Language:
English
繁體中文
Help
圖資館首頁
Login
Back
Switch To:
Labeled
|
MARC Mode
|
ISBD
Kepler problem in the presence of da...
~
Chernin, Arthur.
Kepler problem in the presence of dark energy, and the cosmic local flow
Record Type:
Electronic resources : Monograph/item
Title/Author:
Kepler problem in the presence of dark energy, and the cosmic local flowby Alexander Silbergleit, Arthur Chernin.
Author:
Silbergleit, Alexander.
other author:
Chernin, Arthur.
Published:
Cham :Springer International Publishing :2019.
Description:
viii, 68 p. :ill., digital ;24 cm.
Contained By:
Springer eBooks
Subject:
Dark energy (Astronomy)Congresses.
Online resource:
https://doi.org/10.1007/978-3-030-36752-7
ISBN:
9783030367527$q(electronic bk.)
Kepler problem in the presence of dark energy, and the cosmic local flow
Silbergleit, Alexander.
Kepler problem in the presence of dark energy, and the cosmic local flow
[electronic resource] /by Alexander Silbergleit, Arthur Chernin. - Cham :Springer International Publishing :2019. - viii, 68 p. :ill., digital ;24 cm. - SpringerBriefs in physics,2191-5423. - SpringerBriefs in physics..
Introduction -- Two-Body Problem with Dark Energy -- Radial Motions: Exact Solution and Its Analysis -- Orbital (Planar) Motions: Exact Solution and Its Analysis -- All Motions: Summary. Locality and Stability of Finite Motions -- Dark Energy and the Local Cosmic Flow -- Concluding Remarks.
This book derives and analyzes all solutions to the Kepler problem with dark energy (DE), presenting significant results such as: (a) all radial infinite motions obey Hubble's law at large times; (b) all orbital infinite motions are asymptotically radial and obey Hubble's law; (c) infinite orbital motions strongly dominate the finite ones. This clearly shows the effect of repulsive DE: In the classical Kepler problem, all orbital motions are finite for negative energies and infinite in the opposite case. Another DE effect is spatial localization of bounded orbits: mostly, they are within the equilibrium sphere, where the attractive Newtonian force outbalances the repulsive force of DE.This problem is of particular current interest due to recent studies of the local flows of galaxies showing domination of DE in their dynamics; the book discusses this observation in detail.
ISBN: 9783030367527$q(electronic bk.)
Standard No.: 10.1007/978-3-030-36752-7doiSubjects--Topical Terms:
451535
Dark energy (Astronomy)
--Congresses.
LC Class. No.: QB791.3 / .S55 2019
Dewey Class. No.: 523.1126
Kepler problem in the presence of dark energy, and the cosmic local flow
LDR
:02238nmm a2200337 a 4500
001
569723
003
DE-He213
005
20191129114030.0
006
m d
007
cr nn 008maaau
008
200723s2019 gw s 0 eng d
020
$a
9783030367527$q(electronic bk.)
020
$a
9783030367510$q(paper)
024
7
$a
10.1007/978-3-030-36752-7
$2
doi
035
$a
978-3-030-36752-7
040
$a
GP
$c
GP
041
0
$a
eng
050
4
$a
QB791.3
$b
.S55 2019
072
7
$a
PHR
$2
bicssc
072
7
$a
SCI015000
$2
bisacsh
072
7
$a
PHR
$2
thema
082
0 4
$a
523.1126
$2
23
090
$a
QB791.3
$b
.S582 2019
100
1
$a
Silbergleit, Alexander.
$3
855845
245
1 0
$a
Kepler problem in the presence of dark energy, and the cosmic local flow
$h
[electronic resource] /
$c
by Alexander Silbergleit, Arthur Chernin.
260
$a
Cham :
$b
Springer International Publishing :
$b
Imprint: Springer,
$c
2019.
300
$a
viii, 68 p. :
$b
ill., digital ;
$c
24 cm.
490
1
$a
SpringerBriefs in physics,
$x
2191-5423
505
0
$a
Introduction -- Two-Body Problem with Dark Energy -- Radial Motions: Exact Solution and Its Analysis -- Orbital (Planar) Motions: Exact Solution and Its Analysis -- All Motions: Summary. Locality and Stability of Finite Motions -- Dark Energy and the Local Cosmic Flow -- Concluding Remarks.
520
$a
This book derives and analyzes all solutions to the Kepler problem with dark energy (DE), presenting significant results such as: (a) all radial infinite motions obey Hubble's law at large times; (b) all orbital infinite motions are asymptotically radial and obey Hubble's law; (c) infinite orbital motions strongly dominate the finite ones. This clearly shows the effect of repulsive DE: In the classical Kepler problem, all orbital motions are finite for negative energies and infinite in the opposite case. Another DE effect is spatial localization of bounded orbits: mostly, they are within the equilibrium sphere, where the attractive Newtonian force outbalances the repulsive force of DE.This problem is of particular current interest due to recent studies of the local flows of galaxies showing domination of DE in their dynamics; the book discusses this observation in detail.
650
0
$a
Dark energy (Astronomy)
$v
Congresses.
$3
451535
650
0
$a
Kepler's equation.
$3
855847
650
1 4
$a
Cosmology.
$3
228629
650
2 4
$a
Classical and Quantum Gravitation, Relativity Theory.
$3
376367
700
1
$a
Chernin, Arthur.
$3
855846
710
2
$a
SpringerLink (Online service)
$3
273601
773
0
$t
Springer eBooks
830
0
$a
SpringerBriefs in physics.
$3
557827
856
4 0
$u
https://doi.org/10.1007/978-3-030-36752-7
950
$a
Physics and Astronomy (Springer-11651)
based on 0 review(s)
ALL
電子館藏
Items
1 records • Pages 1 •
1
Inventory Number
Location Name
Item Class
Material type
Call number
Usage Class
Loan Status
No. of reservations
Opac note
Attachments
000000177784
電子館藏
1圖書
電子書
EB QB791.3 .S582 2019 2019
一般使用(Normal)
On shelf
0
1 records • Pages 1 •
1
Multimedia
Multimedia file
https://doi.org/10.1007/978-3-030-36752-7
Reviews
Add a review
and share your thoughts with other readers
Export
pickup library
Processing
...
Change password
Login