Three Form Inflation

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dc.creatorGruzinov, Andrei
dc.date2004-01-26
dc.date.accessioned2026-07-07T02:12:00Z
dc.date.available2026-07-07T02:12:00Z
dc.descriptionIt is noted that inflation driven by a three form with arbitrary self coupling satisfies a consistency relation $n_S-1=2n_T$, between spectral indices of scalar and tensor cosmological perturbations. The standard consistency relation for the ratio of the amplitudes of perturbations is only valid for quadratic self coupling of the three form.
dc.description4 pages
dc.identifierhttps://arxiv.org/abs/astro-ph/0401520
dc.identifierhttp://arxiv.org/abs/astro-ph/0401520
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/7306
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Theory
dc.titleThree Form Inflation
dc.typetext

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