語系:
繁體中文
English
日文
簡体中文
說明(常見問題)
登入
回首頁
切換:
標籤
|
MARC模式
|
ISBD
The three-body problem from Pythagor...
~
SpringerLink (Online service)
The three-body problem from Pythagoras to Hawking[electronic resource] /
紀錄類型:
書目-語言資料,印刷品 : Monograph/item
杜威分類號:
521
書名/作者:
The three-body problem from Pythagoras to Hawking/ by Mauri Valtonen ... [et al.].
其他作者:
Valtonen, Mauri.
出版者:
Cham : : Springer International Publishing :, 2016.
面頁冊數:
xi, 173 p. : : ill. (some col.), digital ;; 24 cm.
Contained By:
Springer eBooks
標題:
Three-body problem - Popular works.
標題:
Popular Science.
標題:
Popular Science in Astronomy.
標題:
Classical and Quantum Gravitation, Relativity Theory.
標題:
Dynamical Systems and Ergodic Theory.
標題:
Astrophysics and Astroparticles.
標題:
Mechanics.
標題:
Mathematical Methods in Physics.
ISBN:
9783319227269
ISBN:
9783319227252
內容註:
1 Classical problems -- 2 From Newton to Einstein: the discovery of laws of motion and gravity -- 3 From comets to chaos -- 4 Fractals, entropy and arrow of time -- 5 Solar System -- 6 Interacting galaxies -- 7 Three body problem in perspective -- 8 Black holes and quasars.
摘要、提要註:
This book, written for a general readership, reviews and explains the three-body problem in historical context reaching to latest developments in computational physics and gravitation theory. The three-body problem is one of the oldest problems in science and it is most relevant even in today's physics and astronomy. The long history of the problem from Pythagoras to Hawking parallels the evolution of ideas about our physical universe, with a particular emphasis on understanding gravity and how it operates between astronomical bodies. The oldest astronomical three-body problem is the question how and when the moon and the sun line up with the earth to produce eclipses. Once the universal gravitation was discovered by Newton, it became immediately a problem to understand why these three-bodies form a stable system, in spite of the pull exerted from one to the other. In fact, it was a big question whether this system is stable at all in the long run. Leading mathematicians attacked this problem over more than two centuries without arriving at a definite answer. The introduction of computers in the last half-a-century has revolutionized the study; now many answers have been found while new questions about the three-body problem have sprung up. One of the most recent developments has been in the treatment of the problem in Einstein's General Relativity, the new theory of gravitation which is an improvement on Newton's theory. Now it is possible to solve the problem for three black holes and to test one of the most fundamental theorems of black hole physics, the no-hair theorem, due to Hawking and his co-workers.
電子資源:
http://dx.doi.org/10.1007/978-3-319-22726-9
The three-body problem from Pythagoras to Hawking[electronic resource] /
The three-body problem from Pythagoras to Hawking
[electronic resource] /by Mauri Valtonen ... [et al.]. - Cham :Springer International Publishing :2016. - xi, 173 p. :ill. (some col.), digital ;24 cm.
1 Classical problems -- 2 From Newton to Einstein: the discovery of laws of motion and gravity -- 3 From comets to chaos -- 4 Fractals, entropy and arrow of time -- 5 Solar System -- 6 Interacting galaxies -- 7 Three body problem in perspective -- 8 Black holes and quasars.
This book, written for a general readership, reviews and explains the three-body problem in historical context reaching to latest developments in computational physics and gravitation theory. The three-body problem is one of the oldest problems in science and it is most relevant even in today's physics and astronomy. The long history of the problem from Pythagoras to Hawking parallels the evolution of ideas about our physical universe, with a particular emphasis on understanding gravity and how it operates between astronomical bodies. The oldest astronomical three-body problem is the question how and when the moon and the sun line up with the earth to produce eclipses. Once the universal gravitation was discovered by Newton, it became immediately a problem to understand why these three-bodies form a stable system, in spite of the pull exerted from one to the other. In fact, it was a big question whether this system is stable at all in the long run. Leading mathematicians attacked this problem over more than two centuries without arriving at a definite answer. The introduction of computers in the last half-a-century has revolutionized the study; now many answers have been found while new questions about the three-body problem have sprung up. One of the most recent developments has been in the treatment of the problem in Einstein's General Relativity, the new theory of gravitation which is an improvement on Newton's theory. Now it is possible to solve the problem for three black holes and to test one of the most fundamental theorems of black hole physics, the no-hair theorem, due to Hawking and his co-workers.
