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Gauge-flation and Cosmic No-Hair Conjecture

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arxiv 1109.5573 v2 pith:7TSNHVUH submitted 2011-09-26 hep-th astro-ph.COgr-qchep-ph

classification hep-thastro-ph.COgr-qchep-ph
keywords conjecturecosmicgauge-flationno-hairinflationaccordanalyticanisotropies
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Gauge-flation, inflation from non-Abelian gauge fields, was introduced in [1,2]. In this work, we study the cosmic no-hair conjecture in gauge-flation. Starting from Bianchi-type I cosmology and through analytic and numeric studies we demonstrate that the isotropic FLRW inflation is an attractor of the dynamics of the theory and that the anisotropies are damped within a few e-folds, in accord with the cosmic no-hair conjecture.

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  1. Pure Chromo-Natural Inflation: Signatures of Particle Production from Weak to Strong Backreaction

    astro-ph.CO 2025-04 conditional novelty 6.0 of 10

    Pure chromo-natural inflation unavoidably transitions from weak to strong backreaction, producing a chiral three-peak gravitational wave spectrum and a scalar peak that can form primordial black holes.

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