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Phenomenology of $D_{s1}$ mesons radiative transitions

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arxiv 2505.01856 v1 pith:VKWC64KO submitted 2025-05-03 hep-ph hep-ex

classification hep-phhep-ex
keywords mesonsgammaradiativecorrespondingpartialquarksrightarrowsignificantly
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

We discuss radiative transitions $D_{s1}\rightarrow D_s\gamma$ and $D_{s1}\rightarrow D_s^*\gamma$ of $p$-wave mesons. Since $D_{s1}$ mesons have no a certain $C$-parity, and the masses of quarks in these mesons differ significantly, then due to the spin-orbit interaction each of $p$-wave mesons with the total angular momentum $J=1$ is a superposition of states with the total spin of quarks $S_{tot}=0$ and $S_{tot}=1$. We explain why the partial width of $D_{s1}(2460)\to D_s\gamma$ radiative transition is significantly larger than the corresponding value for $D_{s1}(2536)\to D_s\gamma$. We also predict the corresponding partial widths of $B_{s1}$ and $B_{c1}$.

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  1. Relativistic effects in $\mbox{M1}$ radiative decays of heavy-light mesons

    hep-ph 2025-07 conditional novelty 5.0 of 10

    A relativistic potential model, with all parameters taken from meson masses, predicts M1 radiative widths for D and D_s mesons and gives a B_s hyperfine splitting close to the new CMS measurement.

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