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Defect Evolution in Cosmology and Co...
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Martins, C.J.A.P.
Defect Evolution in Cosmology and Condensed Matter = Quantitative Analysis with the Velocity-Dependent One-Scale Model /
紀錄類型:
書目-語言資料,印刷品 : Monograph/item
正題名/作者:
Defect Evolution in Cosmology and Condensed Matter/ by C.J.A.P. Martins.
其他題名:
Quantitative Analysis with the Velocity-Dependent One-Scale Model /
作者:
Martins, C.J.A.P.
面頁冊數:
IX, 118 p.online resource. :
Contained By:
Springer Nature eBook
標題:
Cosmology. -
電子資源:
https://doi.org/10.1007/978-3-319-44553-3
ISBN:
9783319445533
Defect Evolution in Cosmology and Condensed Matter = Quantitative Analysis with the Velocity-Dependent One-Scale Model /
Martins, C.J.A.P.
Defect Evolution in Cosmology and Condensed Matter
Quantitative Analysis with the Velocity-Dependent One-Scale Model /[electronic resource] :by C.J.A.P. Martins. - 1st ed. 2016. - IX, 118 p.online resource. - SpringerBriefs in Physics,2191-5423. - SpringerBriefs in Physics,.
Introduction to Defects -- Cosmic Strings -- Domain Walls -- The Rest of the Zoo -- Model Extensions -- Defects in condensed matter.
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.
ISBN: 9783319445533
Standard No.: 10.1007/978-3-319-44553-3doiSubjects--Topical Terms:
579761
Cosmology.
LC Class. No.: QB980-991
Dewey Class. No.: 523.1
Defect Evolution in Cosmology and Condensed Matter = Quantitative Analysis with the Velocity-Dependent One-Scale Model /
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