In quantum mechanics, the action of symmetries on physical states are represented by either linear or, more generally, projective representations. For a particle moving in a crystal without a magnetic field, spatial translations are represented linearly and the corresponding translation operators commute with one another and with the Hamiltonian. However, in the presence of a magnetic field, even when the magnetic field configuration is translationally invariant, wave functions fail to transform linearly under translation. Instead, they are represented projectively, acquiring position-dependent phase factors. The resulting operators are known as magnetic translation operator .
Magnetic Symmetry Operator In this section, we will start with the discussion of the more well-known magnetic translation operator and generalize it to other spatial symmetries such as rotations.
Magnetic Translation Operator To be more specific, consider the Hamiltonian of a quantum particle (with charge q {\displaystyle q} and mass m {\displaystyle m} ) in a magnetic field explicitly depends on the magnetic vector potential A ( r ) {\displaystyle {\bf {A}}({\bf {r}})} , where B = ∇ × A ( r ) {\displaystyle {\bf {B}}=\nabla \times {\bf {A}}({\bf {r}})} :
H = [ p − q A ( r ) ] 2 2 m + V ( r ) {\displaystyle H={\frac {[{\bf {p}}-q{\bf {A}}({\bf {r}})]^{2}}{2m}}+V({\bf {r}})} . For a uniform magnetic field B ( r ) = B z ^ {\displaystyle {\bf {B}}({\bf {r}})=B{\hat {z}}} , the ordinary translation operator T ( a ) = e − i p ⋅ a / ℏ {\displaystyle T({\bf {a}})=e^{-i{\bf {p}}\cdot {\bf {a}}/\hbar }} does not commute with the Hamiltonian even when V ( r + a ) = V ( r ) {\displaystyle V({\bf {r+a}})=V({\bf {r}})} because
T ( a ) − 1 [ p − q A ( r ) ] T ( a ) = p − q A ( r + a ) = p − q A ( r ) − q [ A ( r + a ) − A ( r ) ] = p − q A ( r ) − q ∇ χ a ( r ) . {\displaystyle T({\bf {a}})^{-1}[{\bf {p}}-q{\bf {A}}({\bf {r}})]T({\bf {a}})={\bf {p}}-q{\bf {A}}({\bf {r+a}})={\bf {p}}-q{\bf {A}}({\bf {r}})-q[{\bf {A}}({\bf {r+a}})-{\bf {A}}({\bf {r}})]={\bf {p}}-q{\bf {A}}({\bf {r}})-q\nabla \chi _{\bf {a}}({\bf {r}}).} In the third equality, one writes A ( r + a ) − A ( r ) = ∇ χ a ( r ) {\displaystyle {\bf {A}}({\bf {r+a}})-{\bf {A}}({\bf {r}})=\nabla \chi _{\bf {a}}({\bf {r}})} using the fact that
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