Cosmological cutting rules for Bogoliubov initial states

The field theoretic wavefunction in cosmological spacetimes has received much attention as a fundamental object underlying the generation of primordial perturbations in our universe. Assuming an initial Bunch-Davies state, unitary time evolution implies an infinite set of cutting rules for the wavef...

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Main Author: Diptimoy Ghosh, Enrico Pajer, Farman Ullah
Format: Article
Language:English
Published: SciPost 2025-01-01
Series:SciPost Physics
Online Access:https://scipost.org/SciPostPhys.18.1.005
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author Diptimoy Ghosh, Enrico Pajer, Farman Ullah
author_facet Diptimoy Ghosh, Enrico Pajer, Farman Ullah
author_sort Diptimoy Ghosh, Enrico Pajer, Farman Ullah
collection DOAJ
description The field theoretic wavefunction in cosmological spacetimes has received much attention as a fundamental object underlying the generation of primordial perturbations in our universe. Assuming an initial Bunch-Davies state, unitary time evolution implies an infinite set of cutting rules for the wavefunction to all orders in perturbation theory, collectively known as the cosmological optical theorem. In this work, we generalise these results to the case of Bogoliubov initial states, accounting for both parity-even and parity-odd interactions. We confirm our findings in a few explicit examples, assuming IR-finite interactions. In these examples, we preserve scale invariance by adiabatically turning on interactions in the infinite past rather than imposing a Bogoliubov state at some finite initial time. Finally, we give a prescription for computing Bogoliubov wavefunction coefficients from the corresponding Bunch-Davies coefficients for both $n$-point contact and four-point exchange diagrams.
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spelling doaj-art-37677936cf5e402096928f93af7e3b1c2025-01-07T11:45:42ZengSciPostSciPost Physics2542-46532025-01-0118100510.21468/SciPostPhys.18.1.005Cosmological cutting rules for Bogoliubov initial statesDiptimoy Ghosh, Enrico Pajer, Farman UllahThe field theoretic wavefunction in cosmological spacetimes has received much attention as a fundamental object underlying the generation of primordial perturbations in our universe. Assuming an initial Bunch-Davies state, unitary time evolution implies an infinite set of cutting rules for the wavefunction to all orders in perturbation theory, collectively known as the cosmological optical theorem. In this work, we generalise these results to the case of Bogoliubov initial states, accounting for both parity-even and parity-odd interactions. We confirm our findings in a few explicit examples, assuming IR-finite interactions. In these examples, we preserve scale invariance by adiabatically turning on interactions in the infinite past rather than imposing a Bogoliubov state at some finite initial time. Finally, we give a prescription for computing Bogoliubov wavefunction coefficients from the corresponding Bunch-Davies coefficients for both $n$-point contact and four-point exchange diagrams.https://scipost.org/SciPostPhys.18.1.005
spellingShingle Diptimoy Ghosh, Enrico Pajer, Farman Ullah
Cosmological cutting rules for Bogoliubov initial states
SciPost Physics
title Cosmological cutting rules for Bogoliubov initial states
title_full Cosmological cutting rules for Bogoliubov initial states
title_fullStr Cosmological cutting rules for Bogoliubov initial states
title_full_unstemmed Cosmological cutting rules for Bogoliubov initial states
title_short Cosmological cutting rules for Bogoliubov initial states
title_sort cosmological cutting rules for bogoliubov initial states
url https://scipost.org/SciPostPhys.18.1.005
work_keys_str_mv AT diptimoyghoshenricopajerfarmanullah cosmologicalcuttingrulesforbogoliubovinitialstates