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Gravitational Lensing: Strong, Weak and Micro: Saas-Fee Advanced Course 33, by Peter Schneider, Christopher Kochanek, Joachim Wambsganss
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The observation, in 1919 by A.S. Eddington and collaborators, of the gra- tational de?ection of light by the Sun proved one of the many predictions of Einstein’s Theory of General Relativity: The Sun was the ?rst example of a gravitational lens. In 1936, Albert Einstein published an article in which he suggested - ing stars as gravitational lenses. A year later, Fritz Zwicky pointed out that galaxies would act as lenses much more likely than stars, and also gave a list of possible applications, as a means to determine the dark matter content of galaxies and clusters of galaxies. It was only in 1979 that the ?rst example of an extragalactic gravitational lens was provided by the observation of the distant quasar QSO 0957+0561, by D. Walsh, R.F. Carswell, and R.J. Weymann. A few years later, the ?rst lens showing images in the form of arcs was detected. The theory, observations, and applications of gravitational lensing cons- tute one of the most rapidly growing branches of astrophysics. The gravi- tional de?ection of light generated by mass concentrations along a light path producesmagni?cation,multiplicity,anddistortionofimages,anddelaysp- ton propagation from one line of sight relative to another. The huge amount of scienti?c work produced over the last decade on gravitational lensing has clearly revealed its already substantial and wide impact, and its potential for future astrophysical applications.
- Sales Rank: #3487194 in Books
- Color: Hardcover,
- Brand: Brand: Springer
- Published on: 2006-06-21
- Original language: English
- Number of items: 1
- Dimensions: 9.25" h x 6.25" w x .75" l, 2.00 pounds
- Binding: Hardcover
- 552 pages
- Used Book in Good Condition
From the Back Cover
The theory, observations, and applications of gravitational lensing constitute one of the most rapidly growing branches of astrophysics. The gravitational deflection of light generated by mass concentrations along a light path produces magnification, multiplicity, and distortion of images and delays photon propagation from one line of sight relative to another. The huge amount of scientific work on gravitational lensing produced over the last decade has clearly revealed its already substantial and wide impact and its potential for future astrophysical applications.
The up-to-date contributions in this book are based on the lecture notes of the 33rd Saas–Fee Advanced Course of the Swiss Society of Astronomy and Astrophysics, entitled Gravitational Lensing: Strong, Weak, and Micro. The book comprises four complementary parts, written by leading experts in the field, constituting a genuine textbook about gravitational lensing:
• Peter Schneider – Part 1: Introduction to Gravitational Lensing and Cosmology
• Christopher Kochanek – Part 2: Strong Gravitational Lensing
• Peter Schneider – Part 3: Weak Gravitational Lensing
• Joachim Wambsganss – Part 4: Gravitational Microlensing
Students and researchers alike will benefit from this comprehensive presentation of the astrophysical and astronomical aspects of gravitational lensing.
Most helpful customer reviews
0 of 0 people found the following review helpful.
A classic
By Alan K. Lefor
This is a classic text in the field and would absolutely be considered "required reading" for anyone with a serious interest in Gravitational Lensing. These lectures are thorough, and provide an excellent starting point for people entering the field.
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