2017
DOI: 10.48550/arxiv.1712.04466
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Towards an explicit model of large field inflation

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“…For p > M , the transition to the supersymmetric vacuum requires about p/M steps of the brane/flux annihilation. During the transition, the vacuum energy density gradually decreases as the NS5-brane oscillates between the north and south pole along S 3 [11,12]. This indeed is one way to realize the axion monodromy, the unfolding of the periodic axion field space induced by the coupling of an axion to fluxes [13,14] (for various models, see, e.g., [15,16,17,18,19,20]).…”
Section: Introductionmentioning
confidence: 96%
“…For p > M , the transition to the supersymmetric vacuum requires about p/M steps of the brane/flux annihilation. During the transition, the vacuum energy density gradually decreases as the NS5-brane oscillates between the north and south pole along S 3 [11,12]. This indeed is one way to realize the axion monodromy, the unfolding of the periodic axion field space induced by the coupling of an axion to fluxes [13,14] (for various models, see, e.g., [15,16,17,18,19,20]).…”
Section: Introductionmentioning
confidence: 96%