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Chen, JCAP11, 063 (2024), arXiv:2312.06105 [astro-ph.CO]

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Inflation with vector fields revisited: non-Gaussianities

hep-th · 2026-05-27 · unverdicted · novelty 5.0

In kinetically coupled vector inflation, the bispectrum in the large-h regime exhibits competing local and flattened non-Gaussian signals with distinct h scalings that distinguish vector-supported dynamics.

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  • Inflation with vector fields revisited: non-Gaussianities hep-th · 2026-05-27 · unverdicted · none · ref 28

    In kinetically coupled vector inflation, the bispectrum in the large-h regime exhibits competing local and flattened non-Gaussian signals with distinct h scalings that distinguish vector-supported dynamics.