_2 | J \, M \rangle \langle j_1 \, k_1 \, j_2 \, k_2 | J \, K \rangle \end{align} == Relation to spherical harmonics ==

In the case where integers are involved, the coefficients can be related to integrals of spherical harmonics: \int_{4 \pi} Y_{\ell_1}^{m_1}{}^*(\Omega) Y_{\ell_2}^{m_2}{}^*(\Omega) Y_L^M (\Omega) \, d \Omega = \sqrt{\frac{(2 \ell_1 + 1) (2 \ell_2 + 1)}{4 \pi (2 L + 1)}} \langle \ell_1 \, 0 \, \ell_2 \, 0 | L \, 0 \rangle \langle \ell_1 \, m_1 \, \ell_2 \, m_2 | L \, M \rangle It follows from this and orthonormality of the spherical harmonics that CG coefficients are in fact the expansion coefficients of a product of two spherical harmonics in terms of a single spherical harmonic: Y_{\ell_1}^{m_1}(\Omega) Y_{\ell_2}^{m_2}(\Omega) = \sum_{L, M} \sqrt{\frac{(2 \ell_1 + 1) (2 \ell_2 + 1)}{4 \pi (2 L + 1)}} \langle \ell_1 \, 0 \, \ell_2 \, 0 | L \, 0 \rangle \langle \ell_1 \, m_1 \, \ell_2 \, m_2 | L \, M \rangle Y_L^M (\Omega) == Other properties ==

\sum_m (-1)^{j - m} \langle j \, m \, j \, (-m) | J \, 0 \rangle = \delta_{J, 0} \sqrt{2 j + 1} == Clebsch–Gordan coefficients for specific groups ==

For arbitrary groups and their representations, Clebsch–Gordan coefficients are not known in general. However, algorithms to produce Clebsch–Gordan coefficients for the special unitary group SU(n) are known. In particular, SU(3) Clebsch-Gordan coefficients have been computed and tabulated because of their utility in characterizing hadronic decays, where a flavor-SU(3) symmetry exists that relates the up, down, and strange quarks. A web interface for tabulating SU(N) Clebsch–Gordan coefficients is readily available. ==See also==