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Titlebook: Defect Evolution in Cosmology and Condensed Matter; Quantitative Analysi C.J.A.P. Martins Book 2016 The Author(s) 2016 Cosmic strings.Cosmi

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發(fā)表于 2025-3-21 17:59:25 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
書目名稱Defect Evolution in Cosmology and Condensed Matter
副標(biāo)題Quantitative Analysi
編輯C.J.A.P. Martins
視頻videohttp://file.papertrans.cn/265/264714/264714.mp4
概述A comprehensive review of a model widely used to describe the evolution of cosmic strings, an important class of topological defect.Author pioneered the approach himself and demonstrates here its wide
叢書名稱SpringerBriefs in Physics
圖書封面Titlebook: Defect Evolution in Cosmology and Condensed Matter; Quantitative Analysi C.J.A.P. Martins Book 2016 The Author(s) 2016 Cosmic strings.Cosmi
描述This book sheds new light on topological defects in widely differing systems, using the Velocity-Dependent One-Scale Model to better understand their evolution. Topological defects – cosmic strings, monopoles, domain walls or others - necessarily form at cosmological (and condensed matter) phase transitions. If they are stable and long-lived they will be fossil relics of higher-energy physics. Understanding their behaviour and consequences is a key part of any serious attempt to understand the universe, and this requires modelling their evolution. The velocity-dependent one-scale model is the only fully quantitative model of defect network evolution, and the canonical model in the field. This book provides a review of the model, explaining its physical content and describing its broad range of applicability.
出版日期Book 2016
關(guān)鍵詞Cosmic strings; Cosmic superstrings; Defect networks; Domain wall evolution; Field theory simulations; Go
版次1
doihttps://doi.org/10.1007/978-3-319-44553-3
isbn_softcover978-3-319-44551-9
isbn_ebook978-3-319-44553-3Series ISSN 2191-5423 Series E-ISSN 2191-5431
issn_series 2191-5423
copyrightThe Author(s) 2016
The information of publication is updating

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Model Extensions,of superconducting strings and that of wiggly strings. In the former case we obtain the microscopic string equations of motion in the Witten–Carter–Peter superconducting model, finding that whether the standard scale-invariant evolution of the network is preserved or destroyed due to the presence of
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Defects in Condensed Matter,oach and the damped and non-relativistic limits which are relevant for condensed matter physics. We also reproduce experimental results in this context and show that the vortex-string density is significantly reduced by loop production, an effect not included in the usual ‘coarse-grained’ approach.
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2191-5423 ioneered the approach himself and demonstrates here its wideThis book sheds new light on topological defects in widely differing systems, using the Velocity-Dependent One-Scale Model to better understand their evolution. Topological defects – cosmic strings, monopoles, domain walls or others - neces
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