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Defect Evolution in Cosmology and Condensed Matter : Quantitative Analysis With the Velocity-dependent
About this item
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.
Series Title: Springerbriefs in Physics
Publisher: Springer Verlag
Author: Carlos Martins
Street Date: October 4, 2016
Item Number (DPCI): 248-29-2688
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