Inflationary trispectrum from graviton exchange
David Seery, Martin S. Sloth, Filippo Vernizzi
TL;DR
This paper computes the inflationary trispectrum arising from graviton exchange in single-field slow-roll models, using the in-in formalism in the uniform curvature gauge to evaluate the graviton–scalar–scalar vertex and the resulting four-point function of curvature perturbations. The graviton-exchange contribution, proportional to the tensor-to-scalar ratio $r$, is found to be of the same order as the previously computed scalar-contact contribution, and remains finite after combinations of time integrals. In the counter-collinear limit, the trispectrum becomes locally parametrized with $\tau_{\text{NL}}^{local} \sim r$, and a detailed numerical analysis shows that the total trispectrum can reach $|\tau_{\text{NL}}| \approx 1.218 r$, indicating $\tau_{\text{NL}}$ is generically of order $r$. The work establishes that the total trispectrum in single-field slow-roll inflation is bounded by $\tau_{\text{NL}} \sim r$, challenges the simple $\tau_{\text{NL}} \sim f_{\text{NL}}^2$ expectation, and provides results applicable to multi-field scenarios with flat field space.
Abstract
We compute the connected four-point correlation function of the primordial curvature perturbation generated during inflation with standard kinetic terms, where the correlation is established via exchange of a graviton between two pairs of scalar fluctuations. Any such correlation yields a contribution to the scalar trispectrum of the order of the tensor to scalar ratio r. This contribution is numerically one order of magnitude larger than the one previously calculated on the basis of scalar perturbations interacting at a point and satisfies a simple relation in the limit where the momentum of the graviton which is exchanged becomes much smaller than the external momenta. We conclude that the total non-linearity parameter generated by single-field models of slow-roll inflation is at maximum tauNL ~ r.
