High School In Fermi V-A theory, where does the Weak Interaction occur

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SUMMARY

The discussion centers on the Weak Interaction in Fermi V-A theory, specifically regarding the electron-nucleon interaction's location—either at the nucleus's surface or at the origin. The Weak Interaction Hamiltonian is defined as \(\mathcal{H}(x)=-\dfrac{G_{F}}{\sqrt{2}}\left[J^{\mu}(x)L^{+}_{\mu}(x)+h.c.\right]\), where \(J^{\mu}\) and \(L_{\mu}\) represent Hadron and Lepton currents, respectively. The evaluation of invariant matrix elements is crucial for understanding weak processes like Electron Capture, which involves calculating electron density at the origin versus the surface of the nucleus. The discussion references the nuclear radius estimation formula \(R\sim A^{\frac{1}{3}}\) and highlights the complexities in defining proton radius through various measurement contexts.

PREREQUISITES
  • Understanding of Fermi V-A theory and its implications in particle physics.
  • Familiarity with Lagrangian density and Hamiltonian formalism in quantum field theory.
  • Knowledge of weak interactions and their role in nuclear processes.
  • Basic concepts of nuclear radius estimation and electron scattering techniques.
NEXT STEPS
  • Study the derivation and implications of the Weak Interaction Hamiltonian in particle physics.
  • Explore the methods for calculating invariant matrix elements in quantum field theory.
  • Investigate the discrepancies in proton radius measurements, particularly in muonic atoms.
  • Review the section on finite nuclear radius in Akhiezer and Berestetskii's book on Quantum Electrodynamics.
USEFUL FOR

Physicists, particularly those specializing in particle physics, nuclear physics, and quantum field theory, will benefit from this discussion, as well as researchers exploring weak interactions and their experimental measurements.

charlesmartin14
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Where is the electron-nucleon interaction? On the surface of the nucleus, or at the origin (R-0) ?
 
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Can you write down the interaction term or, even better the whole, Lagrangian density?
 
The Lagrangian contains a 'contact potential' , which Fermi assumed is a contact coupling of two vector currents. (prior to when parity breaking was discovered. This is now part of the Standard Model, in some cryptic form.

IMHO, you can not see it obviously in the Lagrangian until you specify the Dirac Spinors explicitly and evaluate the invariant matrix elements The Weak Interaction Hamiltonian element is

\mathcal{H}(x)=-\dfrac{G_{F}}{\sqrt{2}}\left[J^{\mu}(x)L^{+}_{\mu}(x)+h.c.\right]where

J^{\mu} and L_{\mu}

are (in modern parlance) the Hadron and Lepton currents, resp.,

The question is really how to evaluate the invariant matrix element -- at the surface of the nucleus, or at the origin ? That is, say, given some expression that appears in a cross section or a rate

\sum_{fi}\big\vert\mathcal{M}_{fi}\left[p_{ep}\rightarrow i\nabla)\right]\psi_{ep}(\mathbf{x})\big\vert_{\mathbf{x}=0}\big\vert^{2}

or would we compute the electron density at the surface ?

for example, we do compute the rate of Electron Capture , a typical weak process, we can write the capture rate as

\Gamma_{EC}=\big\vert\Psi_{ep}(0)\big\vert^{2}\mathbf{v}^{in}_{ep}\sigma_{EC}

where \big\vert\Psi_{ep}(0)\big\vert^{2} is the electron density at the origin, representing the nuclear charge.

Or , again, should this be the charge on the surface of the nucleus ?
 
How would you define the „surface of the nucleus”?
 
Whatever the experimentalists tell me their best estimate it.
The nuclear radius can be estimated using a simple formula

R\sim A^{\frac{1}{3}}

where A is the Atomic mass number.

I am asking how the Fermi VA theory is typically used in very detailed calculations.
 
Me neither, I have only seen a „finite nuclear radius” hypothesis only in a Dirac equation context (as a perturbative effect). AFAIK, it was described only in section 13.4 of Akhiezer and Berestetskiis book on QED. A finite nuclear hypothesis in case of a weak coupling is not known to me.
 
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Fermi theory is an effective low-energy theory which treats the nucleons as elementary fields.

To define a "proton radius" you need a context, how you measure it. One way is to use electron scattering, defining a charge radius. Another way is to consider the fine structure of the atomic hydrogen transition lines, also defining a charge radius. There's some "crisis" there, because measuring the charge radius with the transitions in muonic atoms, you get a different (smaller result). For a review, see this recent talk from our Nuclear Physics Colloquium:

http://th.physik.uni-frankfurt.de/~hees/np-colloquium/ss17/talk-gao.pdf
 

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