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Abstract

We present a systematic small-$b$ expansion of the Liouville DOZZ three-point structure constant in the light-operator regime $\alpha_i = b\sigma_i$ as $b\to 0$. In this limit, the exact DOZZ function factorizes into a prefactor $\mathcal{P}(b;\sigma_1,\sigma_2,\sigma_3)$ and a power series in $b^2$, \[ C(b\sigma_1,b\sigma_2,b\sigma_3) =\mathcal{P}(b;\sigma_i)\Bigl[1+\sum_{n=1}^\infty b^{2n}\,\Omega_n(\sigma_1,\sigma_2,\sigma_3)\Bigr]. \] Using Thorn's asymptotic expansion of the $\Upsilon_b$-function, we derive closed-form expressions for the leading coefficients $\Omega_n(\sigma_i)$ and show that each $\Omega_n$ is a symmetric polynomial in the variables $\sigma_i$. Our expansion provides explicit perturbative corrections to the semiclassical Liouville three-point function and therefore supplies a practical tool for applications in celestial holography, in particular, for generating loop-level corrections to the tree-level three-gluon scattering amplitude using the inverse Mellin transform. We conclude by outlining these directions for further development. In particular, we highlight that a primary next step is to extend this framework to four-point amplitudes.