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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...
| Clasificación: | Libro Electrónico |
|---|---|
| Autor principal: | |
| Autor Corporativo: | |
| Formato: | Electrónico eBook |
| Idioma: | Inglés |
| Publicado: |
Cham :
Springer International Publishing : Imprint: Springer,
2016.
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| Edición: | 1st ed. 2016. |
| Colección: | SpringerBriefs in Physics,
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| Temas: | |
| Acceso en línea: | Texto Completo |
MARC
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| 008 | 160903s2016 sz | s |||| 0|eng d | ||
| 020 | |a 9783319445533 |9 978-3-319-44553-3 | ||
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| 100 | 1 | |a Martins, C.J.A.P. |e author. |4 aut |4 http://id.loc.gov/vocabulary/relators/aut | |
| 245 | 1 | 0 | |a Defect Evolution in Cosmology and Condensed Matter |h [electronic resource] : |b Quantitative Analysis with the Velocity-Dependent One-Scale Model / |c by C.J.A.P. Martins. |
| 250 | |a 1st ed. 2016. | ||
| 264 | 1 | |a Cham : |b Springer International Publishing : |b Imprint: Springer, |c 2016. | |
| 300 | |a IX, 118 p. |b online resource. | ||
| 336 | |a text |b txt |2 rdacontent | ||
| 337 | |a computer |b c |2 rdamedia | ||
| 338 | |a online resource |b cr |2 rdacarrier | ||
| 347 | |a text file |b PDF |2 rda | ||
| 490 | 1 | |a SpringerBriefs in Physics, |x 2191-5431 | |
| 505 | 0 | |a Introduction to Defects -- Cosmic Strings -- Domain Walls -- The Rest of the Zoo -- Model Extensions -- Defects in condensed matter. | |
| 520 | |a 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. | ||
| 650 | 0 | |a Cosmology. | |
| 650 | 0 | |a Condensed matter. | |
| 650 | 0 | |a Graph theory. | |
| 650 | 1 | 4 | |a Cosmology. |
| 650 | 2 | 4 | |a Phase Transitions and Multiphase Systems. |
| 650 | 2 | 4 | |a Graph Theory. |
| 710 | 2 | |a SpringerLink (Online service) | |
| 773 | 0 | |t Springer Nature eBook | |
| 776 | 0 | 8 | |i Printed edition: |z 9783319445519 |
| 776 | 0 | 8 | |i Printed edition: |z 9783319445526 |
| 830 | 0 | |a SpringerBriefs in Physics, |x 2191-5431 | |
| 856 | 4 | 0 | |u https://doi.uam.elogim.com/10.1007/978-3-319-44553-3 |z Texto Completo |
| 912 | |a ZDB-2-PHA | ||
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| 950 | |a Physics and Astronomy (SpringerNature-11651) | ||
| 950 | |a Physics and Astronomy (R0) (SpringerNature-43715) | ||