The Sommerfeld problem and inverse problem for the Helmholtz equation

2020

Closed access Metadata (CSL-JSON)
DOI 10.1515/jiip-2020-0033
Data confidence 85 high
How this score is calculated

It is built from checkable properties of the record itself: whether the article has a DOI, how many independent sources confirmed its data, whether the required fields are filled in, and how recent the latest confirmation is. Disagreement between sources and a missing identifier lower it. A value of 80 or above means the record was published without further checking; 60 to 79 means it is published at reduced confidence, with a manual check advisable. A record verified by an editor by hand is never pushed below 90 by a recalculation. This scores our data about the article, not the article itself.

Abstract

Abstract The study of a time-periodic solution of the multidimensional wave equation ∂ 2 ∂ ⁡ t 2 ⁢ u ~ - Δ x ⁢ u ~ = f ~ ⁢ ( x , t ) {\frac{\partial^{2}}{\partial t^{2}}\widetilde{u}-\Delta_{x}\widetilde{u}=% \widetilde{f}(x,t)} , u ~ ⁢ ( x , t ) = e i ⁢ k ⁢ t ⁢ u ⁢ ( x ) {\widetilde{u}(x,t)=e^{ikt}u(x)} , over the whole space ℝ 3 {\mathbb{R}^{3}} leads to the condition of the Sommerfeld radiation at infinity. This is a problem that describes the motion of scattering stationary waves from a source that is in a bounded area. The inverse problem of finding this source is equivalent to reducing the Sommerfeld problem to a boundary value problem for the Helmholtz equation in a finite domain. Therefore, the Sommerfeld problem is a special inverse problem. It should be noted that in the work of Bezmenov [I. V. Bezmenov, Transfer of Sommerfeld radiation conditions to an artificial boundary of the region based on the variational principle, Sb. Math. 185 1995, 3, 3–24] approximate forms of such boundary conditions were found. In [T. S. Kalmenov and D. Suragan, Transfer of Sommerfeld radiation conditions to the boundary of a limited area, J. Comput. Math. Math. Phys. 52 2012, 6, 1063–1068], for a complex parameter λ, an explicit form of these boundary conditions was found through the boundary condition of the Helmholtz potential given by the integral in the finite domain Ω: ($*$) u ⁢ ( x , λ ) = ∫ Ω ε ⁢ ( x - ξ , λ ) ⁢ ρ ⁢ ( ξ , λ ) </