Several months ago, D. Khavinson and I extended the complex dynamics
approach of Khavinson and G. Swiatek
for finding a bound on the number of distinct zeros of
to the case of
,
where
and
are analytic
polynomials.
J. Rabin pointed out
that our result settles a conjecture of S. H. Rhie concerning the maximum
number of lensed images due to an
-point gravitational lens and that Rhie
has constructed examples that settle our question concerning the sharpness
of the bound. A preprint of this paper that includes applications to
gravitational lensing can be found at
http://arxiv.org/abs/math.CV/0401188.
My research concerns complex-valued harmonic functions.
Let
be a complex-valued harmonic function defined on
an open subset of the complex plane
(or on the entire complex plane).
A main result in my thesis (2003) is that the cluster set
combined with the image of the critical set
partitions the complex plane into regions
where each point has the same number of distinct preimages.
The cluster set consists of those finite values
such that
there exists a sequence
in the domain of
where
approaches the boundary of the domain (or
) and
.
The critical set consists of those points
where the function is not locally
.
Graphs of caustics in
gravitational lensing are similar to graphs of the image of the critical set of
complex-valued harmonic functions.
I want to learn more about gravitational lensing. I am hoping that complex analysis will be useful in other lensing problems and also that mathematical techniques used in gravitational lensing could be applied to questions concerning the behavior of complex-valued harmonic functions.
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main index
for Gravitational Lensing in the Kerr Spacetime Geometry.