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Chapter 12 The weak interactions of leptons

Lepton universality

Within the accuracy of the experimental measurements, it can be concluded that $G^{(e)}_F = G^{(\mu)}_F = G^{(\tau)}_F$, providing strong experimental evidence for the lepton universality of the weak charged current; there is a universal coupling strength at the $Weν_e$, $Wμν_μ$ and $Wτν_τ$ interaction vertices.

Neutrino scattering

Let’s consider the deep inelastic interaction with neutrinos and partons.

Neutrino-quark scattering cross section

image-20250904103132598

With $Q^2 \ll m_W^2$, we have

\[M = \frac{g_W^2}{2}\cdot \left[ \bar u(p_3)\gamma^\mu P_Lu(p_1)\right]\cdot \frac{g_{\mu\nu}}{m_W^2}\cdot \left[ \bar u(p_4)\gamma^\mu P_L u(p_2)\right]\]

In the center-of-mass frame, we have (Chapter 4)

\[u_\uparrow =N \begin{bmatrix} c\\ s \mathrm e ^{\mathrm i \phi}\\ c\\ s \mathrm e ^{\mathrm i \phi}\\ \end{bmatrix}, \quad u_\downarrow =N \begin{bmatrix} -s\\ c \mathrm e ^{\mathrm i \phi}\\ s\\ -c \mathrm e ^{\mathrm i \phi}\\ \end{bmatrix},\quad v_\uparrow =N \begin{bmatrix} s\\ - c \mathrm e ^{\mathrm i \phi}\\ -s\\ c \mathrm e ^{\mathrm i \phi}\\ \end{bmatrix}, \quad v_\downarrow =N \begin{bmatrix} c\\ s \mathrm e ^{\mathrm i \phi}\\ c\\ s \mathrm e ^{\mathrm i \phi}\\ \end{bmatrix}\]

Apparently only the LH charity states give the non-zero results, therefore:

\[u_\downarrow(p_1) = \sqrt E \begin{bmatrix} 0\\ 1\\ 0\\ -1 \end{bmatrix},\quad u_\downarrow(p_2) = \sqrt E \begin{bmatrix} -1\\ 0\\ 1\\ 0 \end{bmatrix}, \quad u_\downarrow(p_3) = \sqrt E \begin{bmatrix} -s\\ c\\ s\\ -c \end{bmatrix}, \quad u_\downarrow(p_4) = \sqrt E \begin{bmatrix} -c\\ -s\\ c\\ s \end{bmatrix}\]

where $c = \cos \frac{\theta^{\ast}}{2}, s = \sin\frac{\theta^{\ast}}{2}$, and $\theta^{\ast}$ denotes the angle of z-axis in the center-of-mass frame.

Thus

\[j_l^\mu = \bar u(p_3)\gamma^\mu P_Lu(p_1) = \bar u(p_3)\gamma^\mu u(p_1) = 2E(c, s, -\mathrm is , c)\\ j_q^\nu = \bar u(p_4)\gamma^\mu P_L u(p_2) = 2E(c, -s, -\mathrm i s, -c)\] \[M = \frac{g_W^2}{2}\cdot j_l^\mu\cdot \frac{g_{\mu\nu}}{m_W^2}\cdot j_q^\nu = \frac{2g_W^2E^2}{m_W^2}(c^2+s^2+s^2+c^2) = \frac{4g_W^2E^2}{m_W^2} = \frac{g_W^2s^*}{m_W^2}\]

where $s^* = 2E$.

Because both the quark and neutrino are left-handed, the interaction occurs in an $S_z = 0$ state and thus there is no preferred polar angle in the center-of-mass frame.

