東華大學圖書館 |

語系: 繁體中文

說明(常見問題)

回圖書館首頁

手機版館藏查詢

登入

回首頁

切換: 標籤 | MARC模式 | ISBD

Oscillations of disks

Kato, Shoji.

FindBook

Google Book

Amazon

博客來

Oscillations of disks

紀錄類型:	書目-電子資源 : Monograph/item
正題名/作者:	Oscillations of disks/ by Shoji Kato.
作者:	Kato, Shoji.
出版者:	Tokyo :Springer Japan : : 2016.,
面頁冊數:	xv, 261 p. :ill. (some col.), digital ;24 cm.
內容註:	Introduction -- Basic Quantities Related to Disk Oscillations -- Derivation of Linear Wave Equations and Wave Energy -- Vertical Oscillations -- Disk Oscillations in Radial Direction -- Classification of Oscillations and Their Characteristics -- Frequencies of Trapped Oscillations and Application -- Two Examples of Further Studies on Trapped Oscillations and Application -- Overstability of Oscillations by Viscosity -- Corotation Instability -- Wave-Wave Resonant Instability in Deformed Disks -- Wave-Wave Resonant Instability in Deformed Disks - Applications -- Sonic Point Instability and Stochastic Excitation of Oscillations by Turbulence.
Contained By:	Springer eBooks
標題:	Accretion (Astrophysics) -
電子資源:	http://dx.doi.org/10.1007/978-4-431-56208-5
ISBN:	9784431562085$q(electronic bk.)

Oscillations of disks
Kato, Shoji.

Oscillations of disks[electronic resource] /by Shoji Kato. - Tokyo :Springer Japan :2016. - xv, 261 p. :ill. (some col.), digital ;24 cm. - Astrophysics and space science library,4370067-0057 ;. - Astrophysics and space science library ;437..

Introduction -- Basic Quantities Related to Disk Oscillations -- Derivation of Linear Wave Equations and Wave Energy -- Vertical Oscillations -- Disk Oscillations in Radial Direction -- Classification of Oscillations and Their Characteristics -- Frequencies of Trapped Oscillations and Application -- Two Examples of Further Studies on Trapped Oscillations and Application -- Overstability of Oscillations by Viscosity -- Corotation Instability -- Wave-Wave Resonant Instability in Deformed Disks -- Wave-Wave Resonant Instability in Deformed Disks - Applications -- Sonic Point Instability and Stochastic Excitation of Oscillations by Turbulence.

This book presents the current state of research on disk oscillation theory, focusing on relativistic disks and tidally deformed disks. Since the launch of the Rossi X-ray Timing Explorer (RXTE) in 1996, many high-frequency quasiperiodic oscillations (HFQPOs) have been observed in X-ray binaries. Subsequently, similar quasi-periodic oscillations have been found in such relativistic objects as microquasars, ultra-luminous X-ray sources, and galactic nuclei. One of the most promising explanations of their origin is based on oscillations in relativistic disks, and a new field called discoseismology is currently developing. After reviewing observational aspects, the book presents the basic characteristics of disk oscillations, especially focusing on those in relativistic disks. Relativistic disks are essentially different from Newtonian disks in terms of several basic characteristics of their disk oscillations, including the radial distributions of epicyclic frequencies. In order to understand the basic processes of disk oscillations, studies on binary systems are of importance, as they offer valuable information on wave-wave coupling processes in disk oscillations. Accordingly, some characteristics of oscillations in deformed disks are also presented in this book. The book consists of two parts. Points covered in Part I include, for instance, the basic characteristics of disk oscillations, classification of oscillation modes, and trapping of oscillations. In Part II, the focus is mainly on excitation processes of oscillations, while applications to observations are also discussed.

ISBN: 9784431562085$q(electronic bk.)

