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Identification of a time-dependent UV-photon source in an interstellar cloud
Authors:Aldo Belleni-Morante  Francesco Mugelli
Affiliation:(1) Dipartimento di Ingegneria Civile, via di S. Marta 3, 50139 Firenze, Italia,;(2) Dipartimento di Matematica Applicata, via di S. Marta 3, 50139 Firenze, Italia,
Abstract:Abstract Consider an interstellar cloud that occupies the region $Vsubset{mathbb R}^3$ , bounded by the known surface $partial V$ , and assume that the scattering cross section σs and the total cross section σ are also known. Then, we prove that it is possible to identify the source q=q(x,t) that produces UV-photons inside the cloud, provided that the UV-photon distribution function arriving at a location $widehat{{mathbf x}}$ , far from the cloud, is measured at times $widehat{t}_0$ , $widehat{t}_1 = widehat{t}_0+tau$ , ..., $widehat{t}_J = widehat{t}_0+Jtau$ . Keywords: Photon transport, Semigroups and linear evolution equations, Inverse problems Mathematics Subject Classification (2000): 82A25, 82C70, 34K29, 65M32
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