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Titlebook: Cosmological Implications of Quantum Anomalies; Neil David Barrie Book 2018 Springer Nature Switzerland AG 2018 Baryogenesis.Cosmological

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發(fā)表于 2025-3-21 20:02:06 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
書目名稱Cosmological Implications of Quantum Anomalies
編輯Neil David Barrie
視頻videohttp://file.papertrans.cn/239/238919/238919.mp4
概述Nominated as an outstanding Ph.D thesis by the University of Sydney, New South Wales, Australia.Demonstrates relevance of quantum anomalies for important aspects of modern cosmology.Links particle phy
叢書名稱Springer Theses
圖書封面Titlebook: Cosmological Implications of Quantum Anomalies;  Neil David Barrie Book 2018 Springer Nature Switzerland AG 2018 Baryogenesis.Cosmological
描述.The successes of the standard models of particle physics and cosmology are many, but have proven incapable of explaining all the phenomena that we observe. This book investigates the potentially important role of quantum physics, particularly quantum anomalies, in various aspects of modern cosmology, such as inflation, the dynamical generation of the visible and dark matter in the universe, and gravitational waves. By doing so, the authors demonstrate that exploring the links between cosmology and particle physics is key to helping solve the mysteries of our Universe..
出版日期Book 2018
關(guān)鍵詞Baryogenesis; Cosmological Inflation; Gravitational Waves; Cosmological Reheating; Quantum Anomalies; Gen
版次1
doihttps://doi.org/10.1007/978-3-319-94715-0
isbn_softcover978-3-030-06904-9
isbn_ebook978-3-319-94715-0Series ISSN 2190-5053 Series E-ISSN 2190-5061
issn_series 2190-5053
copyrightSpringer Nature Switzerland AG 2018
The information of publication is updating

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978-3-030-06904-9Springer Nature Switzerland AG 2018
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Springer Theseshttp://image.papertrans.cn/c/image/238919.jpg
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Harald Schoen,Siegfried Schumannf the Universe, but they are incomplete. Many mysteries regarding the workings of nature are yet to be resolved, for which new physics beyond the standard paradigms is required. Examples of these are the properties of neutrinos, the identity and origin of dark matter and dark energy, the origin of t
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Dieter Fuchs,Robert Rohrschneiderse it would have been diluted away by the rapid spacetime expansion. In order to produce a significant asymmetry during inflation, the production rate of baryonic charge must exceed its dilution rate. Despite this challenge, it has been found that inflationary dynamics may be able to support such a
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Wertorientierungen und Parteipr?ferenzch. Unlike the dilution problems associated with inflationary cogenesis considered above, the difficulties with a reheating scenario are related to the high level of uncertainty and complexity of the dynamics associated with the reheating phase. The exact nature of the reheating epoch is mostly unkn
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Wohnsituation nach Trennung und Scheidung,nd the evolution of the universe. Unfortunately, the weakly interacting nature of neutrinos combined with the low temperature of the background today, makes the prospect for detection near impossible in the foreseeable future. Despite this, the dynamics of the C.B could have had significant effects
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