Abstract
We have calculated the photon spectrum and total rate for radiative muon capture in Ca40 using the giant dipole resonance (GDR) model used by Foldy and Walecka to significantly improve theoretical calculations of ordinary muon capture rates. In this model we relate the dipole parts of the nuclear matrix elements relevant for radiative muon capture to integrals over experimental photo-absorption cross sections in the region dominated by the giant dipole resonance. The remaining other multipole and velocity parts of the nuclear matrix elements are evaluated in the closure approximation using harmonic oscillator wave functions. We present numerical results for the photon spectrum as calculated in the GDR model for various values of the weak-interaction coupling constants and of the average maximum photon energy km which is used in the other multipole and velocity parts of the calculation. The most important effect of the GDR calculation is to reduce the dipole contribution to the capture rate, thus giving an absolute radiative rate some 40% lower and a relative rate (ratio of radiative and ordinary rates) some 20% lower than that obtained in the closure-harmonic-oscillator model. As a consequence, the GDR model requires a larger value of the induced pseudoscalar coupling constant gP to reproduce a given spectrum than does the closure-harmonic-oscillator model. Finally, we compare our results with the data of Conversi et al., who found by interpreting their data in the closure-harmonic-oscillator model that gP=(13.3±2.7)gA, where gA is the axial vector coupling constant. We find that the GDR calculation requires gP=(16.5±3.1)gA for a fit to the experiment, where we have assumed km=88 MeV and have taken currently accepted values for the other coupling constants. Alternatively, by taking the Goldberger-Treiman value gP7gA and varying the induced tensor coupling constant gT we obtain a fit to the data for gT35gV. As these results are quire sensitive to km, we give in addition results for other values of km.

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