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NASA NTRS ยท 19760060010

An improved radiation metric

Abstract

An improved radiation metric is obtained in which light rays make a small nonzero angle with the radius, thus representing a source of finite size. Kaufmann's previous solution is criticized. The stabilization of a scatterer near a source of gravitational field and radiation is slightly enhanced for sources of finite size.

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BibTeXRIS

Noerdlinger, P. D.. 1976-01-01. An improved radiation metric. https://ntrs.nasa.gov/citations/19760060010

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