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Titlebook: Linear Isentropic Oscillations of Stars; Theoretical Foundati Paul Smeyers,Tim Van Hoolst Book 2010 Springer-Verlag Berlin Heidelberg 2010

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發(fā)表于 2025-3-21 17:59:54 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
書(shū)目名稱(chēng)Linear Isentropic Oscillations of Stars
副標(biāo)題Theoretical Foundati
編輯Paul Smeyers,Tim Van Hoolst
視頻videohttp://file.papertrans.cn/587/586333/586333.mp4
概述Provides a comprehensive presentation of the fundamental aspects of the theory of the linear, isentropic oscillations in spherically symmetric stars Intermediate steps in the mathematical derivations
叢書(shū)名稱(chēng)Astrophysics and Space Science Library
圖書(shū)封面Titlebook: Linear Isentropic Oscillations of Stars; Theoretical Foundati Paul Smeyers,Tim Van Hoolst Book 2010 Springer-Verlag Berlin Heidelberg 2010
描述The study of stellar oscillations is the preeminent way to investigate the stability of stars and to interpret their variability. The theory of the linear, isentropic oscillations of isolated gaseous stars, and thus of compressible spherically symmetric equilibrium configurations, has largely been developed from the viewpoint of the hypothesis of the physical radial pulsations of stars. Written for doctoral students and researchers, this monograph aims to provide a systematic and consistent survey of the fundamentals of the theory of free, linear, isentropic oscillations in spherically symmetric, gaseous equilibrium stars. The first part of the book presents basic concepts and equations, the distinction between spheroidal and toroidal normal modes, the solution of Poisson’s differential equation for the perturbation of the gravitational potential, and Hamilton’s variational principle. The second part is devoted to the possible existence of waves propagating in the radial direction, theorigin and classification of normal modes, the completeness of the normal modes, and the relation between the local stability with respect to convection and the global stability of a star. The third p
出版日期Book 2010
關(guān)鍵詞Asteroseismology; Cepheids; Convective core; Helioseismology; Star; Stellar oscillations; Stellar pulsatio
版次1
doihttps://doi.org/10.1007/978-3-642-13030-4
isbn_softcover978-3-642-26612-6
isbn_ebook978-3-642-13030-4Series ISSN 0067-0057 Series E-ISSN 2214-7985
issn_series 0067-0057
copyrightSpringer-Verlag Berlin Heidelberg 2010
The information of publication is updating

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Book 2010near, isentropic oscillations of isolated gaseous stars, and thus of compressible spherically symmetric equilibrium configurations, has largely been developed from the viewpoint of the hypothesis of the physical radial pulsations of stars. Written for doctoral students and researchers, this monograp
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at the main leaders in the field have collaborated in a proj.Cataract surgery, with 25-30 million surgeries per year, has become one of most popular surgeries in the world. The calculation of its power is of utmost importance. As new premium intraocular lenses (IOLs) and modern surgical?techniques?h
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Paul Smeyersludes surgical pearls, tips and tricks for junior doctors.This book instructs postgraduate trainees inophthalmology on the basic methodology required to perform intraocular surgery.The text is written clearly and concisely, investigating basic surgical skillsfor the eye to facilitate the training pr
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Paul Smeyersuids such as aqueous humour, and blood. Solid and liquid materials have inherent physical properties related to their components like elasticity, viscosity and density. Such properties determine the materials’ interaction and behaviour. Computation of the extent of displacement, deformation and stra
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Paul Smeyersdisciplinary in the ophthalmology and neurology, new questions about the essence of POAG have been raised. Is POAG just an ocular disease? Is it a disease which involves the eye first and then the whole visual pathway? Or sometimes is it an ocular manifestation of a particular central nervous system
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發(fā)表于 2025-3-23 09:35:44 | 只看該作者
Paul Smeyerss and specific visual field change caused by increased intraocular pressure (IOP). However, when we comprehended the development and progress of glaucoma only limiting to the perspective of the eye itself, we could hardly interpret some problems we encountered clinically. For example, some glaucoma
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