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The book aims to expound the general theory of relativity with a mathematical point of view. Catering to the needs of postgraduate students and researchers in the field of astrophysics and mathematical physics, it offers the readers a comprehensive understanding of the advanced topics of the subject matter. It specifically discusses the mathematical foundation of tensor calculus, gives a background of geodesics, Einstein's field equations, linearised gravity, spacetime of spherically symmetric distribution of matter and black holes, and particle and photon orbits in spacetime. Apart from the formulation of general relativity, Lie derivatives and its applications, and causality of spacetime are also discussed in detail. Certain preliminary concepts of extrinsic curvature, Lagrangian formalism of general theory of relativity and 3 + 1 decomposition of space-time are covered and are provided in the book as appendices.
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"This textbook is suitable for a one-semester introduction to General Relativity for advanced undergraduates in physics and engineering. The book is concise so that the entire material can be covered in the one-semester time frame. Many of the calculations are done in detail, without difficult mathematics, to help the students. Though concise, the theory development is lucid and the readers are exposed to possible analytic calculations. In the second edition, the famous twin paradox with acceleration is solved in full from the accelerated observer's frame. The findings of the Event Horizon Telescope (EHT) collaboration, who captured the first ever image of a black hole, are discussed in detail. The geodetic and frame drag precessions of gyroscopes in orbit about a rotating Earth are worked out and the Gravity Probe B (GPB) experiment is discussed. Also in the second edition are some new exercise problems. Resources are provided to instructors who adopt this textbook for their courses. Adopting instructors can print and copy portions of these resources solely for their teaching needs. All instructional resources are furnished for informational use only, and are subject to change without notice"--
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"Spacetime and Geometry is an introductory textbook on general relativity, specifically aimed at students. Using a lucid style, Carroll first covers the foundations of the theory and mathematical formalism, providing an approachable introduction to what can often be an intimidating subject. Three major applications of general relativity are then discussed: black holes, perturbation theory and gravitational waves, and cosmology. Students will learn the origin of how spacetime curves (the Einstein equation) and how matter moves through it (the geodesic equation). They will learn what black holes really are, how gravitational waves are generated and detected, and the modern view of the expansion of the universe. A brief introduction to quantum field theory in curved spacetime is also included. A student familiar with this book will be ready to tackle research-level problems in gravitational physics"--
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This book, dedicated to Roger Penrose, is a second, mathematically oriented course in general relativity. It contains extensive references and occasional excursions in the history and philosophy of gravity, including a relatively lengthy historical introduction. The book is intended for all students of general relativity of any age and orientation who have a background including at least first courses in special and general relativity, differential geometry, and topology. The material is developed in such a way that through the last two chapters the reader may acquire a taste of the modern mathematical study of black holes initiated by Penrose, Hawking, and others, as further influenced by the initial-value or PDE approach to general relativity. Successful readers might be able to begin reading research papers on black holes, especially in mathematical physics and in the philosophy of physics. The chapters are: Historical introduction, General differential geometry, Metric differential geometry, Curvature, Geodesics and causal structure, The singularity theorems of Hawking and Penrose, The Einstein equations, The 3+1 split of space-time, Black holes I: Exact solutions, and Black holes II: General theory. These are followed by two appendices containing background on Lie groups, Lie algebras, & constant curvature, and on Formal PDE theory.
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Questo libro è stato ideato per un corso che spieghi, nella maniera più semplice possibile, le Teorie della Relatività Ristretta e Generale a studenti che si accostano ad esse per la prima volta. I contenuti di queste due teorie fanno ormai parte del bagaglio culturale necessario ad ogni fisico e ad ogni matematico e, in particolare, esse costituiscono un insieme di conoscenze indispensabili per chiunque si occupi di fisica, astrofisica e cosmologia. This book is designed to explain, in the simplest way possible, the Theories of Special and General Relativity to students who are approaching them for the first time. The contents of these two theories are now part of the cultural background needed by every physicist and mathematician, and, in particular, they constitute an indispensable body of knowledge for anyone involved in physics, astrophysics and cosmology.
