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Theory update

Precision measurements of muon capture by the proton provide a challenging opportunity to test our understanding of chiral symmetry breaking in QCD. In the absence of second class currents, the electroweak structure of a nucleon can be described by four form factors $G_V$, $G_M$, $G_A$, and $G_P$ that determine the matrix elements of the charged vector and axial currents:

$\displaystyle \langle n \vert V_{\mu}^- \vert p \rangle$ $\textstyle =$ $\displaystyle \bar{u}(p_n) \; \left( G_V(q^2) \gamma_{\mu} +
i\frac{G_M(q^2)}{2M_N} \sigma_{\mu\nu} q^{\nu}
\right) \; u(p_p)$ (2)
$\displaystyle \langle n \vert A_{\mu}^- \vert p \rangle$ $\textstyle =$ $\displaystyle \bar{u}(p_n) \; \left( G_A(q^2) \gamma_{\mu}\gamma_5 +
\frac{G_P(q^2)}{2M_N} q_{\mu}\gamma_5
\right) \; u(p_p)$ (3)

where $p_p$ and $p_n$ are the four-momenta of the initial proton and the final neutron, $u(p_p)$ and $u(p_n)$ are the corresponding spinors, $M_N$ is the nucleon mass, and $q=(p_n-p_p)$. Theoretically, the reaction $\mu + p \to \nu_{\mu} + n$ at rest is expected to be well described by effective theory methods, like baryon chiral perturbation theory [4,5,8,9], since the characteristic momentum transfer $q^2 = q_0^2=-0.88 m_{\mu}^2$ is small. While the vector and magnetic form factors are well known from electron scattering data (see [10] and references therein):
$\displaystyle g_V$ $\textstyle =$ $\displaystyle G_V(q_0^2) = 0.9755 \pm 0.0005$ (4)
$\displaystyle g_M$ $\textstyle =$ $\displaystyle G_M(q_0^2) = 3.5821 \pm 0.0025 \quad ,$ (5)

and the axial form factor can be calculated from the nucleon axial coupling constant $g_A=1.2670\pm 0.0035$ [11] and from the nucleon axial charge radius $r_A=(0.65\pm 0.03)\;$fm [4]:
$\displaystyle G_A(q_0^2)$ $\textstyle =$ $\displaystyle 1.245 \pm 0.003 \quad ,$ (6)

the pseudoscalar form factor
$\displaystyle g_P$ $\textstyle =$ $\displaystyle \frac{m_{\mu}}{2M_N} G_P(q_0^2)$ (7)

is experimentally known to much less precision.

The present controversial experimental situation in ordinary (OMC) and radiative (RMC) muon capture is summarized in Fig. 1. The recent RMC result $g_P = 12.2 \pm 0.9 \pm 0.4$ [7] exceeds the theoretical predictions

$\displaystyle g_P$ $\textstyle =$ $\displaystyle \left\{
\begin{array}{ll}
8.44 \pm 0.23 & \cite{ber94} \\
8.21 \pm 0.09 & \cite{fea97}
\end{array}\right.$ (8)

by $4\sigma$. The older OMC results, on the other hand, had the difficult problem of absolute calibration of the neutron detection efficiency.

This was the main reason why they provided measurements of $\Lambda_s$ at the 10% level only. The most accurate measurement with 4.5% precision was performed in Saclay using the lifetime technique in a liquid hydrogen target. At this high density $\mu p$ capture proceeds not only from the free proton, but also from the ortho and para states of the $p\mu p$ molecule. As indicated in Fig. 1 the uncertainty in the transition rate $\lambda_{op}$ between these states leads to a significantly larger error in the interpretation of this measurement.

A recent experiment on $\mu^3\!\mbox{\rm He}$ capture [12] gives $g_p=8.53\pm1.54$ (the accuracy is limited by the theoretical extraction of $g_P$ from the three-nucleon system) in a better agreement with the theoretical values (8).

Theoretically, the dominant contribution to the pseudoscalar form factor is given by the pion pole (PCAC), and the leading correction to the pole term can be derived from QCD Ward identities [4] confirming the old current-algebra result [13]

$\displaystyle G_P(q^2)$ $\textstyle =$ $\displaystyle \frac{4 M_N \; g_{\pi NN} F_{\pi}}{m_{\pi}^2 - q^2} -
\frac{2}{3} g_A(0) M_N^2 r_A^2$ (9)

where $g_{\pi NN}$ is the pion-nucleon coupling constant, and $F_{\pi}$ is the pion decay constant.

Possible corrections to Eq.(9) appear to be small [8,9], however, further theoretical studies are needed in order to conclude whether the relation (9) can be eventually used to determine the $\pi NN$ coupling constant $g_{\pi NN}$ from a precise measurement of $g_P$.

Figure 1: Current constraints on $g_P$ as function of the ortho-para transition rate $\lambda_{OP}$. Experimental results from ordinary muon capture (OMC) [16], radiative muon capture (RMC) [7], and theory (PCAC).
\resizebox*{0.6\textwidth}{0.4\textheight}{\includegraphics{mulop.eps}}

The theoretical calculations of muon capture by the proton were recently reanalyzed in [6], with great care taken to include all known effects and keep approximations to the strictest minimum. The predicted singlet capture rate

$\displaystyle \Lambda_s$ $\textstyle =$ $\displaystyle 688.4 \pm 3.8 \; \mbox{\rm s}^{-1}$ (10)

corresponds to $g_P=8.475\pm 0.076$ calculated with the pion-nucleon coupling constant $g_{\pi NN}=13.37\pm 0.09$ [14].

A significant progress in the understanding of the muon capture in the framework of the low energy effective theory of QCD was made recently by two groups [9,15]. The results of the heavy-baryon chiral perturbation theory (HBChPT) [15] and the small-scale expansion [9] are in a good agreement with the analysis [6] as shown in Table 1.


Table 1: Results of recent calculations of the singlet capture rate $\Lambda_s$
Reference [6] [9] [15]
$\Lambda_s\;\;\mathrm{s}^{-1}$ $688.4 \pm 3.8$ $687.4$ $695$


From the measured singlet capture rate $\Lambda_s$ one can determine a linear combination of the axial and pseudoscalar form factors in a model independent way, as demonstrated in Fig. 2. The ultimate goal of the present experiment is to achieve an accuracy in the $\Lambda_s$ measurement comparable with the present theoretical uncertainties in $g_P$.

Figure 2: The contour plot of the singlet capture rate $\Lambda_s$ as a function of the axial charge $g_A(0)$ and the pseudoscalar form factor $g_P(q^2)$. The bands show the PCAC relation and the present value of $g_A(0)$.
\resizebox*{0.6\textwidth}{0.4\textheight}{\includegraphics{mupgagpmay00.eps}}


next up previous contents
Next: Experimental progress Up: Introduction Previous: Goal and experimental method   Contents
Peter Kammel 2001-02-04