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Titlebook: Oscillations of Disks; Shoji Kato Book 2016 Springer Japan 2016 Corotation Resonance.Discoseismology.Disk Oscillations.Epicyclic Frequenci

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发表于 2025-3-21 16:18:24 | 显示全部楼层 |阅读模式
书目名称Oscillations of Disks
编辑Shoji Kato
视频video
概述Explains the current state of disk-oscillation theory, providing a potentially important tool to accurately determine spins of black hole sources in the universe.Clarifies our current understanding of
丛书名称Astrophysics and Space Science Library
图书封面Titlebook: Oscillations of Disks;  Shoji Kato Book 2016 Springer Japan 2016 Corotation Resonance.Discoseismology.Disk Oscillations.Epicyclic Frequenci
描述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 ch
出版日期Book 2016
关键词Corotation Resonance; Discoseismology; Disk Oscillations; Epicyclic Frequencies; Quasi-Periodic Oscillat
版次1
doihttps://doi.org/10.1007/978-4-431-56208-5
isbn_softcover978-4-431-56779-0
isbn_ebook978-4-431-56208-5Series ISSN 0067-0057 Series E-ISSN 2214-7985
issn_series 0067-0057
copyrightSpringer Japan 2016
The information of publication is updating

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发表于 2025-3-21 23:13:13 | 显示全部楼层
Wave-Wave Resonant Instability in Deformed Diskso et al. (Publ Astron Soc Jpn 63:363, 2011)) formulated the instability in a perspective way. In this chapter, we outline the formulation by Kato (Publ Astron Soc Jpn 65:75, 2013). Applications to time variations in dwarf novae and X-ray binaries are presented in Chap. .
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Frequencies of Trapped Oscillations and Applicationwtonian disks are examined. The oscillation modes examined are one-armed p-mode (one-armed precession mode) and one-armed vertical p-mode (tilt mode). The results are examined whether they can describe positive and negative superhumps in dwarf novae.
发表于 2025-3-22 16:07:41 | 显示全部楼层
Introductionions in accretion disks, focusing on those which will be related to disk oscillations. The main oscillatory phenomena which we focus our attention are V/R variations in Be stars, positive and negative superhumps in dwarf novae, high-frequency quasi-periodic oscillations in neutron-star and black-hole X-ray binaries.
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发表于 2025-3-23 00:03:04 | 显示全部楼层
Wave-Wave Resonant Instability in Deformed Disks: Applicationserhumps. Furthermore, some oscillatory phenomena in X-ray sources might be attributed to this process. In this context we present here attempts to apply the process to describing high-frequency QPOs in X-ray sources, in addition to superhumps.
发表于 2025-3-23 01:34:51 | 显示全部楼层
Corotation Instabilitystron Soc 208:721, 1984) (see Chap. .). This work by Paparoizou and Pringle stimulated many subsequent studies on corotation instability in tori and disks. In this chapter, we will describe the essence of corotation instability in geometrically thin disks by presenting Drury’s work (Mon Not R Astron Soc 217:821, 1985).
发表于 2025-3-23 06:14:26 | 显示全部楼层
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