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We study inflation and the generation of primordial fluctuations in gravity’s rainbow. We calculate the cosmological perturbations and then the scalar and tensor primordial power spectrum. We contrast the predictions of the model with the current observational data from PLANCK and BICEP/Keck. Particularly, we found new results for the scalar spectral index and the tensor-to-scalar ratio along with new observational constraints on the rainbow functions.

生成讲解博客的中文版本

生成AI智能校验的中文版本