ISBN: 9783319227269
Standard No.: 10.1007/978-3-319-22726-9doiSubjects--Topical Terms:
647434
Three-body problem
--Popular works.
LC Class. No.: QB362.T5
Dewey Class. No.: 521
The three-body problem from Pythagoras to Hawking[electronic resource] /
LDR
:02891nam a2200325 a 4500
001
450860
003
DE-He213
005
20161103170345.0
006
m d
007
cr nn 008maaau
008
161210s2016 gw s 0 eng d
020
$a
9783319227269
$q
(electronic bk.)
020
$a
9783319227252
$q
(paper)
024
7
$a
10.1007/978-3-319-22726-9
$2
doi
035
$a
978-3-319-22726-9
040
$a
GP
$c
GP
041
0
$a
eng
050
4
$a
QB362.T5
072
7
$a
WNX
$2
bicssc
072
7
$a
SCI004000
$2
bisacsh
072
7
$a
JNF051040
$2
bisacsh
082
0 4
$a
521
$2
23
090
$a
QB362.T5
$b
T531 2016
245
0 4
$a
The three-body problem from Pythagoras to Hawking
$h
[electronic resource] /
$c
by Mauri Valtonen ... [et al.].
260
$a
Cham :
$b
Springer International Publishing :
$b
Imprint: Springer,
$c
2016.
300
$a
xi, 173 p. :
$b
ill. (some col.), digital ;
$c
24 cm.
505
0
$a
1 Classical problems -- 2 From Newton to Einstein: the discovery of laws of motion and gravity -- 3 From comets to chaos -- 4 Fractals, entropy and arrow of time -- 5 Solar System -- 6 Interacting galaxies -- 7 Three body problem in perspective -- 8 Black holes and quasars.
520
$a
This book, written for a general readership, reviews and explains the three-body problem in historical context reaching to latest developments in computational physics and gravitation theory. The three-body problem is one of the oldest problems in science and it is most relevant even in today's physics and astronomy. The long history of the problem from Pythagoras to Hawking parallels the evolution of ideas about our physical universe, with a particular emphasis on understanding gravity and how it operates between astronomical bodies. The oldest astronomical three-body problem is the question how and when the moon and the sun line up with the earth to produce eclipses. Once the universal gravitation was discovered by Newton, it became immediately a problem to understand why these three-bodies form a stable system, in spite of the pull exerted from one to the other. In fact, it was a big question whether this system is stable at all in the long run. Leading mathematicians attacked this problem over more than two centuries without arriving at a definite answer. The introduction of computers in the last half-a-century has revolutionized the study; now many answers have been found while new questions about the three-body problem have sprung up. One of the most recent developments has been in the treatment of the problem in Einstein's General Relativity, the new theory of gravitation which is an improvement on Newton's theory. Now it is possible to solve the problem for three black holes and to test one of the most fundamental theorems of black hole physics, the no-hair theorem, due to Hawking and his co-workers.
650
0
$a
Three-body problem
$v
Popular works.
$3
647434
650
1 4
$a
Popular Science.
$3
464189
650
2 4
$a
Popular Science in Astronomy.
$3
464217
650
2 4
$a
Classical and Quantum Gravitation, Relativity Theory.
$3
464246
650
2 4
$a
Dynamical Systems and Ergodic Theory.
$3
464934
650
2 4
$a
Astrophysics and Astroparticles.
$3
465672
650
2 4
$a
Mechanics.
$3
189082
650
2 4
$a
Mathematical Methods in Physics.
$3
464098
700
1
$a
Valtonen, Mauri.
$3
647433
710
2
$a
SpringerLink (Online service)
$3
463450
773
0
$t
Springer eBooks
856
4 0
$u
http://dx.doi.org/10.1007/978-3-319-22726-9
950
$a
Physics and Astronomy (Springer-11651)
筆 0 讀者評論
多媒體
多媒體檔案
http://dx.doi.org/10.1007/978-3-319-22726-9
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