Inverse scattering at high energies for the multidimensional relativistic Newton equation in a long-range electromagnetic field

direct consequence of the two properties established in the preceding section is that these measurements would be unchanged if the part of the structure located below

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On the other hand, in view of the Born rule, from applied point of view, Problems 1.3a, 1.3b and similar phaseless inverse scattering problems are much more important than

On the other hand, it was found in [20], [21] (see also [23], [26]) that for inverse problems for the Schr¨ odinger equation at fixed energy E in dimension d ≥ 2 (like Problem

Error estimates for phaseless inverse scattering in the Born approximation at high energies.. Alexey Agaltsov,

Therefore we shall modify in Section 3 the definition of the scattering map to study these modified scattering data in the following three asymptotic regimes: at high energies,

We consider the inverse scattering problem at fixed and sufficiently large energy for the nonrelativistic and relativistic Newton equation in R n , n ≥ 2, with a smooth and short

Therefore we shall modify in Section 3 the definition of the scattering map to study these modified scattering data in the following three asymptotic regimes: at high energies,