Negative square amplitude for a decay process

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SUMMARY

The discussion centers on the computation of the square amplitude ## |\mathcal{M}|^2 ## for a decay process involving Majorana fermions ## \chi_2 ## and ## \chi_1 ##, and a vector boson ## A^{\mu} ##. The interaction is described by the Lagrangian density ## \mathcal{L}_{int} = \frac{ig}{2}( \bar{\chi}_2 \gamma^{\mu} \chi_1 - \bar{\chi}_1 \gamma^{\mu} \chi_2 )A_{\mu} ##. The participant encounters issues leading to a negative square amplitude when assuming the vector boson is massless, indicating a potential error in the calculation of the polarization sums or the treatment of gamma matrices. The discussion references "An Introduction to Quantum Field Theory" by Peskin and Schroeder for conventions and equations.

PREREQUISITES
  • Understanding of Majorana fermions and their properties
  • Familiarity with quantum field theory, particularly Feynman diagrams
  • Knowledge of gamma matrices and their traces
  • Experience with Lagrangian density formulations in particle physics
NEXT STEPS
  • Review the computation of square amplitudes in quantum field theory, specifically in Chapter 5 of "An Introduction to Quantum Field Theory" by Peskin and Schroeder
  • Study the properties and calculations involving Majorana fermions and vector bosons
  • Learn about the implications of negative amplitudes and their physical interpretations
  • Investigate the correct application of polarization sums for massless vector bosons
USEFUL FOR

Particle physicists, graduate students in quantum field theory, and researchers working on decay processes involving Majorana fermions and vector bosons.

simonisr
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Homework Statement


I'm trying to compute the square amplitude ## |\mathcal{M}|^2 ## for a decay process in which a Majorana fermion, call it ## \chi_2 ##, decays into another Majorana fermion, ## \chi_1 ##, and a vector boson denoted by ## A^{\mu} ##. The model is such that the mass of the two fermions differ slightly by a value ## \delta ##, i.e., ## m_2 - m_1 = \delta \ll m_1, m_2 ##, and thus for the decay to be possible we also have that ## m_A < \delta ##. The decay is taken from an interaction term in a Lagrangian density of the form ## \mathcal{L}_{int} = \frac{ig}{2}( \bar{\chi}_2 \gamma^{\mu} \chi_1 - \bar{\chi}_1 \gamma^{\mu} \chi_2 )A_{\mu} ##. I want to compute the square amplitude to tree level, i.e., corresponding to the Feynman diagram simply consisting of one vertex with two external fermions and one external vector boson. I'm using the conventions found in "An Introduction to Quantum Field Theory" by Peskin and Schroeder.

Homework Equations


Equations used throughout my attempted solution, taken from Peskin and Schroeder.

(1) ## \displaystyle\sum_s u^s(p) \bar{u}^s(p) = \gamma_{\mu} p^{\mu} + m ##
(2) ## \displaystyle\sum_{polarizations} \epsilon_{\mu}^*(k) \epsilon_{\nu}(k) \rightarrow - g_{\mu \nu} ##, in the case that the vector boson is massless.
(3) ## \displaystyle\sum_{polarizations} \epsilon_{\mu}^*(k)\epsilon_{\nu}(k) \rightarrow - g_{\mu \nu} + \frac{k_{\mu} k_{\nu}}{m^2} ##, in the case of a vector boson with mass m.
(4) ## Tr(\gamma^{\mu} \gamma^{\nu}) = 4 g^{\mu \nu} ##.
(5) ## Tr(\gamma^{\mu} \gamma^{\nu} \gamma^{\rho} \gamma^{\sigma}) = 4(g^{\mu \nu}g^{\rho \sigma} - g^{\mu \rho}g^{\nu \sigma} + g^{\mu \sigma}g^{\nu \rho}) ##.
(6) Trace of an odd number of gamma matrices yield zero.
(7) ## (\gamma^{\mu})^{\dagger} = \gamma^0 \gamma^{\mu} \gamma^0 ##

