Symmetries

Hibert Space Review

  • $(v,w) \geq 0$, where (a,b) denotes an inner product
    • This is linear in the right argument, and anti-linear in the first argument (ie. take complex conjugates)
    • (v,v) = 0 implies v = 0
  • $v = \Sigma_{i} e_{i} (e_{i}, v)$ always holds in Hilbert spaces (ie. can always decompose into an eigenbasis, where $(e_{i}, e_{j}) = \delta_{ij}$)
    • This can be extended to non-orthonormal bases (ie. $(e_{i}, e_{j}) = G_{ij}$), which implies that $(v,w) = \Sigma_{ij} (v_{i}e_{i})G_{ij}^{-1} (e_{j}, w)$
  • You can add Hilbert spaces of different dimensions together
    • The new Hilbert space has the equivalence relationship of $<v_{1}+v_{2},w_{1}+w_{2}> = <v_{1},w_{1}> + <v_{2},w_{2}>$
    • The total dimensionality of the new Hilbert space is just the sum of the previous two
  • You can also multiply two Hilbert spaces together
    • The equivalence relation which must hold for the product is that $\lambda <v,w> = <\lambda v,w> = <v,\lambda w>$
    • You can decompose this product Hilbert space as a sum of tensor products of the eigenbases of each prior Hilbert space (ie. $H_{prod} = \Sigma_{ia} \Phi_{ia} e_{i} \otimes e_{a}$)

Cannonical Transforms

  • We know that cannonical transformations are an important part of classical Hamiltonian mechanics. What is the analog in quantum?
    • We want the probability to be conserved under a cannonical transformation! (ie. $P(\Phi) = |(\Phi,\Phi)|^{2}$)
    • We also want to preserve linearity (ie. $(\phi_{1}+\phi_{2})’ = \phi_{1}+\phi_{2}$)
    • The only transformations which satisfy these properties are either Unitary or Anti-Unitary (Wigner’s Theorem)

Unitary

  • $U(a\phi+b\psi)= aU\phi + bU\psi$ (can applies either before or after linearity)
  • $UU^{\dag} = I$, where the adjoint of an operator is defined as $(\psi O^{\dag} \phi) = (\phi O \psi)$
  • Needs to be invertible
  • Operator O transforms like $U^{\dag}O U = O'$
    • transform inner product, do adjoint on the left, compare

Anti-Unitary

  • $U(a\phi+b\psi)= a^{*}U\phi + b^{*}U\psi$ (ie. must maintain anti-linearity)
  • $(U\phi, U\psi) = (\psi, \phi) = (\phi, \psi)^{*}$
  • Operators transform like $U^{-1} O U$

Parity

  • Defined as $\Pi^{\dag} \vec{x} \Pi = -\vec{x}$
  • We also define $\Pi* \Pi = 1$, which implies $\Pi = \Pi^{-1}$ and that the eigenstates are $\pm 1$
  • Suppose that $\phi$ is an eigenstate of $\Pi$. Then $(\phi x \phi) = 0$ (Apply parity definition, transfer parity operator to states, apply eigen equation $\Pi \psi = \epsilon \psi$), and then note that you get $-q =q $, which implies q=0
    • As a consequence of this, if you Hamiltonian commutes with parity, then you know that you can write you state as a sum of even and odd states

Time Reversal

  • Time reversal (ie. letting $t \rightarrow -t$) must be described by an anti-unitary operator (otherwise, you get a sea of negative energies)

Rotations

  • Recall that rotation matrices satify $R^{T}R = 1$
  • The set of all rotation matrices for a group (ie. they satisfy group properties)
    • Identity: $\delta_{ij}$
    • The determinant can be $\pm 1$ (plus is called SO(3), minus is called O(3))
  • In the complex plane, we replace Orthogonal, real matrices with unitary matrices
  • For an infinitesimal complex rotation, we can represent a rotation as $U = \approx 1+\frac{i \omega_{ij}}{2}J_{ij}$, where $\omega$ is an anti-symmetric matrix (taken from rotation in real plane) and J is the generator (using Einstein notation for summations)
    • We need this to remain unitary. Using equation $U^{\dag}U=1$ yields that $J_{ij}$ must also be unitary (ie. a unitary peturbation)
    • This also implies that vectors transform like $(1-\frac{\omega_{ij}J_{ij}}{2}) v_{k} (1+\frac{\omega_{ij}J_{ij}}{2}) = v_{k}+\omega_{ij} v_{j}$

