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Special relativity is the basis of many fields in modern physics: particle physics, quantum field theory, high-energy astrophysics, etc. This theory is presented here by adopting a four-dimensional point of view from the start. An outstanding feature of the book is that it doesn’t restrict itself to inertial frames but considers accelerated and rotating observers. It is thus possible to treat physical effects such as the Thomas precession or the Sagnac effect in a simple yet precise manner. In the final chapters, more advanced topics like tensorial fields in spacetime, exterior calculus and relativistic hydrodynamics are addressed. In the last, brief chapter the author gives a preview of gravity and shows where it becomes incompatible with Minkowsky spacetime. Well illustrated and enriched by many historical notes, this book also presents many applications of special relativity, ranging from particle physics (accelerators, particle collisions, quark-gluon plasma) to astrophysics (relativistic jets, active galactic nuclei), and including practical applications (Sagnac gyrometers, synchrotron radiation, GPS). In addition, the book provides some mathematical developments, such as the detailed analysis of the Lorentz group and its Lie algebra. The book is suitable for students in the third year of a physics degree or on a masters course, as well as researchers and any reader interested in relativity. Thanks to the geometric approach adopted, this book should also be beneficial for the study of general relativity. “A modern presentation of special relativity must put forward its essential structures, before illustrating them using concrete applications to specific dynamical problems. Such is the challenge (so successfully met!) of the beautiful book by Éric Gourgoulhon.” (excerpt from the Foreword by Thibault Damour).
Special relativity (Physics) --- Engineering & Applied Sciences --- Applied Physics --- Ether drift --- Mass energy relations --- Relativity theory, Special --- Restricted theory of relativity --- Special theory of relativity --- Physics. --- Applied mathematics. --- Engineering mathematics. --- Gravitation. --- Fluids. --- Astrophysics. --- Particle acceleration. --- Theoretical, Mathematical and Computational Physics. --- Astrophysics and Astroparticles. --- Particle Acceleration and Detection, Beam Physics. --- Classical and Quantum Gravitation, Relativity Theory. --- Fluid- and Aerodynamics. --- Applications of Mathematics. --- Relativity (Physics) --- Mathematics. --- Math --- Science --- Particles (Nuclear physics) --- Acceleration (Mechanics) --- Nuclear physics --- Acceleration --- Mathematical physics. --- Engineering --- Engineering analysis --- Mathematical analysis --- Hydraulics --- Mechanics --- Physics --- Hydrostatics --- Permeability --- Field theory (Physics) --- Matter --- Antigravity --- Centrifugal force --- Astronomical physics --- Astronomy --- Cosmic physics --- Physical mathematics --- Mathematics --- Properties
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This graduate-level, course-based text is devoted to the 3+1 formalism of general relativity, which also constitutes the theoretical foundations of numerical relativity. The book starts by establishing the mathematical background (differential geometry, hypersurfaces embedded in space-time, foliation of space-time by a family of space-like hypersurfaces), and then turns to the 3+1 decomposition of the Einstein equations, giving rise to the Cauchy problem with constraints, which constitutes the core of 3+1 formalism. The ADM Hamiltonian formulation of general relativity is also introduced at this stage. Finally, the decomposition of the matter and electromagnetic field equations is presented, focusing on the astrophysically relevant cases of a perfect fluid and a perfect conductor (ideal magnetohydrodynamics). The second part of the book introduces more advanced topics: the conformal transformation of the 3-metric on each hypersurface and the corresponding rewriting of the 3+1 Einstein equations, the Isenberg-Wilson-Mathews approximation to general relativity, global quantities associated with asymptotic flatness (ADM mass, linear and angular momentum) and with symmetries (Komar mass and angular momentum). In the last part, the initial data problem is studied, the choice of spacetime coordinates within the 3+1 framework is discussed and various schemes for the time integration of the 3+1 Einstein equations are reviewed. The prerequisites are those of a basic general relativity course with calculations and derivations presented in detail, making this text complete and self-contained. Numerical techniques are not covered in this book.
