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• W2783182012 abstract "The reconstruction of a warm inflationary universe model from the scalar spectral index $n_S(N)$ and the tensor to scalar ratio $r(N)$ as a function of the number of e-folds $N$ is studied. Under a general formalism we find the effective potential and the dissipative coefficient in terms of the cosmological parameters $n_S$ and $r$ considering the weak and strong dissipative stages under the slow roll approximation. As a specific example, we study the attractors for the index $n_S$ given by $n_{S}-1propto N^{-1}$ and for the ratio $rpropto N^{-2}$, in order to reconstruct the model of warm inflation. Here, expressions for the effective potential $V(phi)$ and the dissipation coefficient $Gamma(phi)$ are obtained." @default.
• W2783182012 created "2018-01-26" @default.
• W2783182012 creator A5068302866 @default.
• W2783182012 date "2018-03-01" @default.
• W2783182012 modified "2023-10-13" @default.
• W2783182012 title "Reconstructing warm inflation" @default.
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• W2783182012 doi "https://doi.org/10.1140/epjc/s10052-018-5741-0" @default.
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