Abstract:We study the effect of constant shifts on the zeros of rational harmomic functions f (z) = r(z) − z. In particular, we characterize how shifting through the caustics of f changes the number of zeros and their respective orientations. This also yields insight into the nature of the singular zeros of f . Our results have applications in gravitational lensing theory, where certain such functions f represent gravitational point-mass lenses, and a constant shift can be interpreted as the position of the light sourc… Show more
“…Let f be the Rhie function from [11] (see also [12,13]), which has a rational function r of the type (n − 1, n), and which has 5n − 5 zeros. The results in [8] imply that for sufficiently small |c| > 0 the function f c has the same number of zeros as f . The corresponding rational function r c then is of the type (n, n), so the bound N (f ) ≤ 5n − 5 is sharp also in the case (n, n).…”
Section: Resultsmentioning
confidence: 88%
“…A second reason why we have formulated the result for the function f c (rather than just f ) is the application of rational harmonic functions in the context of gravitational lensing; see [5] for a survey. In that application a constant shift represents the position of the light source of the lens, and the change of the number of zeros under movements of the light source is of great interest; see, e.g., [8] for more details. Our note is organized as follows.…”
Generalizing several previous results in the literature on rational harmonic functions, we derive bounds on the maximum number of zeros of functions f (z) = p(z) q(z) − z, which depend on both deg(p) and deg(q). Furthermore, we prove that any function that attains one of these upper bounds is regular.
“…Let f be the Rhie function from [11] (see also [12,13]), which has a rational function r of the type (n − 1, n), and which has 5n − 5 zeros. The results in [8] imply that for sufficiently small |c| > 0 the function f c has the same number of zeros as f . The corresponding rational function r c then is of the type (n, n), so the bound N (f ) ≤ 5n − 5 is sharp also in the case (n, n).…”
Section: Resultsmentioning
confidence: 88%
“…A second reason why we have formulated the result for the function f c (rather than just f ) is the application of rational harmonic functions in the context of gravitational lensing; see [5] for a survey. In that application a constant shift represents the position of the light source of the lens, and the change of the number of zeros under movements of the light source is of great interest; see, e.g., [8] for more details. Our note is organized as follows.…”
Generalizing several previous results in the literature on rational harmonic functions, we derive bounds on the maximum number of zeros of functions f (z) = p(z) q(z) − z, which depend on both deg(p) and deg(q). Furthermore, we prove that any function that attains one of these upper bounds is regular.
“…For these functions, the number of zeros or pre-images is intensively studied; see e.g. [38,19,17,13,7,25,26,32,20,21,22,5,16].…”
Section: The Number Of Pre-imagesmentioning
confidence: 99%
“…Here we focus on solutions of f (z) = η for given (but arbitrary) η ∈ C. As shown in [21] for rational harmonic mappings of the form f (z) = r(z) − z, the number of solutions can vary significantly under changes of η. Moreover, changes only occur when η is "moved" through the caustics of f ; see Figure 1.…”
We derive a formula for the number of pre-images under a non-degenerate harmonic mapping f , using the argument principle. This formula reveals a connection between the pre-images and the caustics. Our results allow to deduce the number of pre-images under f geometrically for every non-caustic point. We approximately locate the pre-images of points near the caustics. Moreover, we apply our results to prove that for every k = n, n + 1, . . . , n 2 there exists a harmonic polynomial of degree n with k zeros.
“…We refer to the expository articles [22,34], and the survey [3]. More recent articles on harmonic mappings with applications to gravitational lensing are [4,20,29,37,38,27,25].…”
We present an iterative root finding method for harmonic mappings in the complex plane, which is a generalization of Newton's method for analytic functions. The complex formulation of the method allows an analysis in a complex variables spirit. For zeros close to poles of f = h + g we construct initial points for which the harmonic Newton iteration is guaranteed to converge. Moreover, we study the number of solutions of f (z) = η close to the critical set of f for certain η ∈ C. We provide a Matlab implementation of the method, and illustrate our results with several examples and numerical experiments, including phase plots and plots of the basins of attraction.
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