Cosmological Wavefunctions as Amplitudes: Dual Shuffle Factorization and Uniqueness from New Hidden Zeros
Abstract
We show that cosmological wavefunctions in φn theories naturally generalize flat-space Tr(φ3) scattering amplitudes: via a simple map from tube variables to Mandelstam invariants, each wavefunction coefficient G becomes an on-shell amplitude-like object AG associated with a generating graph G. At tree level these objects coincide with the Cachazo-He-Yuan construction based on Cayley functions that generalizes Parke-Taylor factors. We uncover new graph-based hidden zeros that extend and unify all known cosmological zeros. Based on this zero structure, we uncover a factorization principle dual to unitarity. Instead of factorization across poles, A AL× AR, a zero at pa∈ GL\!·\! pb∈ GR=0 factorizes the generating graph, G GL× GR, and is equivalent to the shuffle decomposition AG=AGLx29E2AGR. Near-zero factorization is a simple consequence of this new structure. Using dual factorization, we show that locality together with the full set of hidden zeros uniquely fixes tree-level cosmological wavefunctions without assuming unitarity. We show that these zeros are equivalent to special enhanced large-z behavior under Britto-Cachazo-Feng-Witten (BCFW) shifts, extending the zeros--BCFW correspondence beyond flat-space amplitudes. We also find evidence for further extensions of the zero structure and loop-level uniqueness. Our results show that cosmology provides a natural arena for on-shell methods and even reveals new structure in flat-space amplitudes.
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