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The Geometry of Cosmological Correlators
by Paolo Benincasa, Gabriele Dian
Submission summary
Authors (as registered SciPost users): | Gabriele Dian |
Submission information | |
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Preprint Link: | https://arxiv.org/abs/2401.05207v1 (pdf) |
Date submitted: | 2024-03-07 17:36 |
Submitted by: | Dian, Gabriele |
Submitted to: | SciPost Physics |
Ontological classification | |
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Academic field: | Physics |
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Approach: | Theoretical |
Abstract
We provide a first principle definition of cosmological correlation functions for a large class of scalar toy models in arbitrary FRW cosmologies, in terms of novel geometries we name {\it weighted cosmological polytopes}. Each of these geometries encodes a universal rational integrand associated to a given Feynman graph. In this picture, all the possible ways of organising, and computing, cosmological correlators correspond to triangulations and subdivisions of the geometry, containing the in-in representation, the one in terms of wavefunction coefficients and many others. We also provide two novel contour integral representations, one connecting higher and lower loop correlators and the other one expressing any of them in terms of a building block. We study the boundary structure of these geometries allowing us to prove factorisation properties and Steinmann-like relations when single and sequential discontinuities are approached. We also show that correlators must satisfy novel vanishing conditions. As the weighted cosmological polytopes can be obtained as an orientation-changing operation onto a certain subdivision of the cosmological polytopes encoding the wavefunction of the universe, this picture allows us to sharpen how the properties of cosmological correlators are inherited from the ones of the wavefunction. From a mathematical perspective, we also provide an in-depth characterisation of their adjoint surface.
Current status:
Reports on this Submission
Report
See attached pdf. I recommend the paper for publication and have some minor questions for the authors which they can choose to expand upon if they feel would enhance the presentation.
Recommendation
Publish (surpasses expectations and criteria for this Journal; among top 10%)
Author: Gabriele Dian on 2024-12-20 [id 5055]
(in reply to Report 1 on 2024-04-30)The authors would like to thank the referee for their thorough report and valuable comments. Below, we address each of the points raised:
1. The dashing prescription directly follows from a diagrammatic rewriting of Eq. (2.11), after expanding the wavefunctions in terms of the coupling and summing over graphs.
a. our formula 2.36 constitutes an example of a Feynman-like tree theorem , even if it differs from the original formulation for Feynman diagrams in flat space as it relates a 1-loop n_s-site graph to a tree-level (n_s+1) graph -- so the trees are produced by opening up a site rather then cutting a loop-propagator. However, this formulation is valid for arbitrary loops and can be stated as: an L-loop n_s-site integrand can be expressed as an integral of an (L-1)-loop (n_s+1)-site integrand. This formula can be recursed to express the L-loop integrand as an L- fold integral of trees.
b. one can take the point of view of the cosmological tree theorem by Agüi Salcedo and Melville. Such tree-theorem has been proven for one- loop wavefunction integrands. At the moment, we are not able to state that the same structure goes through for correlators. One can note that one-loop correlators can be expressed in terms of a connected wavefunction term and a disconnected one, with the cosmological tree theorem valid for the connected part. One has to see whether it can be economical to check that, representing the connected term via the cosmological tree theorem, it can be re-organised with the disconnected part in a cosmological tree theorem fashion<
Furthermore, it acts as a deformation of the kinematics in the spirit of the BCFW recursion. However, unlike the BCFW approach, this deformation applies solely to the energy of the particle, without imposing energy conservation.
However, we would like to point out how with this geometrical picture at hand, proving the existence of such a relation is simpler.