The Elements of Relativity

Author:   David M. Wittman (Professor, Professor, University of California, Davis)
Publisher:   Oxford University Press
ISBN:  

9780199658640


Pages:   324
Publication Date:   06 June 2018
Format:   Paperback
Availability:   Manufactured on demand   Availability explained
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The Elements of Relativity


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Author:   David M. Wittman (Professor, Professor, University of California, Davis)
Publisher:   Oxford University Press
Imprint:   Oxford University Press
Dimensions:   Width: 18.90cm , Height: 1.60cm , Length: 24.80cm
Weight:   0.708kg
ISBN:  

9780199658640


ISBN 10:   0199658641
Pages:   324
Publication Date:   06 June 2018
Audience:   College/higher education ,  Undergraduate
Format:   Paperback
Publisher's Status:   Active
Availability:   Manufactured on demand   Availability explained
We will order this item for you from a manufactured on demand supplier.

Table of Contents

1: A First Look at Relativity 2: Acceleration and Force 3: Galilean Relativity 4: Reasoning with Frames and Spacetime Diagrams 5: The Speed of Light 6: Time Slow 7: Time Dilation and Length Contraction 8: Special Relativity: Putting it All Together 9: Doppler Effect and Velocity Addition Law 10: The Twin Paradox 11: Spacetime Geometry 12: Energy and Momentum 13: The Equivalence Principle 14: Gravity Reframed 15: Potential 16: Newtonian Gravity 17: Orbits 18: General Relativity and teh Schwarzschild Metric 19: Beyond the Schwarschild Metric 20: Black Holes

Reviews

The Elements of Relativity is unique: Wittman writes for students who lack a detailed physics background but who still wish to learn about the nature of space-time, black holes, and astronomical phenomena like gravitational lensing. The book successfully builds the necessary physics fundamentals at a reasonable pace to allow the reader to tackle the most sophisticated concepts by the end of the book. Highly recommended. * C. Palma, CHOICE *


Author Information

David M. Wittman is a professor at the University of California, Davis. He has discovered millions of galaxies as co-PI of the Deep Lens Survey, which was awarded over 100 nights on 4-m telescopes to study a representative sample of the universe. But discovering millions of galaxies was just the easy part. He analyzed the galaxies' shapes to reveal subtle distortions caused by the gravitational fields of foreground masses, an effect called weak gravitational lensing. He was the first to detect cosmic shear, or weak lensing by the large-scale structure of the universe. He was also the first to detect a cluster of galaxies through its gravitational effects alone, and the first to combine source redshift information with lensing to probe structure in three dimensions (tomography).

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