jdstokes
- 520
- 1
[SOLVED] Mandl and Shaw 2.5
The question is to show that the unitary transformation corresponding to spacetime translation \delta_\alpha of a scalar field is U = e^{-(\mathrm{i}/\hbar) \delta_\alpha P^\alpha } where P^\alpha is the energy-momentum 4-vector of the field.
\varphi (x) \mapsto \varphi'(x') = \varphi(x_\alpha - \delta_\alpha) = U\varphi(x)U^\dag.
Essentially this boils down to showing that
\varphi(x_\alpha-\delta_\alpha) = U \varphi(x_\alpha)U^\dag.
I'm sure I need to use the identity
[P^\alpha, U] = -\mathrm{i}\hbar\frac{\partial U}{\partial x_\alpha},
but I'm not sure how to contort it into a form that will give me what I want.
The question is to show that the unitary transformation corresponding to spacetime translation \delta_\alpha of a scalar field is U = e^{-(\mathrm{i}/\hbar) \delta_\alpha P^\alpha } where P^\alpha is the energy-momentum 4-vector of the field.
\varphi (x) \mapsto \varphi'(x') = \varphi(x_\alpha - \delta_\alpha) = U\varphi(x)U^\dag.
Essentially this boils down to showing that
\varphi(x_\alpha-\delta_\alpha) = U \varphi(x_\alpha)U^\dag.
I'm sure I need to use the identity
[P^\alpha, U] = -\mathrm{i}\hbar\frac{\partial U}{\partial x_\alpha},
but I'm not sure how to contort it into a form that will give me what I want.