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Amplitubes: Graph Cosmohedra

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arxiv 2502.17564 v1 pith:WEBQWVKM submitted 2025-02-24 hep-th gr-qcmath.CO

classification hep-thgr-qcmath.CO
keywords graphassociahedroncosmohedronverticesassociahedraconstructedcosmohedrapolytope
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abstract

The tree-level scattering amplitudes for $\text{tr}(\phi^3)$ theory can be interpreted as a sum over the vertices of a polytope known as the associahedron. For each graph $G$, there exists a natural generalisation of the associahedron, which is constructed by considering tubes and tubings of the underling graph. This family of polytopes are called graph associahedra. The classical associahedra then arise as the graph associahedron for the path graphs. It is therefore natural to associate to each graph associahedron an amplitude-like object, we refer to as the amplitube, defined via a sum over its vertices. Recently, also in the context of trace $\text{tr}(\phi^3)$ theory, progress has been made towards defining a new geometric object, coined the cosmohedron, which computes not the amplitude, but the cosmological wavefunction as a sum over its vertices. This polytope can be constructed by consistently blowing up all boundaries of the associahedron to co-dimension one. Building on these results, in the present paper, we generalise the notion of the wavefunction for arbitrary graphs. These new expressions, which we call cosmological amplitubes, are defined via a sum over the vertices of a corresponding polytope, the graph cosmohedron. The graph cosmohedra are constructed by considering regions and regional tubings of the underlying graph which we introduce. Like the cosmohedron, the graph cosmohedra can be obtained by consistently blowing up all boundaries of the corresponding graph associahedron to co-dimension one. This new family of polytopes constitutes a vast generalisation of the cosmohedron, and we provide explicit embeddings for them, which builds upon an ABHY-like embedding for the graph associahedra.

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Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Higher-Spin Correlators in dS

    hep-th 2026-08 accept novelty 8.0 of 10

    The five-point de Sitter higher-spin correlator is shown to be a spurious-singularity-free rational function organized by graph-theoretic orbits of the complete graph K5.

  2. All Tree-Level Massive Cosmological Correlators via Spectral Gluing

    hep-th 2026-07 conditional novelty 7.0 of 10

    Tree-level massive de Sitter correlators are constructed by gluing Lauricella-type vertex functions according to graph combinatorics, and the hypergeometric content collapses to rational functions once the dynamical p...

  3. Correlators are simpler than wavefunctions

    hep-th 2025-12 unverdicted novelty 6.0 of 10

    Equal-time correlators are simpler than wavefunctions because they come from full-spacetime integrals; this implies fewer poles, cleaner factorization, and a systematic pole expansion whose first subleading term vanishes.

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