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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.
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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.
Produktdetails
- Produktdetails
- Verlag: Oxford University Press
- Seitenzahl: 512
- Erscheinungstermin: 2. Februar 2022
- Englisch
- Abmessung: 250mm x 197mm x 31mm
- Gewicht: 1247g
- ISBN-13: 9780192895646
- ISBN-10: 0192895648
- Artikelnr.: 62536166
- Herstellerkennzeichnung
- Libri GmbH
- Europaallee 1
- 36244 Bad Hersfeld
- gpsr@libri.de
- Verlag: Oxford University Press
- Seitenzahl: 512
- Erscheinungstermin: 2. Februar 2022
- Englisch
- Abmessung: 250mm x 197mm x 31mm
- Gewicht: 1247g
- ISBN-13: 9780192895646
- ISBN-10: 0192895648
- Artikelnr.: 62536166
- Herstellerkennzeichnung
- Libri GmbH
- Europaallee 1
- 36244 Bad Hersfeld
- gpsr@libri.de
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.
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
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
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