General relativity (Physics) --- Physics --- Physical Sciences & Mathematics --- Atomic Physics --- Physics - General --- Physics. --- Mathematics. --- Natural philosophy --- Philosophy, Natural --- Relativistic theory of gravitation --- Relativity theory, General --- Computer mathematics. --- Gravitation. --- Astronomy. --- Astrophysics. --- Cosmology. --- Numerical and Computational Physics. --- Classical and Quantum Gravitation, Relativity Theory. --- Astronomy, Astrophysics and Cosmology. --- Computational Mathematics and Numerical Analysis. --- Physical sciences --- Dynamics --- Gravitation --- Relativity (Physics) --- Computer science --- Numerical and Computational Physics, Simulation. --- Computer mathematics --- Discrete mathematics --- Electronic data processing --- Mathematics --- Astronomical physics --- Astronomy --- Cosmic physics --- Field theory (Physics) --- Matter --- Antigravity --- Centrifugal force --- Properties
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La théorie quantique des champs, la physique des particules, l'astrophysique des hautes énergies, etc. sont autant de domaines de la physique moderne qui s'appuient sur la relativité restreinte. Celle-ci est ici présentée en adoptant directement un point de vue quadridimensionnel, c'est-à-dire en passant par l'espace-temps de Minkowski.Ce livre scientifique a ceci de particulier qu'il ne se limite pas aux référentiels inertiels et considère des observateurs accélérés ou en rotation. Cela permet de discuter simplement et de manière rigoureuse d'effets physiques tels que la précession de Thomas ou l'effet Sagnac. Les derniers chapitres abordent des aspects plus avancés : champs tensoriels, calcul extérieur, hydrodynamique relativiste et traitement de la gravitation.Illustré et agrémenté de nombreuses notes historiques, cet ouvrage fait une part belle aux applications, de la physique des particules (accélérateurs, collisions de particules, plasma quark-gluon) à l'astrophysique (jets relativistes, noyaux actifs de galaxie), en passant par les applications pratiques (gyromètres à effet Sagnac, rayonnement synchrotron, GPS). Le livre contient également des développements mathématiques tels que l'analyse détaillée du groupe de Lorentz et de son algèbre de Lie. Ce livre scientifique s'adresse aux étudiants en dernière année de licence de physique (L3) ou en master (M1 et M2), ainsi qu'aux chercheurs et à toute personne intéressée par la relativité. Sa lecture facilitera également l'apprentissage de la relativité générale, en raison de l'approche géométrique adoptée.
Relativity (Physics) --- Astrophysics. --- Astronomical physics --- Astronomy --- Cosmic physics --- Physics --- Gravitation --- Nonrelativistic quantum mechanics --- Space and time --- Special relativity (Physics) --- General relativity (Physics) --- Relativité restreinte (physique) --- Astrophysique. --- Lorentz, Géométrie de. --- Relativité restreinte (physique) --- Lorentz, Géométrie de.
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This graduate-level, course-based text is devoted to the 3+1 formalism of general relativity, which also constitutes the theoretical foundations of numerical relativity. The book starts by establishing the mathematical background (differential geometry, hypersurfaces embedded in space-time, foliation of space-time by a family of space-like hypersurfaces), and then turns to the 3+1 decomposition of the Einstein equations, giving rise to the Cauchy problem with constraints, which constitutes the core of 3+1 formalism. The ADM Hamiltonian formulation of general relativity is also introduced at this stage. Finally, the decomposition of the matter and electromagnetic field equations is presented, focusing on the astrophysically relevant cases of a perfect fluid and a perfect conductor (ideal magnetohydrodynamics). The second part of the book introduces more advanced topics: the conformal transformation of the 3-metric on each hypersurface and the corresponding rewriting of the 3+1 Einstein equations, the Isenberg-Wilson-Mathews approximation to general relativity, global quantities associated with asymptotic flatness (ADM mass, linear and angular momentum) and with symmetries (Komar mass and angular momentum). In the last part, the initial data problem is studied, the choice of spacetime coordinates within the 3+1 framework is discussed and various schemes for the time integration of the 3+1 Einstein equations are reviewed. The prerequisites are those of a basic general relativity course with calculations and derivations presented in detail, making this text complete and self-contained. Numerical techniques are not covered in this book.
