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Defect evolution in cosmology and co...

Martins, C.J.A.P.

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Defect evolution in cosmology and condensed matter = quantitative analysis with the velocity-dependent one-scale model /

紀錄類型:	書目-電子資源 : Monograph/item
正題名/作者:	Defect evolution in cosmology and condensed matter/ by C.J.A.P. Martins.
其他題名:	quantitative analysis with the velocity-dependent one-scale model /
作者:	Martins, C.J.A.P.
出版者:	Cham :Springer International Publishing : : 2016.,
面頁冊數:	ix, 118 p. :ill., digital ;24 cm.
內容註:	Introduction to Defects -- Cosmic Strings -- Domain Walls -- The Rest of the Zoo -- Model Extensions -- Defects in condensed matter.
Contained By:	Springer eBooks
標題:	Cosmology. -
電子資源:	http://dx.doi.org/10.1007/978-3-319-44553-3
ISBN:	9783319445533$q(electronic bk.)

Defect evolution in cosmology and condensed matter = quantitative analysis with the velocity-dependent one-scale model /
Martins, C.J.A.P.

Defect evolution in cosmology and condensed matterquantitative analysis with the velocity-dependent one-scale model /[electronic resource] :by C.J.A.P. Martins. - Cham :Springer International Publishing :2016. - ix, 118 p. :ill., digital ;24 cm. - SpringerBriefs in physics,2191-5423. - SpringerBriefs in physics..

Introduction to Defects -- Cosmic Strings -- Domain Walls -- The Rest of the Zoo -- Model Extensions -- Defects in condensed matter.

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.

ISBN: 9783319445533$q(electronic bk.)

Standard No.: 10.1007/978-3-319-44553-3doiSubjects--Topical Terms:

531904
Cosmology.

LC Class. No.: QB981

Dewey Class. No.: 523.1

Defect evolution in cosmology and condensed matter = quantitative analysis with the velocity-dependent one-scale model /
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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.
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