The Attempt at a Solution


First I attempt to rewrite the interaction term in a more clear way:
## \mathcal{L}_{int} = \frac{ig}{2}( \bar{\chi}_2 \gamma^{\mu} \chi_1 - \bar{\chi}_1 \gamma^{\mu} \chi_2 )A_{\mu} = \frac{ig}{2}( \chi_2^{\dagger} \gamma^0 \gamma^{\mu} \chi_1 - \bar{\chi}_1 \gamma^{\mu} \chi_2 )A_{\mu} = \frac{ig}{2}( (\chi_1^{\dagger} (\gamma^{\mu})^{\dagger} \gamma^{0} \chi_2 )^{\dagger} - \bar{\chi}_1 \gamma^{\mu} \chi_2 )A_{\mu} \\
= \frac{ig}{2}( (\chi_1^{\dagger} \gamma^{0} \gamma^{\mu} \chi_2 )^{\dagger} - \bar{\chi}_1 \gamma^{\mu} \chi_2 )A_{\mu} = \frac{ig}{2}( (\chi_1^{\dagger} \gamma^{0} \gamma^{\mu} \chi_2 )^* - \bar{\chi}_1 \gamma^{\mu} \chi_2 )A_{\mu} = \frac{ig}{2}( (\bar{\chi}_1 \gamma^{\mu} \chi_2 )^* - \bar{\chi}_1 \gamma^{\mu} \chi_2 )A_{\mu} \\
= \frac{ig}{2} 2i \text{Im}(\bar{\chi}_1 \gamma^{\mu} \chi_2) A_{\mu} = ig \bar{\chi}_1 \gamma^{\mu} \chi_2 A_{\mu} ##
To get the last equality I argue that in the Majorana basis the fields are completely real and the gamma matrices are completely imaginary, and thus the product I'm taking the imaginary part of is a completely imaginary number. This should not depend on the representation of the gamma matrices I'm using so it should be safe to say that the quantity is imaginary and make the replacement.

From this I conclude that the vertex factor for the interaction vertex should be (up to a sign): ## g \gamma^{\mu} ##

Now to the matrix element. I'm a bit lazy about writing out spin indices, but u's carrying the same momenta carry the same spin index.

Let the incoming ## \chi_2 ## fermion have four-momenum ##p##, the outgoing ## \chi_1 ## have four momentum ##q##, and the outgoing vector boson have four-momentum ##k##. We should then get
## i \mathcal{M} = g \bar{u}(q) \gamma^{\mu} u(p) \epsilon_{\mu}^*(k) ## or
## \mathcal{M} = -i g \bar{u}(q) \gamma^{\mu} u(p) \epsilon_{\mu}^*(k) ##.

I compute the complex conjugate of this matrix element, and when doing this we need the following relation.

## (\bar{u}(q)\gamma^{\mu}u(p))^* = \bar{u}(p)\gamma^{\mu}u(q) ##

## \mathcal{M}^* = ig \bar{u}(p) \gamma^{\mu} u(q) \epsilon_{\mu}(k) ##

With this in place I get

## | \mathcal{M} |^2 = g^2 \bar{u}(p) \gamma^{\mu} u(q) \bar{u}(q) \gamma^{\nu} u(p) \epsilon_{\mu}(k) \epsilon_{\nu}^*(k) ##

I then perform the usual spin and polarization sums.

## |\bar{\mathcal{M}}|^2 = \frac{1}{2} \displaystyle\sum_{spins} \displaystyle\sum_{polarizations} |\mathcal{M}|^2 = \frac{g^2}{2} \displaystyle\sum_{spins} \bar{u}(p) \gamma^{\mu} u(q) \bar{u}(q) \gamma^{\nu} u(p) \displaystyle\sum_{polarizations} \epsilon_{\mu}(k) \epsilon_{\nu}^*(k) \\
= \frac{g^2}{2} \text{Tr} [ \gamma^{\mu} (\gamma^{\sigma}q_{\sigma} + m_1) \gamma^{\nu} (\gamma^{\rho} p_{\rho}+m_2) ] T_{\mu \nu} = \frac{g^2}{2}[q_{\sigma} p_{\rho} \text{Tr}(\gamma^{\mu} \gamma^{\sigma} \gamma^{\nu} \gamma^{\rho}) + m_1 m_2 \text{Tr}(\gamma^{\mu} \gamma^{\nu})] T_{\mu \nu} \\
= 2g^2 [ q_{\sigma} p_{\rho} (g^{\mu \sigma}g^{\nu \rho} - g^{\mu \nu}g^{\sigma \rho} + g^{\mu \rho}g^{\sigma \nu}) + m_1 m_2 g^{\mu \nu}] T_{\mu \nu} \\
= 2g^2 (p^{\nu} q^{\mu} + p^{\mu} q^{\nu} - p_{\rho} q^{\rho} g^{\mu \nu} +m_1 m_2 g^{\mu \nu} ) T_{\mu \nu}##

