Null Strings in Schwarzschild Spacetime
arXiv:hep-th/9610243 · doi:10.1103/PhysRevD.55.6409
Abstract
The null string equations of motion and constraints in the Schwarzschild spacetime are given. The solutions are those of the null geodesics of General Relativity appended by a null string constraint in which the "constants of motion" depend on the world-sheet spatial coordinate. Because of the extended nature of a string, the physical interpretation of the solutions is completely different from the point particle case. In particular, a null string is generally not propagating in a plane through the origin, although each of its individual points is. Some special solutions are obtained and their physical interpretation is given. Especially, the solution for a null string with a constant radial coordinate moving vertically from the south pole to the north pole around the photon sphere, is presented. A general discussion of classical null/tensile strings as compared to massless/massive particles is given. For instance, tensile circular solutions with a constant radial coordinate do not exist at all. The results are discussed in relation to the previous literature on the subject.
16 pages, REVTEX, no figures
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- Null Branes in Curved Backgrounds
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- Null Cosmic Strings: Scattering by Black Holes, Optics and Spacetime Content
- Electrodynamics under Action of Null Cosmic Strings
- Null Strings and Membranes in Demianski-Newman Background
- Open Cosmic Strings in Black Hole Space-Times
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