Space research --- Cosmology --- Astrophysics --- Mathematical physics --- Theory of relativity. Unified field theory --- Geophysics --- Computer science --- Computer. Automation --- zwaartekracht --- astrofysica --- theoretische fysica --- informatica --- wiskunde --- relativiteitstheorie --- ruimte (astronomie) --- geofysica --- kosmologie
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Special relativity is the basis of many fields in modern physics: particle physics, quantum field theory, high-energy astrophysics, etc. This theory is presented here by adopting a four-dimensional point of view from the start. An outstanding feature of the book is that it doesn’t restrict itself to inertial frames but considers accelerated and rotating observers. It is thus possible to treat physical effects such as the Thomas precession or the Sagnac effect in a simple yet precise manner. In the final chapters, more advanced topics like tensorial fields in spacetime, exterior calculus and relativistic hydrodynamics are addressed. In the last, brief chapter the author gives a preview of gravity and shows where it becomes incompatible with Minkowsky spacetime. Well illustrated and enriched by many historical notes, this book also presents many applications of special relativity, ranging from particle physics (accelerators, particle collisions, quark-gluon plasma) to astrophysics (relativistic jets, active galactic nuclei), and including practical applications (Sagnac gyrometers, synchrotron radiation, GPS). In addition, the book provides some mathematical developments, such as the detailed analysis of the Lorentz group and its Lie algebra. The book is suitable for students in the third year of a physics degree or on a masters course, as well as researchers and any reader interested in relativity. Thanks to the geometric approach adopted, this book should also be beneficial for the study of general relativity. “A modern presentation of special relativity must put forward its essential structures, before illustrating them using concrete applications to specific dynamical problems. Such is the challenge (so successfully met!) of the beautiful book by Éric Gourgoulhon.” (excerpt from the Foreword by Thibault Damour).
Mathematics --- Astrophysics --- Mathematical physics --- Theory of relativity. Unified field theory --- Fluid mechanics --- Experimental nuclear and elementary particle physics --- Physics --- Geophysics --- vloeistofstroming --- zwaartekracht --- astrofysica --- aerodynamica --- deeltjesfysica --- toegepaste wiskunde --- theoretische fysica --- kernenergie --- wiskunde --- fysica --- relativiteitstheorie
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This graduate-level, course-based text is devoted to the 3+1 formalism of general relativity, which also constitutes the theoretical foundations of numerical relativity. The book starts by establishing the mathematical background (differential geometry, hypersurfaces embedded in space-time, foliation of space-time by a family of space-like hypersurfaces), and then turns to the 3+1 decomposition of the Einstein equations, giving rise to the Cauchy problem with constraints, which constitutes the core of 3+1 formalism. The ADM Hamiltonian formulation of general relativity is also introduced at this stage. Finally, the decomposition of the matter and electromagnetic field equations is presented, focusing on the astrophysically relevant cases of a perfect fluid and a perfect conductor (ideal magnetohydrodynamics). The second part of the book introduces more advanced topics: the conformal transformation of the 3-metric on each hypersurface and the corresponding rewriting of the 3+1 Einstein equations, the Isenberg-Wilson-Mathews approximation to general relativity, global quantities associated with asymptotic flatness (ADM mass, linear and angular momentum) and with symmetries (Komar mass and angular momentum). In the last part, the initial data problem is studied, the choice of spacetime coordinates within the 3+1 framework is discussed and various schemes for the time integration of the 3+1 Einstein equations are reviewed. The prerequisites are those of a basic general relativity course with calculations and derivations presented in detail, making this text complete and self-contained. Numerical techniques are not covered in this book.
Space research --- Cosmology --- Astrophysics --- Mathematical physics --- Theory of relativity. Unified field theory --- Geophysics --- Computer science --- Computer. Automation --- zwaartekracht --- astrofysica --- theoretische fysica --- informatica --- wiskunde --- relativiteitstheorie --- ruimte (astronomie) --- geofysica --- kosmologie
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