arXiv · hep-ph/9509361
$c\to u γ$ in Cabibbo suppressed D meson radiative weak decays
Abstract
We investigate Cabibbo suppressed $D^{0}$, $D^{+}$ and $D^{+}_{s}$ radiative weak decays in order to find the best mode to test $c\to u γ$ decay. Combining heavy quark effective theory and the chiral Lagrangian approach we determine the decay widths. We calculate $Γ(D^{0}\to ρ^{0}/ωγ)/ Γ(D^{0}\to {\bar K}^{*0} γ)$ previously proposed to search for possible New Physics. However, we notice that there are large, unknown, corrections within the Standard Model. We propose a better alternative, the ratio $Γ(D_{s}^{+}\to K^{*+} γ)/ Γ(D_{s}^{+}\to ρ^{+} γ)$, and show that it is less sensitive to the Standard Model.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
B. Bajc, S. Fajfer, R. J. Oakes. 1995-09-22. $c\to u γ$ in Cabibbo suppressed D meson radiative weak decays. https://doi.org/10.1103/physrevd.54.5883
Cite the original work for its findings. Save a collection to share your selection of sources.