Real photon emissions in leptonic decays
We present a non-perturbative calculation of the form factors which contribute to the amplitudes for the radiative decays $P\to \ell \bar \nu_\ell \gamma$, where $P$ is a pseudoscalar meson and $\ell$ is a charged lepton. Together with the non-perturbative determination of the virtual photon correct...
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Main Authors: | , , , , , , , , , , , , , |
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Format: | Journal Article |
Language: | English |
Published: |
27-08-2019
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Subjects: | |
Online Access: | Get full text |
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Summary: | We present a non-perturbative calculation of the form factors which
contribute to the amplitudes for the radiative decays $P\to \ell \bar \nu_\ell
\gamma$, where $P$ is a pseudoscalar meson and $\ell$ is a charged lepton.
Together with the non-perturbative determination of the virtual photon
corrections to the processes $P\to \ell \bar \nu_\ell$, this will allow
accurate predictions to be made at $O(\alpha_{em})$ for leptonic decay rates
for pseudoscalar mesons ranging from the pion to the $B$ meson. We are able to
separate unambiguously the point-like contribution, the square of which leads
to the infrared divergence in the decay rate, from the structure dependent,
infrared-safe, terms in the amplitude. The fully non-perturbative, $O(a)$
improved calculation of the inclusive leptonic decay rates will lead to
significantly improved precision in the determination of the corresponding
Cabibbo-Kobayashi-Maskawa (CKM) matrix elements. Precise predictions for the
emission of a hard photon are also very interesting, especially for the decays
of heavy $D$ and $B$ mesons for which currently only model-dependent
predictions are available to compare with existing experimental data. |
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DOI: | 10.48550/arxiv.1908.10160 |