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Introduction to Black Hole Physics.

What is a black hole? How many of them are in our Universe? Can black holes be created in a laboratory or in particle colliders? Can objects similar to black holes be used for space and time travel? This text discusses these and many other questions providing the reader with the tools required to ex...

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Detalles Bibliográficos
Clasificación:Libro Electrónico
Autor principal: Frolov, Valeri P.
Otros Autores: Zelnikov, Andrei
Formato: Electrónico eBook
Idioma:Inglés
Publicado: Oxford : OUP Oxford, 2011.
Temas:
Acceso en línea:Texto completo

MARC

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020 |a 9780191003226 
020 |a 0191003220 
020 |z 0199692297  |q (hardback) 
020 |z 9780199692293  |q (hardback) 
029 1 |a DEBSZ  |b 456610197 
035 |a (OCoLC)922971950 
050 4 |a QB843.B55.F7623 2011eb 
082 0 4 |a 523.8875 
049 |a UAMI 
100 1 |a Frolov, Valeri P. 
245 1 0 |a Introduction to Black Hole Physics. 
260 |a Oxford :  |b OUP Oxford,  |c 2011. 
300 |a 1 online resource (505 pages) 
336 |a text  |b txt  |2 rdacontent 
337 |a computer  |b c  |2 rdamedia 
338 |a online resource  |b cr  |2 rdacarrier 
588 0 |a Print version record. 
505 0 |a ""Cover""; ""Contents""; ""1 Black Holes: Big Picture""; ""1.1 Gravity and Black Holes""; ""1.2 Brief History of Black Holes""; ""1.3 â€?Dark Starsâ€? vs. Black Holes""; ""1.4 Final State of Stellar Evolution""; ""1.5 Equilibrium of Gravitating Systems""; ""1.6 Important Notions of Astrophysics""; ""1.7 Black Holes in Astrophysics and Cosmology""; ""1.8 Stellar-Mass Black Holes""; ""1.9 Supermassive Black Holes""; ""1.10 Primordial Black Holes""; ""1.11 Black Holes in Theoretical Physics""; ""1.12 Black Holes and Extra Dimensions""; ""2 Physics in a Uniformly Accelerated Frame"" 
505 8 |a ""2.1 Minkowski Spacetime and Its Symmetries""""2.2 Minkowski Spacetime in Curved Coordinates""; ""2.3 Uniformly Accelerated Reference Frame""; ""2.4 Homogeneous Gravitational Field""; ""2.5 Causal Structure""; ""2.6 Wickâ€?s Rotation in the Rindler Space""; ""3 Riemannian Geometry""; ""3.1 Differential Manifold. Tensors""; ""3.2 Metric""; ""3.3 Covariant Derivative""; ""3.4 Lie and Fermi Transport""; ""3.5 Curvature Tensor""; ""3.6 Parallel Transport of a Vector""; ""3.7 Spacetime Symmetries""; ""3.8 Submanifold""; ""3.9 Integration""; ""4 Particle Motion in Curved Spacetime"" 
505 8 |a ""4.1 Equations of Motion""""4.2 Phase Space""; ""4.3 Complete Integrability""; ""5 Einstein Equations""; ""5.1 Einsteinâ€?Hilbert Action""; ""5.2 Einstein Equations""; ""5.3 Linearized Gravity""; ""5.4 Gravitational radiation""; ""5.5 Gravity in Higher-Dimensions""; ""6 Spherically Symmetric Black Holes""; ""6.1 Spherically Symmetric Gravitational Field""; ""6.2 Schwarzschildâ€?de Sitter Metric""; ""6.3 Global Structure of the Schwarzschild Spacetime""; ""6.4 Black Hole Interior""; ""6.5 PainlevÃ?â€?Gullstrand Metric""; ""6.6 Eddingtonâ€?Finkelstein Coordinates""; ""6.7 Charged Black Holes"" 
505 8 |a ""6.8 Higher-Dimensional Spherical Black Holes""""7 Particles and Light Motion in Schwarzschild Spacetime""; ""7.1 Equations of Motion""; ""7.2 Particle Trajectories""; ""7.3 Keplerâ€?s Law""; ""7.4 Light Propagation""; ""7.5 Ray-Tracing in Schwarzschild Spacetime""; ""7.6 Black Hole as a Gravitational Lens""; ""7.7 Radiation from an Object Moving Around the Black Hole""; ""7.8 Equations of Motion in â€?Tiltedâ€? Spherical Coordinates""; ""7.9 Magnetized Schwarzschild Black Hole""; ""7.10 Particle and Light Motion Near Higher-Dimensional Black Holes""; ""8 Rotating Black Holes"" 
505 8 |a ""8.1 Kerr Spacetime""""8.2 Ergosphere. Horizon""; ""8.3 Particle and Light Motion in Equatorial Plane""; ""8.4 Spinning up the Black Hole""; ""8.5 Geodesics in Kerr Spacetime: General Case""; ""8.6 Light Propagation""; ""8.7 Hidden Symmetries of Kerr Spacetime""; ""8.8 Energy Extraction from a Rotating Black Hole""; ""8.9 Black Holes in External Magnetic Field""; ""9 Classical and Quantum Fields near Black Holes""; ""9.1 Introduction""; ""9.2 Static Field in the Schwarzschild Spacetime""; ""9.3 Dimensional Reduction""; ""9.4 Quasinormal Modes""; ""9.5 Massless Fields in the Kerr Spacetime"" 
500 |a ""9.6 Black Hole in a Thermal Bath"" 
504 |a Includes bibliographical references and index. 
520 8 |a What is a black hole? How many of them are in our Universe? Can black holes be created in a laboratory or in particle colliders? Can objects similar to black holes be used for space and time travel? This text discusses these and many other questions providing the reader with the tools required to explore the Black Hole Land independently. 
590 |a ProQuest Ebook Central  |b Ebook Central Academic Complete 
650 0 |a Black holes (Astronomy) 
650 0 |a Gravitational collapse. 
650 0 |a Stars  |x Evolution. 
650 6 |a Trous noirs (Astronomie) 
650 6 |a Effondrement gravitationnel. 
650 6 |a Étoiles  |x Évolution. 
650 7 |a Black holes (Astronomy)  |2 fast 
650 7 |a Gravitational collapse  |2 fast 
650 7 |a Stars  |x Evolution  |2 fast 
700 1 |a Zelnikov, Andrei. 
758 |i has work:  |a Introduction to black hole physics (Text)  |1 https://id.oclc.org/worldcat/entity/E39PCGkht9vXcKjkk9gJPcYpj3  |4 https://id.oclc.org/worldcat/ontology/hasWork 
776 0 8 |i Print version:  |a Frolov, Valeri P.  |t Introduction to Black Hole Physics.  |d Oxford : OUP Oxford, ©2011  |z 9780199692293 
856 4 0 |u https://ebookcentral.uam.elogim.com/lib/uam-ebooks/detail.action?docID=3055296  |z Texto completo 
938 |a ProQuest Ebook Central  |b EBLB  |n EBL3055296 
994 |a 92  |b IZTAP