語系:
繁體中文
English
說明(常見問題)
圖資館首頁
登入
回首頁
切換:
標籤
|
MARC模式
|
ISBD
Secular evolution of self-gravitatin...
~
Fouvry, Jean-Baptiste.
Secular evolution of self-gravitating systems over cosmic age
紀錄類型:
書目-電子資源 : Monograph/item
正題名/作者:
Secular evolution of self-gravitating systems over cosmic ageby Jean-Baptiste Fouvry.
作者:
Fouvry, Jean-Baptiste.
出版者:
Cham :Springer International Publishing :2017.
面頁冊數:
xv, 274 p. :ill., digital ;24 cm.
Contained By:
Springer eBooks
標題:
GalaxiesEvolution.
電子資源:
http://dx.doi.org/10.1007/978-3-319-66760-7
ISBN:
9783319667607$q(electronic bk.)
Secular evolution of self-gravitating systems over cosmic age
Fouvry, Jean-Baptiste.
Secular evolution of self-gravitating systems over cosmic age
[electronic resource] /by Jean-Baptiste Fouvry. - Cham :Springer International Publishing :2017. - xv, 274 p. :ill., digital ;24 cm. - Springer theses,2190-5053. - Springer theses..
Introduction -- Secular Diffusion -- Razor-thin Discs -- Razor-thin Discs and Swing Amplification -- Thickened Discs -- Quasi-Keplerian Systems -- Conclusion.
Tackling galactic evolution in a truly novel way, this outstanding thesis statistically explores the long-term evolution of galaxies, using recent theoretical breakthroughs that explicitly account for their self-gravity. While treating processes statistically, the astrophysical differences on each scale are also captured. As the archetype of self-amplified diffusion, the implications of the thesis go far beyond astrophysics. Gravity is the driving force in galaxies, from their far outskirts to their innermost cores. These "extended kinetic theories" offer unique physical insights into the competing dynamical processes at play, complementing N-body approaches. The thesis successfully gauges the role of nature and nurture in est ablishing the galaxies' observed properties, using kinetic equations to capture both sources of fluctuations. Further, it shows how secular diffusion shapes the phase space structure of cold stellar disks. The thesis subsequently determines the characteristic timescales and examines the signatures of secular evolution in this framework on two scales: from the kinetic evolution in galactic disks and their thickening via giant molecular clouds; all the way down to the stellar resonant relaxation of the central cluster and its black hole.
ISBN: 9783319667607$q(electronic bk.)
Standard No.: 10.1007/978-3-319-66760-7doiSubjects--Topical Terms:
267029
Galaxies
--Evolution.
LC Class. No.: QB857.5.E96
Dewey Class. No.: 523.112
Secular evolution of self-gravitating systems over cosmic age
LDR
:02433nmm a2200325 a 4500
001
523718
003
DE-He213
005
20180430104315.0
006
m d
007
cr nn 008maaau
008
180628s2017 gw s 0 eng d
020
$a
9783319667607$q(electronic bk.)
020
$a
9783319667591$q(paper)
024
7
$a
10.1007/978-3-319-66760-7
$2
doi
035
$a
978-3-319-66760-7
040
$a
GP
$c
GP
041
0
$a
eng
050
4
$a
QB857.5.E96
072
7
$a
PHVB
$2
bicssc
072
7
$a
SCI005000
$2
bisacsh
082
0 4
$a
523.112
$2
23
090
$a
QB857.5.E96
$b
F782 2017
100
1
$a
Fouvry, Jean-Baptiste.
$3
795076
245
1 0
$a
Secular evolution of self-gravitating systems over cosmic age
$h
[electronic resource] /
$c
by Jean-Baptiste Fouvry.
260
$a
Cham :
$b
Springer International Publishing :
$b
Imprint: Springer,
$c
2017.
300
$a
xv, 274 p. :
$b
ill., digital ;
$c
24 cm.
490
1
$a
Springer theses,
$x
2190-5053
505
0
$a
Introduction -- Secular Diffusion -- Razor-thin Discs -- Razor-thin Discs and Swing Amplification -- Thickened Discs -- Quasi-Keplerian Systems -- Conclusion.
520
$a
Tackling galactic evolution in a truly novel way, this outstanding thesis statistically explores the long-term evolution of galaxies, using recent theoretical breakthroughs that explicitly account for their self-gravity. While treating processes statistically, the astrophysical differences on each scale are also captured. As the archetype of self-amplified diffusion, the implications of the thesis go far beyond astrophysics. Gravity is the driving force in galaxies, from their far outskirts to their innermost cores. These "extended kinetic theories" offer unique physical insights into the competing dynamical processes at play, complementing N-body approaches. The thesis successfully gauges the role of nature and nurture in est ablishing the galaxies' observed properties, using kinetic equations to capture both sources of fluctuations. Further, it shows how secular diffusion shapes the phase space structure of cold stellar disks. The thesis subsequently determines the characteristic timescales and examines the signatures of secular evolution in this framework on two scales: from the kinetic evolution in galactic disks and their thickening via giant molecular clouds; all the way down to the stellar resonant relaxation of the central cluster and its black hole.
650
0
$a
Galaxies
$x
Evolution.
$3
267029
650
1 4
$a
Physics.
$3
179414
650
2 4
$a
Astrophysics and Astroparticles.
$3
376943
650
2 4
$a
Cosmology.
$3
228629
710
2
$a
SpringerLink (Online service)
$3
273601
773
0
$t
Springer eBooks
830
0
$a
Springer theses.
$3
557607
856
4 0
$u
http://dx.doi.org/10.1007/978-3-319-66760-7
950
$a
Physics and Astronomy (Springer-11651)
筆 0 讀者評論
全部
電子館藏
館藏
1 筆 • 頁數 1 •
1
條碼號
館藏地
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
000000148027
電子館藏
1圖書
電子書
EB QB857.5.E96 F782 2017
一般使用(Normal)
在架
0
1 筆 • 頁數 1 •
1
多媒體
多媒體檔案
http://dx.doi.org/10.1007/978-3-319-66760-7
評論
新增評論
分享你的心得
Export
取書館別
處理中
...
變更密碼
登入