Non-radial Oscillations of Rotating Gaseous Masses PDF Download
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Author: Maurice James Young Clement
Publisher:
ISBN:
Category : Oscillations
Languages : en
Pages :
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Book Description
Author: Maurice James Young Clement
Publisher:
ISBN:
Category : Oscillations
Languages : en
Pages :
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Book Description
Author: Georg P. Horedt
Publisher: Springer Science & Business Media
ISBN: 1402023510
Category : Science
Languages : en
Pages : 731
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Book Description
This book provides the most complete academic treatment on the application of polytropes ever published. It is primarily intended for students and scientists working in Astrophysics and related fields. It provides a full overview of past and present research results and is an indispensible guide for everybody wanting to apply polytropes.
Author: Subrahmanyan Chandrasekhar
Publisher: World Scientific
ISBN: 1860942083
Category : Science
Languages : en
Pages : 1449
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Book Description
This invaluable book presents selected papers of S Chandrasekhar, co-winner of the Nobel Prize for Physics in 1983 and a scientific giant well known for his prolific and monumental contributions to astrophysics, physics and applied mathematics. The reader will find here most of Chandrasekhar's articles that led to major developments in various areas of physics and astrophysics. There are also articles of a popular and historical nature, as well as some hitherto unpublished material based on Chandrasekhar's talks at conferences. Each section of the book contains annotations by the editor.
Author: Pantelis Pnigouras
Publisher: Springer
ISBN: 3319982583
Category : Science
Languages : en
Pages : 235
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Book Description
This book presents a study of the saturation of unstable f-modes (fundamental modes) due to low-order nonlinear mode coupling. Since their theoretical prediction in 1934, neutron stars have remained among the most challenging objects in the Universe. Gravitational waves emitted by unstable neutron star oscillations can be used to obtain information about their inner structure, that is, the equation of state of dense nuclear matter. After its initial growth phase, the instability is expected to saturate due to nonlinear effects. The saturation amplitude of the unstable mode determines the detectability of the generated gravitational-wave signal, but also affects the evolution of the neutron star. The study shows that the unstable (parent) mode resonantly couples to pairs of stable (daughter) modes, which drain the parent’s energy and make it saturate via a mechanism called parametric resonance instability. Further, it calculates the saturation amplitude of the most unstable f-mode multipoles throughout their so-called instability windows.
Author: Subrahmanyan Chandrasekhar
Publisher: University of Chicago Press
ISBN: 9780226101019
Category : Science
Languages : en
Pages : 764
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Book Description
This is the first of six volumes collecting significant papers of the distinguished astrophysicist and Nobel laureate S. Chandrasekhar. His work is notable for its breadth as well as for its brilliance; his practice has been to change his focus from time to time to pursue new areas of research. The result has been a prolific career full of discoveries and insights, some of which are only now being fully appreciated. Chandrasekhar has selected papers that trace the development of his ideas and that present aspects of his work not fully covered in the books he has periodically published to summarize his research in each area.
Author: Paul Smeyers
Publisher: Springer Science & Business Media
ISBN: 3642130305
Category : Science
Languages : en
Pages : 475
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Book Description
This book surveys the theory of free, linear, isentropic oscillations in spherically symmetric, gaseous equilibrium stars, from basic concepts to asymptotic representations of normal modes and with slow period changes in rapidly evolving pulsating stars.
Author: Subrahmanyan Chandrasekhar
Publisher: University of Chicago Press
ISBN: 9780226100968
Category : Psychology
Languages : en
Pages : 616
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Book Description
This is the fourth of six volumes collecting significant papers of the distinguished astrophysicist and Nobel laureate S. Chandrasekhar. His work is notable for its breadth as well as for its brilliance; his practice has been to change his focus from time to time to pursue new areas of research. The result has been a prolific career full of discoveries and insights, some of which are only now being fully appreciated. Chandrasekhar has selected papers that trace the development of his ideas and that present aspects of his work not fully covered in the books he has periodically published to summarize his research in each area. Volume 4 has three parts. The first, on plasma physics, includes joint work with A. N. Kaufman and K. M. Watson on the stability of the pinch, as well as a paper on Chandrasekhar's own approach to the topic of adiabatic invariants. Part 2 includes work with specific scientific applications of hydrodynamic and hydromagnetic stability not covered in his monograph on the subject. The final part contains Chandrasekhar's papers on the scientific applications of the tensor-virial theorem, in which he restores to its proper place Riemann's neglected work with ellipsoidal figures.
