While it seems possible to present a fairly complete uni?ed theory of undistorted polytropes, as attempted in the previous chapter, the theory of distorted polytropes is much more extended and - phisticated, so that I present merely a brief overview of the theories that seem to me most interesting and important. Basically, the methods proposed to study the hydrostatic equilibrium of a distorted self-gravitating mass can be divided into two major groups (Blinnikov 1975): (i) Analytic or semia- lytic methods using a small parameter connected with the distortion of the polytrope. (ii) More or less accurate numerical methods. Lyapunov and later Carleman (see Jardetzky 1958, p. 13) have demonstrated that a sphere is a unique solution to the problem of hydrostatic equilibrium for a ?uid mass at rest in tridimensional space. The problem complicates enormously if the sphere is rotating rigidly or di?erentially in space round an axis, and/or if it is distorted magnetically or tidally. Even for the simplest case of a uniformly rotating ?uid body with constant density not all possible solutions have been found (Zharkov and Trubitsyn 1978, p. 222). The sphere becomes an oblate ?gure, and we have no a priori knowledge of its strati?cation, boundary shape, planes of symmetry, transfer of angular momentum in di?erentially rotating bodies, etc.
Le informazioni nella sezione "Riassunto" possono far riferimento a edizioni diverse di questo titolo.
1: Polytropic and Adiabatic Processes. 1.1. Basic Concepts. 1.2. Polytropic and Adiabatic Processes in a Perfect Gas. 1.3. Polytropic Processes for a General Equation of State. 1.4. Adiabatic Processes in a Mixture of Black Body Radiation and Perfect Gas. 1.5. Adiabatic Processes in a Mixture of Electron-Positron Pairs and Black Body Radiation. 1.6. Adiabatic Processes in a Completely Degenerate Electron or Neutron Gas. 1.7. Numerical Survey of Equations of State, Adiabatic Exponents, and Polytropic Indices. 1.8. Emden's Theorem. 2: Undistorted Polytropes. 2.1. General Differential Equations. 2.2. The Homology Theorem and Transformations of the Lane-Emden Equation. 2.3. Exact Analytical Solutions of the Lane-Emden Equation. 2.4. Approximate Analytical Solutions. 2.5. Exact Numerical Solutions. 2.6. Physical Characteristics of Undistorted Polytropes. 2.7. Topology of the Lane-Emden Equation. 2.8. Composite and Other Spherical Polytropes. 3: Distorted Polytropes. 3.1. Introduction. 3.2. Chandrasekhar's First Order Theory of Rotationally Distorted Spheres. 3.3. Chandrasekhar's First Order Theory of Tidally Distorted Polytropes. 3.4. Chandrasekhar's Double Star Problem. 3.5. Second Order Extension of Chandrasekhar's Theory to Differentially Rotating Polytropes. 3.6. Double Approximation Method for Rotationally and Tidally Distorted Polytropic Spheres. 3.7. Second Order Level Surface Theory of Rotationally Distorted Polytropes. 3.8. Numerical and Semmumerical Methods Concernmg Distorted Polytropic Spheres. 3.9. Rotating Polytropic Cylinders and Polytropic Rings. 4: Relativistic Polytropes. 4.1. Undistorted Relativistic Polytropes. 4.2. Rotationally Distorted Relativistic Polytropes. 5: Stability and Oscillations. 5.1. Definitions and General Considerations. 5.2. Basic Equations. 5.3. Radial Oscillations of Polytropic Spheres. 5.4. Instability of Truncated Polytropes. 5.5. Nonradial Oscillations of Polytropic Spheres. 5.6. Stability and Oscillations of Polytropic Cylinders. 5.7. Oscillations and Stability of Rotationally and Tidally Distorted Polytropic Spheres. 5.8. The Virial Method for Rotating Polytropes. 5.9. Stability and Oscillations of Rotating Polytropic Cylinders. 5.10. Stability and Oscillations of Rotating Slabs and Disks. 5.11. Stability and Oscillations of Magnetopolytropes. 5.12. Stability and Oscillations of Relativistic Polytropes. 6: Further Applications to Polytropes. 6.1. Applications to Stars and Stellar Systems. 6.2. Polytropic Atmospheres, Polytropic Clouds and Cores, Embedded Polytropes. 6.3. Polytropic Winds. 6.4. Polytropic Accretion Flows, Accretion Disks and Tori. Acknowledgments. Appendix A. Appendix B. Appendix C. References and Author Index. Subject Index.
Book by Horedt Georg P
Le informazioni nella sezione "Su questo libro" possono far riferimento a edizioni diverse di questo titolo.
EUR 10,24 per la spedizione da U.S.A. a Italia
Destinazione, tempi e costiEUR 10,30 per la spedizione da Regno Unito a Italia
Destinazione, tempi e costiDa: -OnTimeBooks-, Phoenix, AZ, U.S.A.
Condizione: good. A copy that has been read, remains in good condition. All pages are intact, and the cover is intact. The spine and cover show signs of wear. Pages can include notes and highlighting and show signs of wear, and the copy can include "From the library of" labels or previous owner inscriptions. 100% GUARANTEE! Shipped with delivery confirmation, if youâre not satisfied with purchase please return item for full refund. Ships via media mail. Codice articolo OTV.1402023502.G
Quantità: 1 disponibili
Da: Better World Books, Mishawaka, IN, U.S.A.
