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Oscillations of Disks - Shoji Kato

Oscillations of Disks (eBook)

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2016 | 1st ed. 2016
XV, 261 Seiten
Springer Tokyo (Verlag)
978-4-431-56208-5 (ISBN)
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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.



Prof. Shoji Kato
Emeritus professor, Department of Astronomy, Kyoto University
 


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 orderto 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.

Prof. Shoji Kato Emeritus professor, Department of Astronomy, Kyoto University  

Erscheint lt. Verlag 26.9.2016
Reihe/Serie Astrophysics and Space Science Library
Astrophysics and Space Science Library
Zusatzinfo XV, 261 p. 49 illus., 6 illus. in color.
Verlagsort Tokyo
Sprache englisch
Themenwelt Mathematik / Informatik Mathematik
Naturwissenschaften Geowissenschaften Geologie
Naturwissenschaften Physik / Astronomie Astronomie / Astrophysik
Technik
Schlagworte Corotation Resonance • Discoseismology • Disk Oscillations • Epicyclic Frequencies • Quasi-Periodic Oscillations • Trapped Oscillations
ISBN-10 4-431-56208-7 / 4431562087
ISBN-13 978-4-431-56208-5 / 9784431562085
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