The cosmological phonon: symmetries and amplitudes on sub-horizon scales

Abstract In contrast to massless spinning particles, scalars are not heavily constrained by unitarity and locality. Off-shell, no gauge symmetries are required to write down manifestly local theories, while on-shell consistent factorisation is trivial. Instead a useful classification scheme for scal...

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Main Authors: Tanguy Grall, Sadra Jazayeri, David Stefanyszyn
Format: Article
Language:English
Published: SpringerOpen 2020-11-01
Series:Journal of High Energy Physics
Subjects:
Online Access:http://link.springer.com/article/10.1007/JHEP11(2020)097
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spelling doaj-09e4002d0f284dc985b9fc7b481c583f2020-11-25T04:10:46ZengSpringerOpenJournal of High Energy Physics1029-84792020-11-0120201115110.1007/JHEP11(2020)097The cosmological phonon: symmetries and amplitudes on sub-horizon scalesTanguy Grall0Sadra Jazayeri1David Stefanyszyn2Department of Applied Mathematics and Theoretical Physics, University of CambridgeDepartment of Applied Mathematics and Theoretical Physics, University of CambridgeDepartment of Applied Mathematics and Theoretical Physics, University of CambridgeAbstract In contrast to massless spinning particles, scalars are not heavily constrained by unitarity and locality. Off-shell, no gauge symmetries are required to write down manifestly local theories, while on-shell consistent factorisation is trivial. Instead a useful classification scheme for scalars is based on the symmetries they can non-linearly realise. Motivated by the breaking of Lorentz boosts in cosmology, in this paper we classify the possible symmetries of a shift-symmetric scalar that is assumed to non-linearly realise Lorentz boosts as, for example, in the EFT of inflation. Our classification method is algebraic; guided by the coset construction and inverse Higgs constraints. We rediscover some known phonon theories within the superfluid and galileid classes, and discover a new galileid theory which we call the extended galileid. Generic galileids correspond to the broken phase of galileon scalar EFTs and our extended galileids correspond to special subsets where each galileon coupling is fixed by an additional symmetry. We discuss the broken phase of theories that also admit a perturbation theory around Poincaré invariant vacua and we show that the so-called exceptional EFTs, the DBI scalar and special galileon, do not admit such a broken phase. Concentrating on DBI we provide a detailed account of this showing that the scattering amplitudes are secretly Poincaré invariant when the theory is expanded around the superfluid background used in the EFT of inflation. We point out that DBI is an exception to the common lore that the residue of the total energy pole of cosmological correlators is proportional to the amplitude. We also discuss the inevitability of poles in 2 → 2 scattering amplitudes when boost are spontaneously broken meaning that such theories do not admit Adler zeros and generalisations even in the presence of a shift symmetry.http://link.springer.com/article/10.1007/JHEP11(2020)097Effective Field TheoriesGlobal SymmetriesSpace-Time Symmetries
collection DOAJ
language English
format Article
sources DOAJ
author Tanguy Grall
Sadra Jazayeri
David Stefanyszyn
spellingShingle Tanguy Grall
Sadra Jazayeri
David Stefanyszyn
The cosmological phonon: symmetries and amplitudes on sub-horizon scales
Journal of High Energy Physics
Effective Field Theories
Global Symmetries
Space-Time Symmetries
author_facet Tanguy Grall
Sadra Jazayeri
David Stefanyszyn
author_sort Tanguy Grall
title The cosmological phonon: symmetries and amplitudes on sub-horizon scales
title_short The cosmological phonon: symmetries and amplitudes on sub-horizon scales
title_full The cosmological phonon: symmetries and amplitudes on sub-horizon scales
title_fullStr The cosmological phonon: symmetries and amplitudes on sub-horizon scales
title_full_unstemmed The cosmological phonon: symmetries and amplitudes on sub-horizon scales
title_sort cosmological phonon: symmetries and amplitudes on sub-horizon scales
publisher SpringerOpen
series Journal of High Energy Physics
issn 1029-8479
publishDate 2020-11-01
description Abstract In contrast to massless spinning particles, scalars are not heavily constrained by unitarity and locality. Off-shell, no gauge symmetries are required to write down manifestly local theories, while on-shell consistent factorisation is trivial. Instead a useful classification scheme for scalars is based on the symmetries they can non-linearly realise. Motivated by the breaking of Lorentz boosts in cosmology, in this paper we classify the possible symmetries of a shift-symmetric scalar that is assumed to non-linearly realise Lorentz boosts as, for example, in the EFT of inflation. Our classification method is algebraic; guided by the coset construction and inverse Higgs constraints. We rediscover some known phonon theories within the superfluid and galileid classes, and discover a new galileid theory which we call the extended galileid. Generic galileids correspond to the broken phase of galileon scalar EFTs and our extended galileids correspond to special subsets where each galileon coupling is fixed by an additional symmetry. We discuss the broken phase of theories that also admit a perturbation theory around Poincaré invariant vacua and we show that the so-called exceptional EFTs, the DBI scalar and special galileon, do not admit such a broken phase. Concentrating on DBI we provide a detailed account of this showing that the scattering amplitudes are secretly Poincaré invariant when the theory is expanded around the superfluid background used in the EFT of inflation. We point out that DBI is an exception to the common lore that the residue of the total energy pole of cosmological correlators is proportional to the amplitude. We also discuss the inevitability of poles in 2 → 2 scattering amplitudes when boost are spontaneously broken meaning that such theories do not admit Adler zeros and generalisations even in the presence of a shift symmetry.
topic Effective Field Theories
Global Symmetries
Space-Time Symmetries
url http://link.springer.com/article/10.1007/JHEP11(2020)097
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