Tao Zhu, Wen Zhao, Yongqing Huang, Anzhong Wang, Qiang Wu
In this paper, we study the effects of parity violation on non-gaussianities of primordial gravitational waves in the framework of Ho\v{r}ava-Lifshitz theory of gravity, in which high-order spatial derivative operators, including the ones violating parity, generically appear. By calculating the three-point correlation function, we find that the leading-order contributions to the non-gaussianities come from the usual second-order derivative operators, which produce the same bispectrum as that found in general relativity. The contributions from high-order spatial n-th derivative operators are always suppressed by a factor $(H/M_*)^{n-2} \; (n \ge 3)$, where $H$ denotes the inflationary energy and $M_*$ the suppression mass scale of the high-order spatial derivative operators of the theory. Therefore, the next leading-order contributions come from the three-dimensional gravitational Chern-Simons term. With some reasonable arguments, it is shown that this 3-dimensional operator is the only one that violates the parity and in the meantime has non-vanishing contributions to non-gaussianities.
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http://arxiv.org/abs/1305.0600
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