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Questo libro è stato ideato per un corso che spieghi, nella maniera più semplice possibile, le Teorie della Relatività Ristretta e Generale a studenti che si accostano ad esse per la prima volta. I contenuti di queste due teorie fanno ormai parte del bagaglio culturale necessario ad ogni fisico e ad ogni matematico e, in particolare, esse costituiscono un insieme di conoscenze indispensabili per chiunque si occupi di fisica, astrofisica e cosmologia. This book is designed to explain, in the simplest way possible, the Theories of Special and General Relativity to students who are approaching them for the first time. The contents of these two theories are now part of the cultural background needed by every physicist and mathematician, and, in particular, they constitute an indispensable body of knowledge for anyone involved in physics, astrophysics and cosmology.
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This book, dedicated to Roger Penrose, is a second, mathematically oriented course in general relativity. It contains extensive references and occasional excursions in the history and philosophy of gravity, including a relatively lengthy historical introduction. The book is intended for all students of general relativity of any age and orientation who have a background including at least first courses in special and general relativity, differential geometry, and topology. The material is developed in such a way that through the last two chapters the reader may acquire a taste of the modern mathematical study of black holes initiated by Penrose, Hawking, and others, as further influenced by the initial-value or PDE approach to general relativity. Successful readers might be able to begin reading research papers on black holes, especially in mathematical physics and in the philosophy of physics. The chapters are: Historical introduction, General differential geometry, Metric differential geometry, Curvature, Geodesics and causal structure, The singularity theorems of Hawking and Penrose, The Einstein equations, The 3+1 split of space-time, Black holes I: Exact solutions, and Black holes II: General theory. These are followed by two appendices containing background on Lie groups, Lie algebras, & constant curvature, and on Formal PDE theory.
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Questo libro è stato ideato per un corso che spieghi, nella maniera più semplice possibile, le Teorie della Relatività Ristretta e Generale a studenti che si accostano ad esse per la prima volta. I contenuti di queste due teorie fanno ormai parte del bagaglio culturale necessario ad ogni fisico e ad ogni matematico e, in particolare, esse costituiscono un insieme di conoscenze indispensabili per chiunque si occupi di fisica, astrofisica e cosmologia. This book is designed to explain, in the simplest way possible, the Theories of Special and General Relativity to students who are approaching them for the first time. The contents of these two theories are now part of the cultural background needed by every physicist and mathematician, and, in particular, they constitute an indispensable body of knowledge for anyone involved in physics, astrophysics and cosmology.
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The general theory of relativity, Einstein's theory of gravitation, has been included as a compulsory subject in undergraduate and graduate courses in Physics and Applied Mathematics all over the world. However, the physics-first approach that is taken by many textbooks is not universally used, as the approach often depends on the instructors' or students' background. Conceived from the lecture notes made by the author over a teaching career spanning 18 years, this book introduces the general theory of relativity for advanced students with a strong mathematical background. The proposed book takes a 'math-first approach' for which the mathematical formalism comes first and is then applied to physics. It presents a concise yet comprehensive and structured understanding of general theory of relativity. The book discusses the mathematical foundation of general theory of relativity and focuses heavily on topics such as tensor calculus, geodesics, Einstein field equations, linearized gravity, Lie derivatives and their applications, causal structure of space-time, rotating black holes and a basic knowledge of cosmology and astrophysics. All of this is explained through a large number of worked examples and exercises. The book aims to expound the general theory of relativity with a mathematical point of view. Catering to the needs of postgraduate students and researchers in the field of astrophysics and mathematical physics, it offers the readers a comprehensive understanding of the advanced topics of the subject matter. It specifically discusses the mathematical foundation of tensor calculus, gives a background of geodesics, Einstein's field equations, linearised gravity, spacetime of spherically symmetric distribution of matter and black holes, and particle and photon orbits in spacetime. Apart from the formulation of general relativity, Lie derivatives and its applications, and causality of spacetime are also discussed in detail. Certain preliminary concepts of extrinsic curvature, Lagrangian formalism of general theory of relativity and 3 + 1 decomposition of space-time are covered and are provided in the book as appendices.
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A textbook for 2nd and 3rd year undergraduate students using the fundamental principle of covariance as a basis for studying classical mechanics, electrodynamics, the special theory of relativity, and the general theory of relativity, before moving on to more advanced topics of field theory, differential forms, and modified theories of gravity.
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