Primordial Non-Gaussianity of Gravitational Waves in Ho\v{r}ava-Lifshitz Gravity
Yongqing Huang, Anzhong Wang, Razieh Yousefi, and Tao Zhu

TL;DR
This paper investigates the non-Gaussian features of primordial gravitational waves in Hořava-Lifshitz gravity, revealing specific shape dependencies and consistency with Planck data, influenced by the theory's unique interactions.
Contribution
It provides the first detailed analysis of the 3-point correlation function of gravitational waves in Hořava-Lifshitz gravity, highlighting how higher-order curvature terms affect non-Gaussianity shapes.
Findings
Certain curvature terms peak at squeezed configurations.
The Riemann cubic term favors equilateral shapes with same spins.
Constraints on energy scales are consistent with Planck observations.
Abstract
In this paper, we study 3-point correlation function of primordial gravitational waves generated in the de Sitter background in the framework of the general covariant Ho\v{r}ava-Lifshitz gravity with an arbitrary coupling constant . We find that, at cubic order, the interaction Hamiltonian receives contributions from four terms built of the 3-dimensional Ricci tensor of the leaves constant. In particular, the 3D Ricci scalar yields the same -dependence as that in general relativity, but with different magnitude due to coupling with the field and a UV history. Interestingly, the two terms and exhibit peaks at the squeezed limit. We show that this is due to the effects of the polarization tensors. The signal generated by the fourth term, , favors the…
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