I have made the replacement ## T_{\mu \nu} = \displaystyle\sum_{polarizations} \epsilon_{\mu}(k) \epsilon_{\nu}^*(k) ## to make it look a bit nicer.

Now the solution splits into two, depending on if ## m_A = 0 ## or not.

Assume ## k^2 = m_A^2 ## such that ## T_{\mu \nu} = -g_{\mu \nu} + \frac{k_{\mu} k_{\nu}}{m_A^2} ##. I then get

## |\bar{\mathcal{M}}|^2 = -2g^2 (p^{\nu} q^{\mu} + p^{\mu} q^{\nu} - p_{\rho} q^{\rho} g^{\mu \nu} +m_1 m_2 g^{\mu \nu} ) (g_{\mu \nu} - \frac{k_{\mu} k_{\nu}}{m^2}) \\
= -2g^2 (- p \cdot q + 3 m_1 m_2 - 2 \frac{(p \cdot k)(q \cdot k)}{m_A^2}) \\
= 2g^2 ( p \cdot q - 3 m_1 m_2 + 2 \frac{(p \cdot k)(q \cdot k)}{m_A^2}) \geq 0 ##
This quantity is positive or zero and could be ok, even though some issues arise in the massless limit ## m_A \rightarrow 0##

The really strange stuff happens if I assume that ## k^2 = 0 ## when computing the polarization sum.

Assume ## k^2 = 0 ## such that ## T_{\mu \nu} = -g_{\mu \nu}##. I then get.

## |\bar{\mathcal{M}}|^2 = -2g^2 (p^{\nu} q^{\mu} + p^{\mu} q^{\nu} - p_{\rho} q^{\rho} g^{\mu \nu} +m_1 m_2 g^{\mu \nu} ) g_{\mu \nu} \\
= -2 g^2 (2 p \cdot q - 4 p \cdot q + 4 m_1 m_2) \\
= 4 g^2 (p \cdot q - 2 m_1 m_2) < 0 ##
This does not make any sense at all. I've computed the absolute square of a complex number and obtained something which is negative. I have tried to figure out my error for quite a while now but I cannot seem to find it. I would be very grateful if anyone could point me in the right direction.
 
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Most of the calculations in Peskin and Schroeder are quite advanced=I have the book, but I am hardly competent with any of it. In any case, I think I see an error that you made. When you wrote out ## |\bar{M} |^2 ##, in two places, you have separate ## \mu ## and ## \nu ## superscripts and subscripts (on the ## \gamma ## terms and on the ## \epsilon ## terms), when these need to be the same (e.g. both ## \mu ## ). ## \\ ## Editing: And then again, I'm not so sure about what I just mentioned, because the ## \mu ## looks like it gets repeated for both ## M ## and ## M^* ##. Each term has the form: ## \gamma^{\mu} \epsilon_{\mu} ##, (with a sum over ## \mu ##). Instead, I think, because of this, you need to take care in how the ## \gamma^{\mu} \gamma^{\nu} ## and ## \epsilon_{\mu} \epsilon_{\nu} ## get combined, and I'm not sure that they can get separated and grouped in the manner that you did. ## \\ ## Additional editing: On further study, I think what you have for this ## \mu ## and ## \nu ## is correct. I'll keep looking to see if something else might appear... ## \\ ## Suggestion is to review the first couple of pages of Chapter 5 which are found on pp.131-133 of my copy of the book. There they discuss how to compute ## |M|^2 ## and a couple of tricks that simplify the calculation.
 
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