= Inversion of restricted ray transforms of symmetric tensor fields in n-dimensional Euclidean space =

We derive explicit inversion formulas recovering the solenoidal part of a symmetric m-tensor field on n-dimensional Euclidean space from the restricted ray transform. The set of lines we consider are all lines passing through a curve satisfying the so-called Kirillov-Tuy type condition.

'''People''': Venkateswaran P. Krishnan and Rohit Kumar Mishra <<BR>>
'''Status''': Paper in preparation