Solving Mandl & Shaw 2.5: Show U = e^(-i/h)δαPα

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Discussion Overview

The discussion centers on demonstrating the unitary transformation associated with spacetime translation of a scalar field as described in Mandl and Shaw problem 2.5. The focus is on the mathematical formulation and manipulation of operators, particularly the energy-momentum 4-vector and its commutation relations.

Discussion Character

  • Technical explanation
  • Mathematical reasoning
  • Debate/contested

Main Points Raised

  • One participant states that the unitary transformation can be expressed as \( U = e^{-(\mathrm{i}/\hbar) \delta_\alpha P^\alpha} \) and suggests using the identity involving the commutator of \( P^\alpha \) and \( U \) to derive the desired result.
  • Another participant proposes using the relation \( U \psi(x) = [U, \psi(x)] + \psi(x) U \) to manipulate the expression for \( U \psi(x) U^\dagger \) and suggests employing the commutation relation \( [P^a, \psi(x)] = -i \hbar \frac{\partial \psi}{\partial x^a} \) to further develop the argument.
  • A different participant expresses uncertainty about the effectiveness of the proposed approach, noting that higher-order terms in the expansion of \( e^{-\mathrm{i}\hbar \delta_\alpha P^\alpha} \) could complicate the derivation.
  • One participant retracts a previous statement, emphasizing that for infinitesimal displacements, higher-order terms may not contribute significantly, and that finite displacements can be achieved by compounding infinitesimal operators.
  • Another participant reiterates the idea that the full Taylor series expansion of \( \varphi(x_\alpha - \delta_\alpha) \) can be derived through commutators, although they acknowledge that the process may become complex.

Areas of Agreement / Disagreement

Participants express varying degrees of confidence in their approaches, with some uncertainty about the implications of higher-order terms and the effectiveness of different mathematical manipulations. No consensus is reached on a definitive method or solution.

Contextual Notes

The discussion involves assumptions about the behavior of operators under infinitesimal transformations and the applicability of Taylor series expansions, which may not be fully resolved within the posts.

jdstokes
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[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.
 
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I think the idea is to use

U \psi \left(x\right) = \left[ U , \psi \left(x\right) \right] + \psi \left(x\right) U

to write

U \psi \left(x\right) U^{\dagger} = \left[ U , \psi \left(x\right) \right] U^\dagger + \psi \left(x\right).

Then use

\left[P^a , \psi \left(x\right) \right] =-i \hbar \frac{\partial \psi}{\partial x^a} \left(x\right)

and the power series expansion of U to work out

\left[ U , \psi \left(x\right) \right].
 
Last edited:
Interesting idea but I'm not sure if it can be made to work,

[P^\alpha,\varphi] = -\mathrm{i}\hbar\partial^\alpha \varphi \implies [P^\alpha P^\beta,\varphi] = -\mathrm{i}\hbar(P^\alpha \partial^\beta\varphi + \partial^\alpha \varphi P^\beta).

Higher terms in the expansion of e^{-\mathrm{i}\hbar \delta_\alpha P^\alpha} contain bigger and bigger versions of this.
 
Scrap that last post, the point is when the displacement is infinitesimal, higher order terms don't contribute. Finite displacements can be obtained by infinitely compounding the infinitesimal operator.
 
jdstokes said:
Scrap that last post, the point is when the displacement is infinitesimal, higher order terms don't contribute. Finite displacements can be obtained by infinitely compounding the infinitesimal operator.

I think that by playing with commutators, the full Taylor series expansion of \varphi(x_\alpha-\delta_\alpha), can be obtained, not just the first two terms of the Taylor series expansion.

In the middle, things probably get somewhat messy, though.
 

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