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• W2798971796 abstract "The reconstruction of an inflationary universe in the context of the Galileon model or G-model, considering as attractors the scalar spectral index $n_S(N)$ and the tensor to scalar ratio $r(N)$ as a function of the number of e-folding $N$ is studied. By assuming a coupling of the form $G(phi,X)=g(phi),X$, we obtain the effective potential $V$ and the coupling parameter $g$ in terms of the cosmological parameters $n_S$ and $r$ under the slow roll approximation. From some examples for $n_S(N)$ and $r(N)$, different results for the effective potential $V(phi)$ and the coupling parameter $g(phi)$ are found." @default.
• W2798971796 created "2018-05-07" @default.
• W2798971796 creator A5068302866 @default.
• W2798971796 date "2018-07-31" @default.
• W2798971796 modified "2023-10-09" @default.
• W2798971796 title "Reconstructing <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML display=inline><mml:mi>G</mml:mi></mml:math> inflation: From the attractors <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML display=inline><mml:msub><mml:mi>n</mml:mi><mml:mi>S</mml:mi></mml:msub><mml:mo stretchy=false>(</mml:mo><mml:mi>N</mml:mi><mml:mo stretchy=false>)</mml:mo></mml:math> and <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML display=inline><mml:mi>r</mml:mi><mml:mo stretchy=…" @default.
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• W2798971796 doi "https://doi.org/10.1103/physrevd.98.023542" @default.
• W2798971796 hasPublicationYear "2018" @default.
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