Angular Momentum

  • We know that $[J_{i}, J_{j}] = i\epsilon_{ijk} J_{3}$ (fundamental algebra of angular momentum)
    • We also know that we can write $J = L+S$, where L is the angular momentum of the particle, and S is the spin
    • Spin commutes with position and momentum, while angular momentum doesn’t
  • We know that $[J^{2}, J_{i}]=0$ for i=0,1,2. What are the eigenvalues of J?
    • We can define raising and lowering operators $J_{\pm} = J_{1}+iJ_{2}$. We can use these to generate a ladder of eigenstates for $J_{3}$
    • For the z component
      • $J_{3} \psi_{m} = m\psi_{m}$
      • Act raising and lowering operators on both sides, use fundamental commutator to see that $J_{3}(J_{+} \psi_{m}) = m (J_{+} \psi_{m})$ (same for minus)
    • We can rewrite $J^{2} = J_{-}J_{+}+J_{3}+J_{3}^{2}$ (use the fact that $J^{2} = J_{1}^{2}+J_{2}^{2}+J_{3}^{2}$, plus the commutator relationship). acting this onto $\psi$, which is an eigenstate of $J_{z}$ and $J^{2}$ yields $J^{2}\psi = (j+j^{2}) \psi$
      • Acting $J_{\pm}$ on $\psi_{j}$ (eigenstate of $J_{3}$) yields $(j\pm 1) \psi_{j\pm 1}$
    • Similar argument shows that there is a lower bound of j’=-j (can represent $J^{2}$ by swapping plus and minus around, and futzing with the sign of $J_{3}$)
  • What values can j take?
    • We know $J_{3}(J_{+}^{N})\psi_{-j} = (-j+N) \psi_{-j} = -j$, which implies that j must be an integer or a half integer
  • What is the normalization of $J_{\pm}$?
    • $J_{+}\psi_{m} = \alpha(j,m) \psi_{m+1}$
    • Take the norm of this (remembering that $J_{+}^{\dag} = J_{-}$), you can show that $J_{\pm} \psi_{m} = \sqrt{j(j+1)-m^{2}\mp m} \psi_{m \pm 1}$

Clebsch-Gordan Coefficients

  • Suppose that you have some Hilbert space which is a product of n particles, each with their own spin (ie. $\phi(\Sigma_{i}^{n} n_{i}x_{i})$)
  • For simplicity, let’s examine the two particle case. We can decompose the wavefunction like
    • $\psi_{jm}^{j_{1}j_{2}} = \Sigma_{m_{1}m_{2}} C_{j_{1}j_{2}}(j,m; m_{1}m_{2}) \phi_{m_{1}m_{2}}^{j_{1}j_{2}}$
      • In words, we can represent a state of total angular momentum j and total z-spin m as a linear combination of states of definite z-spin m for each hilbert space
    • We have two selection rules on this system:
      • $C_{j_{1}j_{2}}(jm;m_{1},m_{2}) = 0$ if $m_{1}+m_{2}\neq m$
      • $C_{j_{1}j_{2}}(jm;m_{1},m_{2}) = 0$ if $|j_{1}-j_{2}| \leq j \leq j_{1}+j_{2}$
    • You could in theory construct these coefficients via recursion
      • note that $\psi_{jj}^{j_{1}j_{2}} = \psi_{j_{1}j_{2}}^{j_{1}j_{2}}$ for $m=j$ and $m_{1}=j_{1}$ and $m_{2}=j_{2}$ for physical reasons (it’s the only possible way of doing this addition)
      • Imagine that you lower the z angular momentum by 1. The only way this couple happen is if either particle 1 reduces m by 1, or particle 2 reduces m by 1. You can then generate these states and their normalizations via lowering operators.
      • This procedure then recurses: you reason about what states you could generate by changing z angular momentum by 1, then generating their normalizations

