Geodesic
Exterior fields of collapsed bodies
Teoretičeskaâ i matematičeskaâ fizika, Tome 24 (1975) no. 1, pp. 136-140 Cet article a éte moissonné depuis la source Math-Net.Ru

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Static spherically symmetric solutions of the Einstein equations (without the cosmological term) and the Schrödinger–Fock–Klein (or Proca) equations with the massive scalar field $\varphi$ (or vector field $B_{\mu}$) in the central coordinate system with the interval $ds^2=e^{\nu}dx^{0\,2} -e^{\lambda}dr^2-r^2d\Omega^2$ are investigated. It is shown that every solution $\{\nu, \lambda, \varphi\}$ $(resp., \{\nu, \lambda, B_{\mu}\})$ with asymptotically flat metrics and $\varphi\not\equiv 0$ $(resp., B_{\mu}\not\equiv 0)$ is regular with respect to $r$ in the interval $(0,\infty)$. 
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A. A. Solodov. Exterior fields of collapsed bodies. Teoretičeskaâ i matematičeskaâ fizika, Tome 24 (1975) no. 1, pp. 136-140. http://geodesic.mathdoc.fr/item/TMF_1975_24_1_a16/

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