Abstract.
In the mutated hybrid-inflation standard case, the spectral index \(n_{\rm s}\) is constrained by the e-folds number N, and the gravitational waves are negligible \((r\sim 10^{-4})\). Therefore, we propose to study this model in the framework of the Randall-Sundrum II braneworld scenario. Using the latest observational measurements from Planck data, we have shown that the inflation observables ( \(n_{\rm s}\), r, and \(\frac{{\rm d} n_{\rm s}}{{\rm d} \ln k}\) depend on all parameters. On the other hand, from the observed central value of the power spectrum perturbation \( P_{\rm R}(k)\), we have determined the energy scale which must be \(V_{0}^{1/4} \succsim 10^{14}\) GeV and we evaluate the brane tension value \( \lambda\). We showed that the spectral index takes the central value \(n_{\rm s}\sim 0.96\) and the gravitational waves becomes important \(r\sim 2\times 10^{-2}\). Furthermore the running \(\frac{{\rm d} n_{\rm s}}{{\rm d} \ln k}\) is perfectly in agreement with the recent observations. For the reheating phase, we have determined the value of reheating temperature \(T_{\rm re}\sim 10^{9}\) GeV.
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Ferricha-Alami, M., Sakhi, Z., Chakir, H. et al. Mutated hybrid inflation on brane and reheating temperature. Eur. Phys. J. Plus 132, 303 (2017). https://doi.org/10.1140/epjp/i2017-11575-8
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DOI: https://doi.org/10.1140/epjp/i2017-11575-8