Astrophysical Applications of Gravitational Lensing

doi:10.1017/CBO9781139940306

Gravitational lenses offer the best, and sometimes the only, means of tackling key problems in many fields of astrophysics and cosmology. According to Einstein's theory, the curvature of light-rays increases with mass; gravitational lenses can be used to map the distribution of mass in a Universe in which virtually all matter is dark matter of an unknown nature. Gravitational lensing has significantly improved our knowledge of many astrophysical phenomena, such as exoplanets, galaxies, active galactic nuclei, quasars, clusters, large-scale structure and the Universe itself. All these topics are covered fully in this book, together with two tutorials on lens and microlensing modelling. The future of lensing in relation to large surveys and the anticipated discoveries of thousands more gravitational lenses is also discussed, making this volume an ideal guide for postgraduate students and practising researchers in the use of gravitational lenses as a tool in their investigations.

'Each article is self-contained and as a whole it presents an overview of the field of strong lensing … For the reader who is entering the filed this is a useful collection that summarizes it well.'

Alan Heavens Source: The Observatory

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Astrophysical Applications of Gravitational Lensing

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Contents

Frontmatter
pp i-vi

Contents
pp vii-vii

List of contributors
pp viii-viii

List of participants
pp ix-x

Preface
pp xi-xii

Acknowledgements
pp xiii-xiv

1 - Lensing basics
pp 1-30

2 - Exoplanet microlensing
pp 31-50

3 - Four case studies of microlensing
pp 51-120

4 - Gravitational (micro)lensing of quasars and AGN
pp 121-140

5 - Dark matter in clusters and large-scale structure
pp 141-182

6 - The future of strong lensing
pp 183-212

7 - Methods for strong lens modelling
pp 213-250

8 - Tutorial on inverse ray shooting
pp 251-290

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