Abstract
The impact of gravitational lenses on our knowledge of the Universe is inversely proportional to their scarcity. In the weak-field limit, lensing studies are based on well-established physics and thus offer a direct, simple approach to address many pressing problems of astrophysics and cosmology. Examples of these are the significance of dark matter and the density, age and size of the Universe. I describe examples of these applications. I also present new developments in cosmological applications of gravitational lenses, regarding estimates of the Hubble constant using strong lensing of quasars. I describe our recent measurements of time delays for the images of SDSS J1004+4112, and discuss prospects for the future utilizing synoptic telescopes, planned, under construction, and beginning operations.
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Acknowledgements
I acknowledge support from the Smithsonian Institution and from HST grants in support of CASTLES. I would also like to thank the CASTLES team, Janine Fohlmeister and Joachim Wambsganss for always interesting discussions. I am very grateful to the SOC, as well as Xavier Barcons and Luis Goicoechea for the invitation to present a talk at SEA 2008 in Santander.
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Falco, E.E. (2010). Gravitational Lenses: An Update. In: Diego, J., Goicoechea, L., González-Serrano, J., Gorgas, J. (eds) Highlights of Spanish Astrophysics V. Astrophysics and Space Science Proceedings. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-11250-8_3
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DOI: https://doi.org/10.1007/978-3-642-11250-8_3
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