Tensor non-Gaussianities from Non-minimal Coupling to the Inflaton
Emanuela Dimastrogiovanni, Matteo Fasiello, Gianmassimo Tasinato,, David Wands

TL;DR
This paper explores how non-minimal coupling of extra massive spin-2 particles during inflation can generate significant tensor non-Gaussianities, with potential observational signatures in future gravitational wave detectors like LISA.
Contribution
It demonstrates that non-minimal coupling allows massive spin-2 particles to produce observable tensor non-Gaussianities, extending the understanding of inflationary tensor signals.
Findings
Tensor bispectrum depends on extra field mass and sound speed.
Shape-function of non-Gaussianities interpolates between local and equilateral.
LISA can potentially detect the predicted tensor non-Gaussianities.
Abstract
Tensor non-Gaussianity represents an important future probe of the physics of inflation. Inspired by recent works, we elaborate further on the possibility of significant primordial tensor non-Gaussianities sourced by extra fields during inflation. Unitarity constraints limit the impact of extra (spinning) particle content by means of a lower bound on the corresponding mass spectrum. For spin-2 particles, this takes the form of the well-known Higuchi bound. Massive () particles will typically decay during inflation unless they are non-minimally coupled to the inflaton sector: the inflating field "lifts" the dynamics of the extra field(s), effectively getting around the limits imposed by unitarity. There exist several models that realize such a mechanism, but we focus here on the set-up of [1] where, through an EFT approach, one is able to capture the essential features common…
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