Identification of a localized source in an interstellar cloud: an inverse problem
Atti della Accademia nazionale dei Lincei. Rendiconti Lincei. Matematica e applicazioni, Série 9, Tome 16 (2005) no. 3, pp. 203-209

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We study an inverse problem for photon transport in an interstellar cloud. In particular, we evaluate the position $x_{0}$ of a localized source $q(x) = q_{0} \delta(x-x_{0})$, inside a nebula (for example, a star). We assume that the photon transport phenomenon is one-dimensional. Since a nebula moves slowly in time, the number of photons $U$ inside the cloud changes slowly in time. For this reason, we consider the so-called quasi-static approximation $u$ to the exact solution $U$. By using semigroup theory, we prove existence and uniqueness of $u$. Because of some monotonic properties of the operator which describes $u$ as a function of $q$, the «position» of the source can be evaluated.
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     author = {Lisi, Meri and Totaro, Silvia},
     title = {Identification of a localized source in an interstellar cloud: an inverse problem},
     journal = {Atti della Accademia nazionale dei Lincei. Rendiconti Lincei. Matematica e applicazioni},
     pages = {203--209},
     publisher = {mathdoc},
     volume = {Ser. 9, 16},
     number = {3},
     year = {2005},
     zbl = {1225.82059},
     mrnumber = {MR2227744},
     language = {en},
     url = {http://geodesic.mathdoc.fr/item/RLIN_2005_9_16_3_a5/}
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Lisi, Meri; Totaro, Silvia. Identification of a localized source in an interstellar cloud: an inverse problem. Atti della Accademia nazionale dei Lincei. Rendiconti Lincei. Matematica e applicazioni, Série 9, Tome 16 (2005) no. 3, pp. 203-209. http://geodesic.mathdoc.fr/item/RLIN_2005_9_16_3_a5/