Abstract
Cosmology is experiencing an exciting phase, characterized by the enormous amount of data which are already available or will soon become available. This epoch, which has been dubbed the era of precision cosmology, clearly requires an adequate theoretical effort to provide predictions at high level of accuracy. At the same time, the quality of the data available allows one to face with totally new and challenging questions. In this chapter we will focus on three complementary issues: (i) observable predictions of inflation in the early universe; (ii) a short overview of some cosmological effects of modified gravity scenarios; (iii) neutrinos in cosmology and large-scale structures.
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This approximation neglects non-linearities induced by the fact that the signal is in redshift space.
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Acknowledgements
The authors are supported by the Astroparticle INFN I.S. “INDARK”. Matteo Viel is supported by the ERC-StG “cosmoIGM”. The work of Nicola Bartolo and Sabino Matarrese was supported in part by ASI/INAF Agreement I/072/09/0 for the Planck LFI Activity of Phase E2. We thank Fabio Finelli, Michele Liguori, Francisco Villaescusa-Navarro for useful discussions.
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Bartolo, N., Matarrese, S., Viel, M. (2018). Cosmology: Searching for Deviations from the Standard Cosmological Model. In: Aloisio, R., Coccia, E., Vissani, F. (eds) Multiple Messengers and Challenges in Astroparticle Physics. Springer, Cham. https://doi.org/10.1007/978-3-319-65425-6_7
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