Titlebook: Cosmological Probes of Light Relics; Benjamin Wallisch Book 2019 The Editor(s) (if applicable) and The Author(s), under exclusive license

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Searching for Light Relics with the CMB,s through the sensitivity to this effect that the recent CMB?data has provided a robust detection of free-streaming neutrinos. In this chapter, we revisit the phase shift of the CMB?anisotropy spectrum as a probe of new physics. The phase shift is particularly interesting because its physical origin

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Searching for Light Relics with LSS, constrained to be less than ten percent of the total energy density in radiation. Upcoming cosmic microwave background (CMB) experiments, however, have the potential to measure the radiation density at the one-percent level, which is close to well-motivated theoretical targets. In this chapter, we

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Measurement of Neutrinos in the BAO Spectrum, energy density in the early universe and, therefore, played an important role in the evolution of cosmological perturbations. In particular, fluctuations in the neutrino density produced a distinct shift in the temporal phase of sound waves in the primordial plasma. In this chapter, we report on th

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Conclusions and Outlook,ot only become precise enough to answer questions about the universe at large, but also to start addressing puzzles in the microscopic description of Nature. Cosmological measurements are particularly well suited to study Standard Model neutrinos and to shed light on the possible existence of other

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Light Species in Cosmology and Particle Physics,mates for the constraining power of astrophysical systems and cosmology, we introduce the particle physics aspects of this thesis, discuss the main cosmological parameter capturing neutrinos and any other light thermal relics, and examine the possible signatures of these particles in cosmological observables.

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