Condizione: Good. 1st Edition. Former library book; may include library markings. Used book that is in clean, average condition without any missing pages. Codice articolo 16339175-20
Quantità: 1 disponibili
Da: Ria Christie Collections, Uxbridge, Regno Unito
Condizione: New. In. Codice articolo ria9781402023507_new
Quantità: Più di 20 disponibili
Da: moluna, Greven, Germania
Condizione: New. 1: Polytropic and Adiabatic Processes. 1.1. Basic Concepts. 1.2. Polytropic and Adiabatic Processes in a Perfect Gas. 1.3. Polytropic Processes for a General Equation of State. 1.4. Adiabatic Processes in a Mixture of Black Body Radiation and Perfect Gas. 1. Codice articolo 65999975
Quantità: Più di 20 disponibili
Da: GreatBookPrices, Columbia, MD, U.S.A.
Condizione: New. Codice articolo 6362882-n
Quantità: 15 disponibili
Da: GreatBookPrices, Columbia, MD, U.S.A.
Condizione: As New. Unread book in perfect condition. Codice articolo 6362882
Quantità: 15 disponibili
Da: Grand Eagle Retail, Mason, OH, U.S.A.
Hardcover. Condizione: new. Hardcover. While it seems possible to present a fairly complete uni?ed theory of undistorted polytropes, as attempted in the previous chapter, the theory of distorted polytropes is much more extended and - phisticated, so that I present merely a brief overview of the theories that seem to me most interesting and important. Basically, the methods proposed to study the hydrostatic equilibrium of a distorted self-gravitating mass can be divided into two major groups (Blinnikov 1975): (i) Analytic or semia- lytic methods using a small parameter connected with the distortion of the polytrope. (ii) More or less accurate numerical methods. Lyapunov and later Carleman (see Jardetzky 1958, p. 13) have demonstrated that a sphere is a unique solution to the problem of hydrostatic equilibrium for a ?uid mass at rest in tridimensional space. The problem complicates enormously if the sphere is rotating rigidly or di?erentially in space round an axis, and/or if it is distorted magnetically or tidally. Even for the simplest case of a uniformly rotating ?uid body with constant density not all possible solutions have been found (Zharkov and Trubitsyn 1978, p. 222). The sphere becomes an oblate ?gure, and we have no a priori knowledge of its strati?cation, boundary shape, planes of symmetry, transfer of angular momentum in di?erentially rotating bodies, etc. Provides the complete academic treatment on the application of polytropes. This book is primarily intended for students and scientists working in Astrophysics and related fields. It provides an overview of past and present research results and is useful for those wanting to apply polytropes. Shipping may be from multiple locations in the US or from the UK, depending on stock availability. Codice articolo 9781402023507
Quantità: 1 disponibili
Da: AHA-BUCH GmbH, Einbeck, Germania
Buch. Condizione: Neu. Neuware - While it seems possible to present a fairly complete uni ed theory of undistorted polytropes, as attempted in the previous chapter, the theory of distorted polytropes is much more extended and - phisticated, so that I present merely a brief overview of the theories that seem to me most interesting and important. Basically, the methods proposed to study the hydrostatic equilibrium of a distorted self-gravitating mass can be divided into two major groups (Blinnikov 1975): (i) Analytic or semia- lytic methods using a small parameter connected with the distortion of the polytrope. (ii) More or less accurate numerical methods. Lyapunov and later Carleman (see Jardetzky 1958, p. 13) have demonstrated that a sphere is a unique solution to the problem of hydrostatic equilibrium for a uid mass at rest in tridimensional space. The problem complicates enormously if the sphere is rotating rigidly or di erentially in space round an axis, and/or if it is distorted magnetically or tidally. Even for the simplest case of a uniformly rotating uid body with constant density not all possible solutions have been found (Zharkov and Trubitsyn 1978, p. 222). The sphere becomes an oblate gure, and we have no a priori knowledge of its strati cation, boundary shape, planes of symmetry, transfer of angular momentum in di erentially rotating bodies, etc. Codice articolo 9781402023507
Quantità: 2 disponibili
Da: AussieBookSeller, Truganina, VIC, Australia
Hardcover. Condizione: new. Hardcover. While it seems possible to present a fairly complete uni?ed theory of undistorted polytropes, as attempted in the previous chapter, the theory of distorted polytropes is much more extended and - phisticated, so that I present merely a brief overview of the theories that seem to me most interesting and important. Basically, the methods proposed to study the hydrostatic equilibrium of a distorted self-gravitating mass can be divided into two major groups (Blinnikov 1975): (i) Analytic or semia- lytic methods using a small parameter connected with the distortion of the polytrope. (ii) More or less accurate numerical methods. Lyapunov and later Carleman (see Jardetzky 1958, p. 13) have demonstrated that a sphere is a unique solution to the problem of hydrostatic equilibrium for a ?uid mass at rest in tridimensional space. The problem complicates enormously if the sphere is rotating rigidly or di?erentially in space round an axis, and/or if it is distorted magnetically or tidally. Even for the simplest case of a uniformly rotating ?uid body with constant density not all possible solutions have been found (Zharkov and Trubitsyn 1978, p. 222). The sphere becomes an oblate ?gure, and we have no a priori knowledge of its strati?cation, boundary shape, planes of symmetry, transfer of angular momentum in di?erentially rotating bodies, etc. Provides the complete academic treatment on the application of polytropes. This book is primarily intended for students and scientists working in Astrophysics and related fields. It provides an overview of past and present research results and is useful for those wanting to apply polytropes. Shipping may be from our Sydney, NSW warehouse or from our UK or US warehouse, depending on stock availability. Codice articolo 9781402023507
Quantità: 1 disponibili