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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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发表于 2025-3-21 20:02:06 | 显示全部楼层 |阅读模式
书目名称Cosmological Implications of Quantum Anomalies
编辑Neil David Barrie
视频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
丛书名称Springer Theses
图书封面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
关键词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
Audiometry
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Wertorientierungen und Parteipräferenzch. 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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