Compact Objects in Astrophysics

Compact Objects in Astrophysics PDF

Author: Max Camenzind

Publisher: Springer Science & Business Media

Published: 2007-02-24

Total Pages: 691

ISBN-13: 3540499121

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Modern comprehensive introduction and overview of the physics of White Dwarfs, Neutron Stars and Black Holes, including all relevant observations. Contains a basic introduction to General Relativity, including the modern 3+1 split of spacetime and of Einstein’s equations. The split is used for the first time to derive the structure equations for rapidly rotating neutron stars and Black Holes. Detailed discussions and derivations of current theoretical results. In particular also the most recent equations of state for neutron star matter are explained. Topics , such as colour superconductivity are discussed and used for modelling. A book for graduate students and researchers. Contains exercises and some solutions.

Black Holes, White Dwarfs, and Neutron Stars

Black Holes, White Dwarfs, and Neutron Stars PDF

Author: Stuart L. Shapiro

Publisher: John Wiley & Sons

Published: 2008-11-20

Total Pages: 663

ISBN-13: 3527617671

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This self-contained textbook brings together many different branches of physics--e.g. nuclear physics, solid state physics, particle physics, hydrodynamics, relativity--to analyze compact objects. The latest astronomical data is assessed. Over 250 exercises.

MHD Flows in Compact Astrophysical Objects

MHD Flows in Compact Astrophysical Objects PDF

Author: Vasily S. Beskin

Publisher: Springer Science & Business Media

Published: 2009-12-08

Total Pages: 425

ISBN-13: 3642012906

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Accretion flows, winds and jets of compact astrophysical objects and stars are generally described within the framework of hydrodynamical and magnetohydrodynamical (MHD) flows. Analytical analysis of the problem provides profound physical insights, which are essential for interpreting and understanding the results of numerical simulations. Providing such a physical understanding of MHD Flows in Compact Astrophysical Objects is the main goal of this book, which is an updated translation of a successful Russian graduate textbook. The book provides the first detailed introduction into the method of the Grad-Shafranov equation, describing analytically the very broad class of hydrodynamical and MHD flows. It starts with the classical examples of hydrodynamical accretion onto relativistic and nonrelativistic objects. The force-free limit of the Grad-Shafranov equation allows us to analyze in detail the physics of the magnetospheres of radio pulsars and black holes, including the Blandford-Znajek process of energy extraction from a rotating black hole immersed in an external magnetic field. Finally, on the basis of the full MHD version of the Grad-Shafranov equation the author discusses the problems of jet collimation and particle acceleration in Active Galactic Nuclei, radio pulsars, and Young Stellar Objects. The comparison of the analytical results with numerical simulations demonstrates their good agreement. Assuming that the reader is familiar with the basic physical and mathematical concepts of General Relativity, the author uses the 3+1 split approach which allows the formulation of all results in terms of physically clear language of three dimensional vectors. The book contains detailed derivations of equations, numerous exercises, and an extensive bibliography. It therefore serves as both an introductory text for graduate students and a valuable reference work for researchers in the field.

Compact Stars

Compact Stars PDF

Author: Norman K. Glendenning

Publisher: Springer Science & Business Media

Published: 2012-12-06

Total Pages: 402

ISBN-13: 1468404911

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A whole decades research collated, organised and synthesised into one single book! Following a 60-page review of the seminal treatises of Misner, Thorne, Wheeler and Weinberg on general relativity, Glendenning goes on to explore the internal structure of compact stars, white dwarfs, neutron stars, hybrids, strange quark stars, both the counterparts of neutron stars as well as of dwarfs. This is a self-contained treatment and will be of interest to graduate students in physics and astrophysics as well as others entering the field.

Compact Stellar X-ray Sources

Compact Stellar X-ray Sources PDF

Author: Walter Lewin

Publisher: Cambridge University Press

Published: 2006-04-06

Total Pages: 667

ISBN-13: 1139451774

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X-ray astronomy is the prime available window on astrophysical compact objects: black holes, neutron stars and white dwarfs. In this book, prominent experts provide a comprehensive overview of the observations and astrophysics of these objects. This is a valuable reference for graduate students and active researchers.

Black Holes, White Dwarfs and Neutron Stars

Black Holes, White Dwarfs and Neutron Stars PDF

Author: Stuart L. Shapiro

Publisher: Wiley-VCH

Published: 1983

Total Pages: 645

ISBN-13: 9780471873167

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This self-contained textbook brings together many different branches of physics--e.g. nuclear physics, solid state physics, particle physics, hydrodynamics, relativity--to analyze compact objects. The latest astronomical data is assessed. Over 250 exercises.

Compact Star Physics

Compact Star Physics PDF

Author: Jürgen Schaffner-Bielich

Publisher: Cambridge University Press

Published: 2020-08-27

Total Pages: 325

ISBN-13: 1107180899

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This introduction to compact star physics explains key concepts from general relativity, thermodynamics and nuclear physics.

Physics of Relativistic Objects in Compact Binaries: from Birth to Coalescence

Physics of Relativistic Objects in Compact Binaries: from Birth to Coalescence PDF

Author: Monica Colpi

Publisher: Springer Science & Business Media

Published: 2009-03-28

Total Pages: 386

ISBN-13: 1402092644

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A very attractive feature of the theory of general relativity is that it is a perfectexampleofa“falsi?able”theory:notunableparameterispresentinthe theory and therefore even a single experiment incompatible with a prediction of the theory would immediately lead to its inevitable rejection, at least in the physical regime of application of the aforementioned experiment. This fact provides additional scienti?c value to one of the boldest and most fascinating achievements of the human intellect ever, and motivates a wealth of e?orts in designing and implementing tests aimed at the falsi?cation of the theory. The ?rst historical test on the theory has been the de?ection of light gr- ing the solar surface (Eddington 1919): the compatibility of the theory with this ?rst experiment together with its ability to explain the magnitude of the perihelion advance of Mercury contributed strongly to boost acceptance and worldwideknowledge.However,technologicallimitations preventedphysicists from setting up more constraining tests for several decades after the formu- tion of the theory. In fact, a relevant problem with experimental general r- ativity is that the predicted deviations from the Newtonian theory of gravity areverysmallwhentheexperimentsarecarriedoutinterrestriallaboratories.

Accretion Power in Astrophysics

Accretion Power in Astrophysics PDF

Author: Juhan Frank

Publisher: Cambridge University Press

Published: 2002-01-17

Total Pages: 390

ISBN-13: 9780521629577

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Accretion Power in Astrophysics examines accretion as a source of energy in both binary star systems containing compact objects, and in active galactic nuclei. Assuming a basic knowledge of physics, the authors describe the physical processes at work in accretion discs and other accretion flows. The first three chapters explain why accretion is a source of energy, and then present the gas dynamics and plasma concepts necessary for astrophysical applications. The next three chapters then develop accretion in stellar systems, including accretion onto compact objects. Further chapters give extensive treatment of accretion in active galactic nuclei, and describe thick accretion discs. A new chapter discusses recently discovered accretion flow solutions. The third edition is greatly expanded and thoroughly updated. New material includes a detailed treatment of disc instabilities, irradiated discs, disc warping, and general accretion flows. The treatment is suitable for advanced undergraduates, graduate students and researchers.