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- W3099282142 abstract "We consider two non-canonical scalar fields (tachyon and DBI) with E-model type of the potential. We study cosmological inflation in these models to find possible $alpha$-attractors. We show that similar to the canonical scalar field case, in both tachyon and DBI models there is a value of the scalar spectral index in small $alpha$ limit which is just a function of the e-folds number. However, the value of $n_{s}$ in DBI model is somewhat different from the other ones. We also compare the results with Planck2015 TT, TE, EE+lowP data. The reheating phase after inflation is studied in these models which gives some more constraints on the model's parameters." @default.
- W3099282142 created "2020-11-23" @default.
- W3099282142 creator A5010161607 @default.
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- W3099282142 date "2018-05-01" @default.
- W3099282142 modified "2023-10-16" @default.
- W3099282142 title "α-Attractor and reheating in a model with noncanonical scalar fields" @default.
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- W3099282142 doi "https://doi.org/10.1142/s0218271818500761" @default.
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