Wigner Eckart Theorem

  • Suppose that you have a set of 2j+1 operators $O_{j}^{m}$, with m ranging from -j to j in integer increments
  • Also suppose that this set of operators obeys the angular momemtum commutation relationships:
    • $[J_{3},O_{j}^{m}] = m O_{j}^{m}$
    • $[J_{\pm},O_{j}^{m}] = \sqrt{j(j+1)-m^{2}\mp m} O_{j}^{m}$
  • We want to show that $(\phi_{j’’}^{m’’}O_{j}^{m}\psi_{j’}^{m’}) = C(j’’m’’;j’m’) (\phi || P|| \psi)$
    • This is the Wigner Eckart Theorem. What the hell does it mean?
    • $O_{j}$ is a spherical tensor operator
      • Spherical denotes the fact that we are using a spherical basis of coordinates (think spherical harmonics)
      • Tensor implies that the set of $O_{j}$ transforms like a tensor (ie. applying a rotation on the set just yields a linear combination of the original set)
    • The C are the Clebsch-Gordan coefficients between a given set of spherical harmonics
    • The remaining element is called the reduced matrix element. The important part is that this proportionality factor is independent of m, m’, or which $O_{j}$ you use
  • This allows you to calculate a bunch of matrix elements by only calculating one matrix element, then using the proportionality to “rotate” to another matrix element

Indistinguishable Particles

  • For simplicity, assume that we have two particles, whose total Hamiltonian is $H_{0}=H_{1}+H_{2}$. Naively, we would write the total wavefunction as $\phi_{0} = \phi_{1}\phi_{2}$, but if we have a boson or a fermion, this isn’t invariant under particle swap
    • So, we need to create a more symmetric state: $\Phi = \frac{1}{\sqrt{2}}(\phi_{1}\phi_{2} \pm \phi_{2}\phi_{1})$ where the plus is for bosons and minus is for fermions
    • Calculating the probability density yields that $P = \int d^{3}\vec{x_{1}}d^{3}\vec{x_{2}} |\phi_{1}(x_{1})|^{2}\phi_{2}(x_{2})|^{2}+|\phi_{1}(x_{2})|^{2}\phi_{2}(x_{1})|^{2} \pm 2 Re(\phi_{1}(x_{1})\phi_{2}(x_{2})\phi_{1}^{*}(x_{2})\phi_{2}^{*}(x_{1}))$
      • The last term arises from the bosonic and fermionic interactions
  • To generalize to N particles:
    • Suppose that each particle has it’s own hamiltonian h and wavefunction $\phi$ which satisfy $h e_{\alpha} = E_{\alpha} e_{\alpha}$ and $\phi = \Sigma_{\alpha} \phi_{\alpha} e_{\alpha}$
    • We can write the total hamiltonian of N particles as the sum of each particle’s hamiltonian, and the wavefunction as $\psi = \Sigma \phi_{\alpha_{i}…\alpha_{n}} e_{alpha_{1}} \otimes … e_{alpha_{n}}$
      • If everything was distinguishable, then $\phi_{\alpha_{i}…\alpha_{n}} = \Sigma_{i=1}^{N} \phi_{i}(x_{i})$
    • What is the size of the Hilbert space of we have indistinguishable particles?
      • We go by induction. With 0 particles, we have 1, represented by $\Omega_{\Sigma_{i=1}^{N} n_{i}}$
      • How to we add particles? we define a creation operator $a^{\dag}_{i}$
        • such that a new particle is created in the ith state
      • an anihilation operator such that $a_{i}$ such that a particle is removed from the ith slot. If $n_{i}=0$, then the overall resulting state is 0
      • We can construct the cannonical bosonic commutator relationships
        • $a_{i}a_{j}-a_{j}a_{i} = 0$
        • $a_{i}^{\dag}a_{j}^{\dag}-a_{j}^{\dag}a_{i}^{\dag} = 0$
        • $a_{i}a_{j}^{\dag}-a_{j}^{\dag}a_{i} = \delta_{ij}$
        • We can motivate these by examining $a_{j}a_{i}^{\dag}\Omega = \delta_{ij}$ and $a_{i}^{\dag}a_{j} \Omega =0$
          • We can also define the normalization from these commutators: $a_{i}^{\dag} \Omega_{…n_{i}…} = \sqrt{n_{i}+1} \Omega_{…(n_{i}+1)…}$ and $a_{i} \Omega_{…n_{i}…} = \sqrt{n_{i}} \Omega_{…(n_{i}-1)…}$
      • We can construct an analogous set of anticommutator relationships for the fermions
        • $b_{i}b_{j}+b_{j}b_{i} = b_{i}^{\dag}b_{j}^{\dag}+b_{j}^{\dag}b_{i}^{\dag} = 0$
        • $b_{i}b_{j}^{\dag}+b_{j}^{\dag}b_{i} = \delta_{ij}$