Aimed at advanced undergraduate or graduate physics students, the book aims to give a working understanding of astronomy and gravitational waves, as well as introducing the reader to the key concepts in cosmology and classical field theory.
Aimed at advanced undergraduate or graduate physics students, the book aims to give a working understanding of astronomy and gravitational waves, as well as introducing the reader to the key concepts in cosmology and classical field theory.Hinweis: Dieser Artikel kann nur an eine deutsche Lieferadresse ausgeliefert werden.
Andrew Steane is a Professor of Physics at the University of Oxford. He has conducted experimental and theoretical research into the foundations of physics and has performed pioneering quantum experiments with ultra-cold atomic clouds, as well as establishing the ion trap quantum computing program at Oxford. Professor Steane discovered quantum error correction and the CSS (Calderbank Shor Steane) codes and he is a recipient of the Maxwell Medal and Prize of the Institute of Physics, and the Trotter Prize of Texas A&M University. He regularly lectures on relativity and other areas of physics and has published two undergraduate physics textbooks and two books on science and religion with Oxford University Press.
Inhaltsangabe
1: Preface 2: Terminology and notation 3: The elements of general relativity 4: An introductory example: the uniform static field 5: Life in a rotating world 6: Linearized general relativity 7: Slow stationary sources 8: Gravitational waves 9: Manifolds 10: Vectors on manifolds 11: The affine connection 12: Further useful ideas 13: Tensors 14: Parallel transport and geodesics 15: Physics in curved spacetime 16: Curvature 17: The Einstein field equation 18: Schwarzschild-Droste solution 19: Further spherically symmetric solutions 20: Rotating bodies; the Kerr metric 21: Black holes 22: Black hole thermodynamics 23: Cosmology 24: Cosmological dynamics 25: The growth of structure 26: Observational cosmology 27: The very early universe 28: First steps in classical field theory 29: Lagrangian mechanics for fields 30: Conclusion Free
1: Preface 2: Terminology and notation 3: The elements of general relativity 4: An introductory example: the uniform static field 5: Life in a rotating world 6: Linearized general relativity 7: Slow stationary sources 8: Gravitational waves 9: Manifolds 10: Vectors on manifolds 11: The affine connection 12: Further useful ideas 13: Tensors 14: Parallel transport and geodesics 15: Physics in curved spacetime 16: Curvature 17: The Einstein field equation 18: Schwarzschild-Droste solution 19: Further spherically symmetric solutions 20: Rotating bodies; the Kerr metric 21: Black holes 22: Black hole thermodynamics 23: Cosmology 24: Cosmological dynamics 25: The growth of structure 26: Observational cosmology 27: The very early universe 28: First steps in classical field theory 29: Lagrangian mechanics for fields 30: Conclusion Free
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