Constant-roll inflation with tachyon field in the holographic braneworld
arXiv:2401.00352 · doi:10.1088/1361-6382/ad6058
Abstract
We study inflation driven by the tachyon field in the holographic braneworld by assuming the second slow-roll parameter is constant. The parameter can be either defined by the tachyon scalar field and the Hubble parameter or by the Hubble parameter only. By assuming a constant , we derive and numerically solve a differential equation for the Hubble expansion rate. We calculate numerically the scalar spectral index and the tensor-to-scalar ratio. We confront the results with the observational data and find some constraints on the free model parameters. The swampland conjectures are discussed in the context of the constant-roll inflation, with some accent on the holographic model.
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