Standard No.: 10.1007/978-4-431-56208-5doiSubjects--Topical Terms:

897821
Accretion (Astrophysics)

LC Class. No.: QB466.A25

Dewey Class. No.: 523.01

Oscillations of disks
LDR:03267nmm a2200337 a 4500 001 2051942
003 DE-He213
005 20170314154438.0
006 m d
007 cr nn 008maaau
008 170421s2016 ja s 0 eng d
020 $a 9784431562085$q(electronic bk.)
020 $a 9784431562061$q(paper)
024 7 $a 10.1007/978-4-431-56208-5 $2 doi
035 $a 978-4-431-56208-5
040 $a GP $c GP
041 0 $a eng
050 4 $a QB466.A25
072 7 $a PGC $2 bicssc
072 7 $a SCI004000 $2 bisacsh
072 7 $a SCI005000 $2 bisacsh
082 0 4 $a 523.01 $2 23
090 $a QB466.A25 $b K19 2016
100 1 $a Kato, Shoji. $3 3134761
245 1 0 $a Oscillations of disks $h [electronic resource] / $c by Shoji Kato.
260 $a Tokyo : $b Springer Japan : $b Imprint: Springer, $c 2016.
300 $a xv, 261 p. : $b ill. (some col.), digital ; $c 24 cm.
490 1 $a Astrophysics and space science library, $x 0067-0057 ; $v 437
505 0 $a Introduction -- Basic Quantities Related to Disk Oscillations -- Derivation of Linear Wave Equations and Wave Energy -- Vertical Oscillations -- Disk Oscillations in Radial Direction -- Classification of Oscillations and Their Characteristics -- Frequencies of Trapped Oscillations and Application -- Two Examples of Further Studies on Trapped Oscillations and Application -- Overstability of Oscillations by Viscosity -- Corotation Instability -- Wave-Wave Resonant Instability in Deformed Disks -- Wave-Wave Resonant Instability in Deformed Disks - Applications -- Sonic Point Instability and Stochastic Excitation of Oscillations by Turbulence.
520 $a This book presents the current state of research on disk oscillation theory, focusing on relativistic disks and tidally deformed disks. Since the launch of the Rossi X-ray Timing Explorer (RXTE) in 1996, many high-frequency quasiperiodic oscillations (HFQPOs) have been observed in X-ray binaries. Subsequently, similar quasi-periodic oscillations have been found in such relativistic objects as microquasars, ultra-luminous X-ray sources, and galactic nuclei. One of the most promising explanations of their origin is based on oscillations in relativistic disks, and a new field called discoseismology is currently developing. After reviewing observational aspects, the book presents the basic characteristics of disk oscillations, especially focusing on those in relativistic disks. Relativistic disks are essentially different from Newtonian disks in terms of several basic characteristics of their disk oscillations, including the radial distributions of epicyclic frequencies. In order to understand the basic processes of disk oscillations, studies on binary systems are of importance, as they offer valuable information on wave-wave coupling processes in disk oscillations. Accordingly, some characteristics of oscillations in deformed disks are also presented in this book. The book consists of two parts. Points covered in Part I include, for instance, the basic characteristics of disk oscillations, classification of oscillation modes, and trapping of oscillations. In Part II, the focus is mainly on excitation processes of oscillations, while applications to observations are also discussed.
650 0 $a Accretion (Astrophysics) $3 897821
650 0 $a Oscillations. $3 560896
650 1 4 $a Physics. $3 516296
650 2 4 $a Astronomy, Astrophysics and Cosmology. $3 890823
650 2 4 $a Theoretical, Mathematical and Computational Physics. $3 1066859
650 2 4 $a Planetology. $3 546174
650 2 4 $a Mathematical Applications in the Physical Sciences. $3 1566152
710 2 $a SpringerLink (Online service) $3 836513
773 0 $t Springer eBooks
830 0 $a Astrophysics and space science library ; $v 437. $3 3134762
856 4 0 $u http://dx.doi.org/10.1007/978-4-431-56208-5
950 $a Physics and Astronomy (Springer-11651)