Cosmological Polytopes and the Wavefunction of the Universe
Nima Arkani-Hamed, Paolo Benincasa, Alexander Postnikov

TL;DR
This paper introduces cosmological polytopes as a geometric framework to understand the wavefunction of the universe in cosmological models, linking positive geometry with quantum cosmology and revealing new representations and symmetries.
Contribution
It establishes a novel geometric approach using cosmological polytopes to analyze the wavefunction of the universe, connecting physics with intrinsic mathematical structures.
Findings
Cosmological polytopes encode the singularity structure of the wavefunction.
Triangulations of polytopes reproduce known and new wavefunction representations.
Polylogarithms associated with graphs are derived from the geometry of the polytopes.
Abstract
We present a connection between the physics of cosmological time evolution and the mathematics of positive geometries, roughly analogous to similar connections seen in the context of scattering amplitudes. We consider the wavefunction of the universe in a class of toy models of conformally coupled scalars (with non-conformal interactions) in FRW cosmologies. The contribution of each Feynman diagram to the wavefunction of the universe is associated with a certain universal rational integrand, which we identify as the canonical form of a "cosmological polytope", which have an independent, intrinsic definition, making no reference to physics. The singularity structure of the wavefunction for this model of scalars is common to all theories, and is geometrized by the cosmological polytope. Natural triangulations of the polytope reproduce the path-integral and "old-fashioned perturbation…
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Cosmology and Gravitation Theories · Noncommutative and Quantum Gravity Theories
