Titlebook: Weigh Them All!; Cosmological Searche Sunny Vagnozzi Book 2020 The Editor(s) (if applicable) and The Author(s), under exclusive license to

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Massive Neutrinos Meet Inflation,e values inferred for . might be sensitive to the assumptions I make when introducing . into the picture, or to the very fact that I introduced . in first place. Recall, in fact, that in the baseline .CDM model, . is not a free parameter, but is fixed to ., the minimum value allowed by oscillations data.

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Massive Neutrinos Meet Inflation,e values inferred for . might be sensitive to the assumptions I make when introducing . into the picture, or to the very fact that I introduced . in first place. Recall, in fact, that in the baseline .CDM model, . is not a free parameter, but is fixed to ., the minimum value allowed by oscillations data.

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Scale-Dependent Galaxy Bias and CMB Lensing-Galaxy Cross-Correlations,However, naïvely comparing the constraining power of .(.) versus BAO measurements revealed that improvements are needed in order to fully harness the constraining power of the former, especially in terms of getting a better handle on the galaxy bias.

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Scale-Dependent Galaxy Bias and CMB Lensing-Galaxy Cross-Correlations,However, naïvely comparing the constraining power of .(.) versus BAO measurements revealed that improvements are needed in order to fully harness the constraining power of the former, especially in terms of getting a better handle on the galaxy bias.

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Overview of Physical Cosmology,ic, and correspondingly the Friedmann equations, Eqs. (2.4) and (2.5). In this Chapter, I will provide a more detailed (but still rather brief) picture of physical cosmology and the (thermal) history of the Universe, starting from the equations we have seen in Sect. 2.2 and elementary notions of the

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Overview of Physical Cosmology,ic, and correspondingly the Friedmann equations, Eqs. (2.4) and (2.5). In this Chapter, I will provide a more detailed (but still rather brief) picture of physical cosmology and the (thermal) history of the Universe, starting from the equations we have seen in Sect. 2.2 and elementary notions of the

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