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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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樓主: Tamoxifen
21#
發(fā)表于 2025-3-25 04:42:36 | 只看該作者
Measurement of Neutrinos in the BAO Spectrum,ence for a non-zero phase shift at greater than 95simulations and forecasts. Besides providing a new measurement of the cosmic neutrino background, this work is the first application of the BAO feature beyond its application as a standard ruler and to early universe physics.
22#
發(fā)表于 2025-3-25 08:00:31 | 只看該作者
J?rg Faust,Hans-Joachim Lauth,Wolfgang Munodel. In this chapter, we give a concise introduction to the topic of this thesis, the search for these elusive particles by identifying and extracting their robust signatures in cosmological observables. Moreover, we outline the rest of the thesis and provide a collection of the employed notation and conventions.
23#
發(fā)表于 2025-3-25 11:41:02 | 只看該作者
Introduction,del. In this chapter, we give a concise introduction to the topic of this thesis, the search for these elusive particles by identifying and extracting their robust signatures in cosmological observables. Moreover, we outline the rest of the thesis and provide a collection of the employed notation and conventions.
24#
發(fā)表于 2025-3-25 16:04:17 | 只看該作者
Book 2019ly become precise enough to answer questions about the universe on the largest scales, but also to address puzzles in the microscopic description of Nature. This thesis investigates new ways of probing the early universe, the properties of neutrinos and the possible existence of other light particle
25#
發(fā)表于 2025-3-25 22:51:59 | 只看該作者
2190-5053 icles thathave ever been in thermal equilibrium or imply strong bounds on their properties..? ? ? ? ? ? ? ? ? ? ? ? ? ? ?.978-3-030-31100-1978-3-030-31098-1Series ISSN 2190-5053 Series E-ISSN 2190-5061
26#
發(fā)表于 2025-3-26 01:34:00 | 只看該作者
Searching for Light Relics with the CMB,t simple models to illustrate each of these effects and provide observational constraints from the Planck temperature and polarization data on additional forms of radiation. We also estimate the capabilities of future CMB?Stage-4 experiments. Whenever possible, we give analytic interpretations and c
27#
發(fā)表于 2025-3-26 05:11:57 | 只看該作者
28#
發(fā)表于 2025-3-26 09:06:01 | 只看該作者
29#
發(fā)表于 2025-3-26 14:00:50 | 只看該作者
https://doi.org/10.1007/978-3-030-31098-1Cosmic Neutrinos/Cosmic Neutrino Background; Light Thermal Relics; Early Universe Cosmology; Cosmologic
30#
發(fā)表于 2025-3-26 19:47:30 | 只看該作者
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