Imaging the 3-d cosmological mass distribution with weak gravitational lensing

Nov, 2001
4 pages
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Citations per year

2002200620102014201702468
Abstract: (arXiv)
I show how weak gravitational lensing can be used to image the 3-D mass distribution in the Universe. An inverse relation to the lensing equation, relating the lensing potential evaluated at each source to the full 3-D Newtonian potential, is derived. I consider the normal modes of the lensing problem and clarify the equations using a small-angle approximation. Finally I consider the prospects of using this method to estimate the 3-D matter distribution from a realistic galaxy lensing survey.