語系:
繁體中文
English
說明(常見問題)
回圖書館首頁
手機版館藏查詢
登入
回首頁
到查詢結果
[ author_sort:"martins, c.j.a.p." ]
切換:
標籤
|
MARC模式
|
ISBD
Defect evolution in cosmology and co...
~
Martins, C.J.A.P.
FindBook
Google Book
Amazon
博客來
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$q(electronic bk.)
Defect evolution in cosmology and condensed matter = quantitative analysis with the velocity-dependent one-scale model /
Martins, C.J.A.P.
Defect evolution in cosmology and condensed matter
quantitative analysis with the velocity-dependent one-scale model /[electronic resource] :by C.J.A.P. Martins. - Cham :Springer International Publishing :2016. - ix, 118 p. :ill., digital ;24 cm. - SpringerBriefs in physics,2191-5423. - SpringerBriefs in physics..
Introduction to Defects -- Cosmic Strings -- Domain Walls -- The Rest of the Zoo -- Model Extensions -- Defects in condensed matter.
This book sheds new light on topological defects in widely differing systems, using the Velocity-Dependent One-Scale Model to better understand their evolution. Topological defects - cosmic strings, monopoles, domain walls or others - necessarily form at cosmological (and condensed matter) phase transitions. If they are stable and long-lived they will be fossil relics of higher-energy physics. Understanding their behaviour and consequences is a key part of any serious attempt to understand the universe, and this requires modelling their evolution. The velocity-dependent one-scale model is the only fully quantitative model of defect network evolution, and the canonical model in the field. This book provides a review of the model, explaining its physical content and describing its broad range of applicability.
ISBN: 9783319445533$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 /
LDR
:01996nmm a2200325 a 4500
001
2051941
003
DE-He213
005
20170314153102.0
006
m d
007
cr nn 008maaau
008
170421s2016 gw s 0 eng d
020
$a
9783319445533$q(electronic bk.)
020
$a
9783319445519$q(paper)
024
7
$a
10.1007/978-3-319-44553-3
$2
doi
035
$a
978-3-319-44553-3
040
$a
GP
$c
GP
041
0
$a
eng
050
4
$a
QB981
072
7
$a
PHR
$2
bicssc
072
7
$a
SCI015000
$2
bisacsh
082
0 4
$a
523.1
$2
23
090
$a
QB981
$b
.M386 2016
100
1
$a
Martins, C.J.A.P.
$3
3134758
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.
260
$a
Cham :
$b
Springer International Publishing :
$b
Imprint: Springer,
$c
2016.
300
$a
ix, 118 p. :
$b
ill., digital ;
$c
24 cm.
490
1
$a
SpringerBriefs in physics,
$x
2191-5423
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.
$3
531904
650
0
$a
Condensed matter.
$3
526213
650
0
$a
Deviation (Mathematics)
$3
3134759
650
1 4
$a
Physics.
$3
516296
650
2 4
$a
Phase Transitions and Multiphase Systems.
$3
1066389
650
2 4
$a
Applications of Graph Theory and Complex Networks.
$3
3134760
710
2
$a
SpringerLink (Online service)
$3
836513
773
0
$t
Springer eBooks
830
0
$a
SpringerBriefs in physics.
$3
1314314
856
4 0
$u
http://dx.doi.org/10.1007/978-3-319-44553-3
950
$a
Physics and Astronomy (Springer-11651)
筆 0 讀者評論
館藏地:
全部
電子資源
出版年:
卷號:
館藏
1 筆 • 頁數 1 •
1
條碼號
典藏地名稱
館藏流通類別
資料類型
索書號
使用類型
借閱狀態
預約狀態
備註欄
附件
W9286594
電子資源
11.線上閱覽_V
電子書
EB QB981
一般使用(Normal)
在架
0
1 筆 • 頁數 1 •
1
多媒體
評論
新增評論
分享你的心得
Export
取書館
處理中
...
變更密碼
登入