Heavy-to-light scalar form factors from Muskhelishvili-Omn\`es dispersion relations
De-Liang Yao, P. Fernandez-Soler, M. Albaladejo, F.-K. Guo, J. Nieves

TL;DR
This paper uses Muskhelishvili-Omnès dispersion relations and chiral symmetry constraints to accurately compute scalar form factors in heavy meson semileptonic decays, fitting to lattice QCD and sum rule data.
Contribution
It introduces a combined dispersive and chiral approach to determine scalar form factors across multiple decay channels, improving CKM element extraction.
Findings
Good simultaneous fit to four decay channels' scalar form factors
Precise determination of CKM matrix elements $|V_{cd}|$, $|V_{cs}|$, and $|V_{ub}|$
Predictions for vector form factors at $q^2=0$ and above
Abstract
By solving the Muskhelishvili-Omn\`es integral equations, the scalar form factors of the semileptonic heavy meson decays , , and are simultaneously studied. As input, we employ unitarized heavy meson-Goldstone boson chiral coupled-channel amplitudes for the energy regions not far from thresholds, while, at high energies, adequate asymptotic conditions are imposed. The scalar form factors are expressed in terms of Omn\`es matrices multiplied by vector polynomials, which contain some undetermined dispersive subtraction constants. We make use of heavy quark and chiral symmetries to constrain these constants, which are fitted to lattice QCD results both in the charm and the bottom sectors, and in this latter sector to the light-cone sum rule predictions close to…
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