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Inverse backscattering in two dimensions

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Abstract

This article extends the authors' previous results (Commun. Math. Phys.124, 169–215 (1989) to inverse scattering in two space dimensions. The new problem in two dimensions is the behavior of the backscattering amplitude near zero energy. Generically, this has the form

$$a({\xi \mathord{\left/ {\vphantom {\xi {\left| \xi \right|,}}} \right. \kern-\nulldelimiterspace} {\left| \xi \right|,}} - {\xi \mathord{\left/ {\vphantom {\xi {\left| \xi \right|,\left| \xi \right|}}} \right. \kern-\nulldelimiterspace} {\left| \xi \right|,\left| \xi \right|}}) = 2\pi (2\pi \beta + \ln \left| \xi \right|)^{ - 1} + b(\xi ),$$

whereb(0)=0 andb(ζ) is Hölder continuous. In order to work in weighted Hölder spaces as before, the constant β and the functionb(ζ) must now be interpreted as “coordinates” on the space of backscattering data. In this setting the mapping to backscattering data is again a local diffeomorphism at a dense open set in the real-valued potentials.

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Communicated by B. Simon

Partially supported by NSF Grant DMS89-02246

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Eskin, G., Ralston, J. Inverse backscattering in two dimensions. Commun.Math. Phys. 138, 451–486 (1991). https://doi.org/10.1007/BF02102037

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