As for the cross section,

\[\frac{\mathrm d \sigma}{\mathrm d \Omega^*} =\frac{1}{64\pi^2s^*}\langle|M_{fi}|^2\rangle\]

where

\[\langle|M_{fi}|^2\rangle = \frac 1 2 \left(\frac{g_W^2s^*}{m_W^2}\right)^2\]

Thus

\[\frac{\mathrm d \sigma_{\nu q}}{\mathrm d \Omega^*} =\frac{1}{64\pi^2s^*}\langle|M_{fi}|^2\rangle =\left(\frac{g_W^2}{8\sqrt 2\pi m_W^2}\right)^2 s^* = \frac {G_F^2}{4\pi^2}s^*\]

And

\[\sigma_{\nu q} = \frac {G_F^2}{\pi}s^*\]

Antineutrino-quark scattering

image-20250904111050167

\[M = \frac{g_W^2}{2}\cdot \left[ \bar v(p_3)\gamma^\mu P_Lv(p_1)\right]\cdot \frac{g_{\mu\nu}}{m_W^2}\cdot \left[ \bar u(p_4)\gamma^\mu P_L u(p_2)\right] \\ = \frac{g_W^2}{2}\cdot \left[ \bar v_\uparrow(p_3)\gamma^\mu v_\uparrow(p_1)\right]\cdot \frac{g_{\mu\nu}}{m_W^2}\cdot \left[ \bar u_\downarrow(p_4) \gamma^\mu u_\downarrow(p_2)\right]\] \[v_\uparrow(p_1) = \sqrt E \begin{bmatrix} 0\\ -1\\ 0\\ 1 \end{bmatrix},\quad u_\downarrow(p_2) = \sqrt E \begin{bmatrix} -1\\ 0\\ 1\\ 0 \end{bmatrix}, \quad v_\uparrow(p_3) = \sqrt E \begin{bmatrix} s\\ -c\\ -s\\ c \end{bmatrix}, \quad u_\downarrow(p_4) = \sqrt E \begin{bmatrix} -c\\ -s\\ c\\ s \end{bmatrix}\] \[j_l^\mu = \bar v(p_1)\gamma^\mu v(p_3) = 2E(c, s, \mathrm is , c)\\ j_q^\nu = \bar u(p_4)\gamma^\mu u(p_2) = 2E(c, -s, -\mathrm i s, -c)\] \[M = \frac{g_W^2}{2}\cdot j_l^\mu \cdot \frac{g_{\mu\nu}}{m_W^2}\cdot j_q^\nu = \frac{g_W^2s^*}{2m_W^2}\cdot 2\cos^2\frac{\theta^*}{2} = \frac{g_W^2s^*}{2m_W^2} (1+\cos\theta^*)\]

The origin of this difference can be understood in terms of spins of the particles. The $V - A$ nature of the weak interaction means that the $\bar \nu q$ interaction occurs in an $S_z = 1$ state and this results in an angular dependence of the matrix element of $\frac 1 2 (1 + \cos \theta^*)$.

\[\langle|M_{fi}|^2\rangle = \frac 1 2 \left(\frac{g_W^2s^*}{m_W^2}\right)^2\cdot \frac 1 4 (1+\cos\theta^*)^2\] \[\frac{\mathrm d \sigma_{\bar \nu q}}{\mathrm d \Omega^*} = \frac{1}{64\pi^2s^*}\langle|M_{fi}|^2\rangle =\left(\frac{g_W^2}{8\sqrt 2\pi m_W^2}\right)^2 s^* \cdot \frac 1 4 (1+\cos\theta^*)^2 = \frac {G_F^2}{4\pi^2}s^*\cdot \frac 1 4 (1+\cos\theta^*)^2\] \[\sigma_{\bar \nu q} =\frac {G_F^2}{3\pi}s^*\]

image-20250904113736232

Neutrino–nucleon differential cross sections

The Lorentz invariant form of differential cross section:

\[y = \frac{p_2\cdot q}{p_2\cdot p_1} = \frac{p_2\cdot (p_1-p_3)}{p_2\cdot p_1}\]

where

\[p_1 = (E, 0, 0 ,E)\\ p_2 = (E, 0, 0, -E)\\ p_3 = (E, E\sin\theta^*, 0, E\cos\theta^*)\] \[y = \frac12(1-\cos\theta^*)\]