Author: Kenneth R. Lang
Publisher: Springer Science & Business Media
ISBN: 3662216426
Category : Science
Languages : en
Pages : 805
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Book Description
This second edition contains corrections of misprints and errors found by the author, as well as those suggested during the Russian translation of the first printing. The Russian editors and translators who kindly supplied this material include V. E. CHERTOPRUD, A. G. DOROSHKEVICH, V. L. HOHLOVA, M. Yu. KHLOPOV, D. K. NADIOZHIN, L. M. ÜZERNOI, I. G. PERSIANTSEV, L. A. POKROVSKII, A. V. ZASOV, and Yu. K. ZEMTSOV. Supplemental references for the period 1974 to 1980 have also been added as appendix where they are included under the headings of general references and specific references for each chapter. Although specialized references come mainly from American journals, references to reviews and books are also included to help guide the reader to other sources. The author encourages suggestions for additions and corrections to possible future editions of this volume. KENNETH R. LANG Department of Physics, Tufts University Medford, Massachusetts January, 1980 Preface This book is meant to be a reference source for the fundamental formulae of astrophysics. Wherever possible, the original source of the material being pre sented is referenced, together with references to more recent modifications and applications. More accessible reprints and translations of the early papers are also referenced. In this way the reader is provided with the often ignored his torical context together with an orientation to the more recent literature.
Author: Kenneth Lang
Publisher: Springer Science & Business Media
ISBN: 3662111888
Category : Science
Languages : en
Pages : 757
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Book Description
This book is meant to be a reference source for the fundamental formulae of astrophysics. Wherever possible, the original source of the material being pre sented is referenced, together with references to more recent modifications and applications. More accessible reprints and translations of the early papers are also referenced. In this way the reader is provided with the often ignored his torical context together with an orientation to the more recent literature. Any omission of a reference is, of course, not meant to reflect on the quality of its contents. In order to present a wide variety of concepts in one volume, a concise style is used and derivations are presented for only the simpler formulae. Ex tensive derivations and explanatory comments may be found in the original references or in the books listed in the selected bibliography which follows. Following the convention in astrophysics, the C. g. S. (centimeter-gram-second) system of units is used unless otherwise noted. To conserve space, the funda mental constants are not always defined, and unless otherwise noted the fol lowing symbols have the following meaning and value. Symbol Meaning Value 10 c Speed of light in vacuum 2. 997924562(11) x 10 cm S-l h=2nh Planck's constant 6. 626196(50) x 10 - 27 erg s Rationalized Planck's constant 1. 0545919(80) x 10- 27 erg s h=h/2n k Boltzmann's constant 1. 380622(59) x 10 - 16 erg K - 1 4.
Author: Subrahmanyan Chandrasekhar
Publisher: University of Chicago Press
ISBN: 9780226100999
Category : Science
Languages : en
Pages : 612
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Book Description
This is the fifth of six volumes collecting significant papers of the distinguished astrophysicist and Nobel laureate S. Chandrasekhar. His work is notable for its breadth as well as for its brilliance; his practice has been to change his focus from time to time to pursue new areas of research. The result has been a prolific career full of discoveries and insights, some of which are only now being fully appreciated. Chandrasekhar has selected papers that trace the development of his ideas and that present aspects of his work not fully covered in the books he has periodically published to summarize his research in each area. Volume 5 covers all of Chandrasekhar's contributions to the general theory of relativity and relativity's astrophysical applications (except his research on black holes and colliding gravitational waves, which is covered in Volume 6). The major topics include the influence of general relativity on the pulsations and stability of stars; the back reaction of gravitational waves on their sources; and post-Newtonian approximations to general relativity and their astrophysical applications. In addition to research papers, the volume includes two 1972 lectures in which Chandrasekhar assessed the past, present, and future of relativistic astrophysics. The foreword by astrophysicist Kip S. Thorne is an absorbing, brief history of the field since 1961, capturing the atmosphere of the early research and clarifying Chandrasekhar's dominant role in it. Chandrasekhar has never written a monograph synthesizing his research in relativistic astrophysics, and therefore this volume of his papers serves as a summary of that work for students and more senior researchers.
