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Anatomy of Family Trees in Cosmological Correlators

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arxiv 2509.02684 v1 pith:XXSSSQWL submitted 2025-09-02 hep-th astro-ph.COhep-ph

Anatomy of Family Trees in Cosmological Correlators

classification hep-th astro-ph.COhep-ph
keywords familytreesanalyticalcorrelatorscosmologicalsingularitiesintegralsparameters
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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The time-ordered multilayer integrals have long been cited as major challenges in the analytical study of cosmological correlators and wavefunction coefficients. The recently proposed family tree decomposition technique solved these time integrals in terms of canonical objects called family trees, which are multivariate hypergeometric functions with energies as variables and twists as parameters. In this work, we provide a systematic study of the analytical properties of family trees. By exploiting the great flexibility of Mellin representations of family trees, we identify and characterize all their singularities in both variables and parameters and find their exact series representations around all singularities with finite convergent domains. These series automatically generate analytical continuation of arbitrary family trees over many distinct regions in the energy space. As a corollary, we show the factorization of family trees at zero partial-energy singularities to all orders. Our findings offer essential analytical data for further understanding and computing cosmological correlators.

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Cited by 8 Pith papers

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