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• W2022480636 abstract "We calculate the spectral index and tensor-to-scalar ratio for patch inflation arisen from the Gauss–Bonnet braneworld scenario. The patch cosmological models consist of Gauss–Bonnet (GB), Randall–Sundrum (RS), and 4D general relativistic (GR) cases. In order to compare with the observation data, we perform leading-order calculations for all patch models by choosing large-field, small-field, and hybrid potentials. We show that the large-field potentials are sensitive to a given patch model, while the small-field and hybrid potentials are insensitive to a given patch model. It is easier to discriminates between quadratic potential and quartic potential in the GB model rather than RS and GR models. Irrespective of patch models, it turns out that the small-field potentials are the promising models in view of the observation." @default.
• W2022480636 created "2016-06-24" @default.
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• W2022480636 date "2005-02-01" @default.
• W2022480636 modified "2023-09-30" @default.
• W2022480636 title "Inflation parameters from Gauss–Bonnet braneworld" @default.
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• W2022480636 doi "https://doi.org/10.1016/j.physletb.2005.01.019" @default.
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