Defect evolution in cosmology and condensed matter : quantitative analysis with the velocity-dependent one-scale model 的封面图片
Defect evolution in cosmology and condensed matter : quantitative analysis with the velocity-dependent one-scale model
題名:
Defect evolution in cosmology and condensed matter : quantitative analysis with the velocity-dependent one-scale model
著者:
Martins, C. J. A. P., (Carlos J. A. P.)
ISBN(國際標準書號):
9783319445519
出版資訊:
Switzerland : Springer, c2016.
規格:
ix, 118 p. : ill. ; 24 cm
叢書:
SpringerBriefs in physics

SpringerBriefs in physics.
叢書題名:
SpringerBriefs in physics

SpringerBriefs in physics.
內容:
Introduction to Defects -- Cosmic Strings -- Domain Walls -- The Rest of the Zoo -- Model Extensions -- Defects in condensed matter.
摘要:
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.
主題:
Cosmology.
Condensed matter.
Deviation (Mathematics)
摘要:
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.