國立高雄大學圖資館 |

語系: 繁體中文

說明(常見問題)

圖資館首頁

登入

回首頁 到查詢結果 [ subject:"Dark energy (Astronomy)" ]

切換: 標籤 | MARC模式 | ISBD

Kepler problem in the presence of da...

Chernin, Arthur.

Kepler problem in the presence of dark energy, and the cosmic local flow

紀錄類型:	書目-電子資源 : Monograph/item
正題名/作者:	Kepler problem in the presence of dark energy, and the cosmic local flowby Alexander Silbergleit, Arthur Chernin.
作者:	Silbergleit, Alexander.
其他作者:	Chernin, Arthur.
出版者:	Cham :Springer International Publishing :2019.
面頁冊數:	viii, 68 p. :ill., digital ;24 cm.
Contained By:	Springer eBooks
標題:	Dark energy (Astronomy)Congresses.
電子資源:	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)