Therefore

\[\frac{\mathrm d \sigma_{\nu q}}{\mathrm d y} =\frac{\mathrm d \sigma_{\nu q}}{\mathrm d \Omega^*}\left|\frac{\mathrm d \Omega^*}{\mathrm d y}\right| = \frac{G_F^2}{4\pi^2}s^*\cdot 4\pi = \frac {G_F^2}{\pi}s^*\]

and

\[\frac{\mathrm d \sigma_{\bar \nu q}}{\mathrm d y} =\frac{\mathrm d \sigma_{\nu q}}{\mathrm d \Omega^*}\left|\frac{\mathrm d \Omega^*}{\mathrm d y}\right| = \frac{G_F^2}{4\pi^2}s^*\cdot \frac 1 4 (1+\cos\theta^*)^2\cdot 4\pi = \frac {G_F^2}{\pi}(1-y)^2 s^*\]

Neutrino deep inelastic scattering

Let’s integregate the neutrino-quark interaction calculation into Feynman’s parton model.

\[\frac{\mathrm d \sigma_{\nu p}}{\mathrm d y_q}=\frac {G_F^2}{\pi}s^*\cdot (d(x)+(1-y_q^2)\bar u(x))\mathrm d x\]

where

\[s^* = (p_1+xp_2)^2 = xs\]

and

\[y_q = \frac{x p_2\cdot q}{p_1\cdot xp_2} = y\]

i.e.,

\[\frac{\mathrm d \sigma_{\nu p}}{\mathrm d x\mathrm d y}=\frac {G_F^2}{\pi}sx(d(x)+(1-y)^2\bar u(x))\]

Analogously

\[\frac{\mathrm d \sigma_{\bar \nu p}}{\mathrm d x\mathrm d y}=\frac {G_F^2}{\pi}sx(u(x)+(1-y)^2\bar d(x))\]

and

\[\frac{\mathrm d \sigma_{\nu n}}{\mathrm d x\mathrm d y}=\frac {G_F^2}{\pi}sx(u(x)+(1-y)^2\bar d(x))\] \[\frac{\mathrm d \sigma_{\bar \nu n}}{\mathrm d x\mathrm d y}=\frac {G_F^2}{\pi}sx(d(x)+(1-y)^2\bar u(x))\]

due to the symmetry of proton ande neutron.

For nucleur $N$ with the same number of protons and neutrons, we have

\[\frac{\mathrm d^2 \sigma_{\nu N}}{\mathrm d x\mathrm d y}=\frac 1 2\left(\frac{\mathrm d \sigma_{\nu p}}{\mathrm d x\mathrm d y}+\frac{\mathrm d \sigma_{\nu n}}{\mathrm d x\mathrm d y}\right)=\frac {G_F^2m_N}{\pi}E_{\nu}x[u(x)+d(x)+(1-y)^2(\bar u(x)+\bar d(x))]\]

And

\[\frac{\mathrm d \sigma_{\nu N}}{\mathrm d y}=\frac 1 2\left(\frac{\mathrm d \sigma_{\nu p}}{\mathrm d x\mathrm d y}+\frac{\mathrm d \sigma_{\nu n}}{\mathrm d x\mathrm d y}\right)=\frac {G_F^2m_N}{\pi}E_{\nu}[f_q+(1-y)^2f_{\bar q}]\]

where $f_q$ represents the intergral of x, same as the other f-term.

Neutrino scattering experiments


(TO BE CONTINUED)


Structure functions in neutrino interactions

For QED deep inelastic interaction, we have

\[\frac{\mathrm d \sigma}{\mathrm d x\mathrm dy} = \frac{4\pi\alpha^2s}{Q^4}\left[\left(1-y\right){F_2(x, Q^2)}+xy^2 F_1(x, Q^2)\right]\]

For weak interaction, we have the structure function

\[\frac{\mathrm d \sigma}{\mathrm d x\mathrm dy} = \frac{G_F^2s}{2\pi}\left[\left(1-y\right){F_2(x, Q^2)}+xy^2 F_1(x, Q^2)+y(1-\frac y 2)xF_3(x, Q^2)\right]\]

According to parton model for proton,

\[F_2 = 2xF_1 = 2x(d(x)+\bar u(x))\\ F_3 = 2(d(x)-\bar u(x))\]

Charged-current electron–proton scattering


(TO BE CONTINUED)