標(biāo)題: Titlebook: Beyond the Standard Model Cocktail; A Modern and Compreh Yann Gouttenoire Book 2022 The Editor(s) (if applicable) and The Author(s), under [打印本頁] 作者: bankrupt 時(shí)間: 2025-3-21 16:25
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書目名稱Beyond the Standard Model Cocktail讀者反饋學(xué)科排名
作者: invade 時(shí)間: 2025-3-21 20:17 作者: 充氣球 時(shí)間: 2025-3-22 01:46 作者: 陳腐的人 時(shí)間: 2025-3-22 07:22 作者: hauteur 時(shí)間: 2025-3-22 09:24 作者: DRILL 時(shí)間: 2025-3-22 16:53
Clare J. Hooper,Bruna Neves,Georgeta Bordearoweak (EW) symmetry was effective (we say “restored”). The electromagnetism and the weak interaction constituted a single electroweak interaction, and electroweak and Higgs bosons were continuously created and absorbed in the plasma. This raises the question on how the Higgs field acquired the non-作者: impaction 時(shí)間: 2025-3-22 19:25
Lecture Notes in Computer Sciencer of the universe, as well as the origin of inflation. These, together with a number of other fundamental theoretical puzzles associated with e.g. the flavour structure of the matter sector and the ultra-violet properties of the Higgs scalar field, motivate extensions of the Standard Model featuring作者: Commonplace 時(shí)間: 2025-3-22 23:10
Clare J. Hooper,Bruna Neves,Georgeta Bordeaf GW experiments to probe the existence of a early matter era or an early second period of inflation, In this chapter, we use those findings to constrain particle physics models leading to such a change of cosmology with a particular focus on models of heavy Dark Matter.作者: 泛濫 時(shí)間: 2025-3-23 04:04 作者: 贊美者 時(shí)間: 2025-3-23 06:39 作者: FOIL 時(shí)間: 2025-3-23 13:41 作者: 掙扎 時(shí)間: 2025-3-23 17:12 作者: NICHE 時(shí)間: 2025-3-23 18:19 作者: 旁觀者 時(shí)間: 2025-3-23 22:55 作者: 發(fā)誓放棄 時(shí)間: 2025-3-24 02:37
Lecture Notes in Computer ScienceThe possible existence of new confining sectors is motivated by most major failures of our understanding of Nature at a fundamental level. First, the stability of particle Dark Matter can be elegantly achieved as an accident if it is a composite state of a new strongly-coupled sector, similarly to proton stability in QCD, see e.g.?[.].作者: 圖表證明 時(shí)間: 2025-3-24 06:34 作者: dysphagia 時(shí)間: 2025-3-24 13:28 作者: CHANT 時(shí)間: 2025-3-24 16:20 作者: interior 時(shí)間: 2025-3-24 21:56 作者: Intractable 時(shí)間: 2025-3-25 00:45 作者: mitral-valve 時(shí)間: 2025-3-25 05:11 作者: Semblance 時(shí)間: 2025-3-25 10:10
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 .).作者: 恃強(qiáng)凌弱的人 時(shí)間: 2025-3-25 15:37
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.作者: OVER 時(shí)間: 2025-3-25 19:43 作者: Proponent 時(shí)間: 2025-3-25 23:18
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?作者: Toxoid-Vaccines 時(shí)間: 2025-3-26 03:12 作者: RAG 時(shí)間: 2025-3-26 04:46
,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.作者: 剛開始 時(shí)間: 2025-3-26 11:36 作者: TATE 時(shí)間: 2025-3-26 15:10
,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.作者: 彎曲道理 時(shí)間: 2025-3-26 20:46
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作者: Aura231 時(shí)間: 2025-3-26 23:12 作者: botany 時(shí)間: 2025-3-27 04:50 作者: 身心疲憊 時(shí)間: 2025-3-27 07:46 作者: MEN 時(shí)間: 2025-3-27 11:56 作者: TRUST 時(shí)間: 2025-3-27 15:41 作者: 斗志 時(shí)間: 2025-3-27 21:34 作者: objection 時(shí)間: 2025-3-27 22:14
Thermal Dark Matter,Fig.?., instead of listing the different possible candidates, we prefer to focus on one of the best motivated and most studied scenario: the one in which Dark Matter is thermally produced. For reviews on DM history, observations, models and searches, we refer to [.,.,.,.,.,.,.,.,.,.,.,.,.,.,.,.,.,.,作者: 我不重要 時(shí)間: 2025-3-28 02:55
Homeopathic Dark Matter,lated theories beyond the TeV range. How can we gain an experimental access to such energy scales? High energy cosmic rays currently constitute a privileged access to that realm, as opposed to the more subtle one offered by various precision measurements. Many telescopes are indeed now observing suc作者: 怒目而視 時(shí)間: 2025-3-28 09:55 作者: Osteons 時(shí)間: 2025-3-28 11:15 作者: 心痛 時(shí)間: 2025-3-28 16:36
,Probe Heavy DM with?GW from?CS,f GW experiments to probe the existence of a early matter era or an early second period of inflation, In this chapter, we use those findings to constrain particle physics models leading to such a change of cosmology with a particular focus on models of heavy Dark Matter.作者: Digest 時(shí)間: 2025-3-28 21:35 作者: 祖先 時(shí)間: 2025-3-28 23:34 作者: MENT 時(shí)間: 2025-3-29 07:01 作者: Locale 時(shí)間: 2025-3-29 10:03
2190-5053 scale, which are among the most studied dark matter candidates. Motivated by the absence of experimental evidence for such particles, this thesis explores the possibility that dark matter is much heavier than what is conventionally assumed..978-3-031-11864-7978-3-031-11862-3Series ISSN 2190-5053 Series E-ISSN 2190-5061 作者: 宴會(huì) 時(shí)間: 2025-3-29 12:05 作者: exophthalmos 時(shí)間: 2025-3-29 17:23
