Progress in relativistic gravitational theory using the inverse scattering method

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dc.creatorNeugebauer, G.
dc.creatorMeinel, R.
dc.date2003-04-23
dc.date.accessioned2026-07-07T10:28:04Z
dc.date.available2026-07-07T10:28:04Z
dc.descriptionThe increasing interest in compact astrophysical objects (neutron stars, binaries, galactic black holes) has stimulated the search for rigorous methods, which allow a systematic general relativistic description of such objects. This paper is meant to demonstrate the use of the inverse scattering method, which allows, in particular cases, the treatment of rotating body problems. The idea is to replace the investigation of the matter region of a rotating body by the formulation of boundary values along the surface of the body. In this way we construct solutions describing rotating black holes and disks of dust ("galaxies"). Physical properties of the solutions and consequences of the approach are discussed. Among other things, the balance problem for two black holes can be tackled.
dc.description31 pages, 5 figures, to appear in J. Math. Phys
dc.identifierhttps://arxiv.org/abs/gr-qc/0304086
dc.identifierhttp://arxiv.org/abs/gr-qc/0304086
dc.identifierJ.Math.Phys.44:3407,2003
dc.identifierdoi:10.1063/1.1590419
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/177323
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Theory
dc.subjectMathematical Physics
dc.titleProgress in relativistic gravitational theory using the inverse scattering method
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