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Defect Evolution in Cosmology and Condensed Matter: Quantitative Analysis With the Velocity-Dependent One-Scale Model (Springerbriefs in Physics) (en Inglés)
C.j.a.p. Martins (Autor)
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Springer
· Tapa Blanda
Defect Evolution in Cosmology and Condensed Matter: Quantitative Analysis With the Velocity-Dependent One-Scale Model (Springerbriefs in Physics) (en Inglés) - C.J.A.P. Martins
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Reseña del libro "Defect Evolution in Cosmology and Condensed Matter: Quantitative Analysis With the Velocity-Dependent One-Scale Model (Springerbriefs in Physics) (en Inglés)"
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.
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