Neutrino-neutrino to WW amplitude via Z-exchange

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Homework Statement



I am working through an example in Chapter 6 of Quigg's Gauge Theories. I have it mostly figured out, with the exception of how to work out the S^{\mu}S^{\nu} term. All he writes is "...the term is impotent between massless spinors."

Homework Equations


I begin with:

nunu_WW_amplitude.png


What I want to know is how to obtain the factors that include S:

result.png


The Attempt at a Solution


I have all of the terms except those which include S. An explicit calculation or explanation would be extremely appreciated!

[Edit] I will show my work to point out where I am stuck.

I worked out the term involving g^{\mu\nu}. After the contraction of \gamma_\nu g^{\mu\nu}, the polarization vectors contract with the terms in square brackets to give:

\epsilon_+^{*\alpha}\epsilon_-^{*\beta}[...] = \epsilon_+^{*} \cdot \epsilon_-^{*} (k_- - k_+)_{\nu} + \epsilon_-^{*} \cdot k_+ \epsilon_{+\nu}^* - \epsilon_+^* \cdot k_- \epsilon_{-\nu}^* [1]

My understanding is that the S^{\mu}S^{\nu} will act on [1] above, but I do not see how to get the desired result. I thought that the contravariant S^{\nu} term would contract with the covariants, but instead somehow the k_+ and k_- in the second and third terms of [1] above are replaced by S. Either this is something I do not quite get, or I am being foolish.blankvin
 
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Are you just looking for the amplitude?
 
saybrook1 said:
Are you just looking for the amplitude?

I know what the amplitude is. It is how to deal with the S^{\mu}S^{\nu} that I do not know.blankvin
 
Yeah sorry, the first time I saw your post I was on mobile. I will check back on it when I have time if you haven't received a response yet.
 
I figured it out.

Working out the S^{\mu}S^{\nu} terms lead to zero contribution to the amplitude.

This blunder will be blamed on fatigue.blankvin
 
To solve this, I first used the units to work out that a= m* a/m, i.e. t=z/λ. This would allow you to determine the time duration within an interval section by section and then add this to the previous ones to obtain the age of the respective layer. However, this would require a constant thickness per year for each interval. However, since this is most likely not the case, my next consideration was that the age must be the integral of a 1/λ(z) function, which I cannot model.
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