Calculating Boosted Relativistic Normalization in Quantum Field Theory

In summary: This is a summary of the conversation. In summary, Peskin Schroeder found that the normalization constant for relativistic field theory, δ(p'-q'), is equal to the normalization constant for non-relativistic field theory, δ(p-q), multiplied by the boost in z direction. They computed this by considering on-shell momenta and noting that the measure ##\mathrm{d}^3 p/E## is invariant.
  • #1
abhinavabhatt
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TL;DR Summary
how to compute the Lorentz transformation(Boost along any direction) of Dirac Delta function?
In Quantum field theory by Peskin Schroeder for relativistic normalization
δ(p'-q')=δ(p-q) dp'3/dp3

where the boost is in z direction. How did they compute it?
 

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  • #2
Here, PS consider on-shell momenta, i.e., momenta fulfilling the on-shell condition ##p^2=m^2## or ##E=\sqrt{\vec{p}^2+m^2}##. For these the measure ##\mathrm{d}^3 p/E## is invariant (Lorentz scalar). This implies that the distribution ##E_p \delta^{(3)}(\vec{p}-\vec{q})## is a Lorentz scalar.
 
  • #3
Thanks a lot for your reply.I understand this .Can you tell me how prove it directly using the delta function properties without presuming the invariant measure ?
 
  • #4
It's clear that it's enough to prove it for ##\delta^{(3)}(\vec{p})##. This distribution is for sure invariant under rotations. For boosts you need the assumption that we talk about four-momenta that are onshell, i.e., ##p^0=\sqrt{\vec{p}^2+m^2}##. Then a Lorentz boost with velocity ##\vec{v}## reads
$$\begin {pmatrix} p^{\prime 0} \\ \vec{p}' \end{pmatrix} = \begin{pmatrix} \gamma (p^0-\vec{v} \cdot \vec{p}) \\ \vec{p}+\hat{v} (\gamma-1) (\hat{v} \cdot \vec{p})-\gamma p^0 \vec{v} \end{pmatrix}.$$
From this we get for the Jacobi matrix of the transformation
$$\frac{\partial p_j'}{\partial p_k} = \delta_{jk} + \hat{v}_j \hat{v}_k (\gamma-1)-\gamma p_k/p^0 v_j.$$
Now we have to calculate the determinant of this matrix,
$$J=\mathrm{det} \frac{\partial p_j'}{\partial p_k} = \frac{\gamma (p_0-\vec{p} \cdot \vec{v})}{p_0} =\frac{p_0'}{p_0}.$$
Now from the transformation of the ##\delta## distribution you get
$$\delta^{(3)}(\vec{p}')=\frac{1}{J} \delta^{(3)}(\vec{p})=\frac{p_0}{p_0'} \delta^{(3)}(\vec{p})$$
or
$$p_0' \delta^{(3)}(\vec{p}')=p_0 \delta^{(3)}(\vec{p}).$$
Here ##p_0=E=\sqrt{\vec{p}^2+m^2}## and ##p_0'=E'=\sqrt{\vec{p}{\prime 2}+m^2}## and thus, on the mass shell
$$E' \delta^{(3)}(\vec{p}')=E \delta^{(3)}(\vec{p}),$$
i.e., ##E \delta^{(3)}(\vec{p})## transforms as a scalar field under Lorentz transformations.
 
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  • #5
Thanks a lot for the answer.
 
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1. What is Relativistic Normalization?

Relativistic Normalization is a mathematical concept used in physics to adjust measurements and calculations to account for the effects of relativity.

2. Why is Relativistic Normalization necessary?

Relativistic effects, such as time dilation and length contraction, occur when objects are moving at high speeds. Relativistic Normalization helps to accurately account for these effects in calculations and measurements.

3. How is Relativistic Normalization calculated?

Relativistic Normalization is calculated using the Lorentz factor, which takes into account the velocity and mass of an object. It is often used in equations involving special relativity.

4. Can Relativistic Normalization be applied to all objects?

Yes, Relativistic Normalization can be applied to all objects, as long as they are moving at high speeds. However, the effects may be negligible for objects moving at low speeds.

5. What are some real-world applications of Relativistic Normalization?

Relativistic Normalization is used in various fields of physics, such as astrophysics and particle physics, to accurately describe and predict the behavior of objects moving at high speeds. It is also used in the design and operation of technologies like GPS systems and particle accelerators.

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