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Effective field theory of statistical anisotropies for primordial bispectrum and gravitational waves

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arxiv 1702.03744 v1 pith:JVI7A7ZK submitted 2017-02-13 astro-ph.CO hep-th

Effective field theory of statistical anisotropies for primordial bispectrum and gravitational waves

classification astro-ph.CO hep-th
keywords anisotropiesfieldgaugeperturbationsstatisticalbispectrumcalculateeffective
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We present the effective field theory studies of primordial statistical anisotropies in models of anisotropic inflation. The general action in unitary gauge is presented to calculate the leading interactions between the gauge field fluctuations, the curvature perturbations and the tensor perturbations. The anisotropies in scalar power spectrum and bispectrum are calculated and the dependence of these anisotropies to EFT couplings are presented. In addition, we calculate the statistical anisotropy in tensor power spectrum and the scalar-tensor cross correlation. Our EFT approach incorporates anisotropies generated in models with non-trivial speed for the gauge field fluctuations and sound speed for scalar perturbations such as in DBI inflation.

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  1. Isotropic universes with a preferred direction

    astro-ph.CO 2026-08 conditional novelty 7.0

    A tuned vector-field EFT can have an exactly isotropic FLRW background while hiding a preferred direction that reappears in perturbations as direction-dependent propagation and scalar–tensor mixing.