The Cosmological Phonon: Symmetries and Amplitudes on Sub-Horizon Scales
Tanguy Grall, Sadra Jazayeri, David Stefanyszyn

TL;DR
This paper classifies scalar theories with non-linearly realized Lorentz boost symmetries, introduces a new extended galileid theory, and analyzes their scattering amplitudes and phase structures in cosmological contexts.
Contribution
It provides an algebraic classification of shift-symmetric scalars with broken Lorentz boosts, discovers the extended galileid theory, and analyzes the amplitude structures of DBI and galileid theories.
Findings
Rediscovered known phonon theories within superfluid and galileid classes.
Discovered the extended galileid theory with fixed couplings due to additional symmetry.
Showed that DBI scalar amplitudes are secretly Poincaré invariant around superfluid backgrounds.
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 . Generic galileids correspond to the…
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