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Titlebook: Beyond the Standard Model Cocktail; A Modern and Compreh Yann Gouttenoire Book 2022 The Editor(s) (if applicable) and The Author(s), under

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21#
發(fā)表于 2025-3-25 05:11:59 | 只看該作者
22#
發(fā)表于 2025-3-25 10:10:25 | 只看該作者
Lecture Notes in Computer Science.,.,.,.,.,.,.,.]. For textbooks, we call attention to [.,.,.,.,.,.,.]. The results of the present chapter, in particular Sect.?. which deals with Sommerfeld effects and the unitarity limit, are crucial for Chap.?. on Homeopathic Dark Matter. All the figures in the chapter are mine (Fig.?., ., ., ., . and .).
23#
發(fā)表于 2025-3-25 15:37:53 | 只看該作者
Lecture Notes in Computer Science new degrees of freedom and new energy scales. In turn, such new physics can substantially impact the expansion history in the early universe and leads to deviations with respect to the standard cosmological model. Any deviations in the Friedmann equation occurring at temperatures above the MeV remain to date essentially unconstrained.
24#
發(fā)表于 2025-3-25 19:43:26 | 只看該作者
25#
發(fā)表于 2025-3-25 23:18:34 | 只看該作者
Rafa? Olszowski,Marcin Chmielowskio equilibrate their strengths? Why do neutrinos have non-vanishing masses while the SM predicts they should be massless? Why is the electron 300 000 times lighter than the top quark? Why does the strong force seem to be invariant under Charge-conjugation and Parity?
26#
發(fā)表于 2025-3-26 03:12:03 | 只看該作者
27#
發(fā)表于 2025-3-26 04:46:37 | 只看該作者
,Standard Model of?Elementary Particles, seventy of them earned the Nobel prize, since the introduction of the photon by Einstein in 1905 [.] or the unification of Quantum Mechanics and Special Relativity by Dirac in 1928 [., .]. The SM has been theoretically achieved after three major breakthroughs in the end 60s/early 70s.
28#
發(fā)表于 2025-3-26 11:36:44 | 只看該作者
29#
發(fā)表于 2025-3-26 15:10:24 | 只看該作者
,Gravitational Waves from?Cosmic Strings, new degrees of freedom and new energy scales. In turn, such new physics can substantially impact the expansion history in the early universe and leads to deviations with respect to the standard cosmological model. Any deviations in the Friedmann equation occurring at temperatures above the MeV remain to date essentially unconstrained.
30#
發(fā)表于 2025-3-26 20:46:30 | 只看該作者
2190-5053 nd cosmology.Covers all major open puzzles and present the s.This book provides a remarkable and complete survey of important questions at the interface between theoretical particle physics and cosmology..After discussing the theoretical and experimental physics revolution that led to the rise of th
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