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Defect evolution in cosmology and condensed matter: quantitative analysis with the velocity-dependent one-scale model
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 tra...
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| Lenguaje: | eng |
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Springer
2016
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| Acceso en línea: | https://dx.doi.org/10.1007/978-3-319-44553-3 http://cds.cern.ch/record/2221162 |