Non-Gaussianity from $X, Y$ gauge bosons in Cosmological Collider Physics

Heavy fields of Hubble scale order present during inflation contribute to the non-Gaussian signature for the three-point function of the inflaton. Taking into account that Hubble scale is around the scale of grand unified theory (GUT), this opens a possibility that the GUT scale signatures, which ar...

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Bibliographische Detailangaben
Hauptverfasser: Maru, Nobuhito, Okawa, Akira
Format: Artikel
Sprache:eng
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