Weakly dissipative plasma equilibria in Kerr geometry
Axisymmetric neutral plasma equilibria of electrons and ions near black holes can be constructed from solutions of ideal multifluid equations; the solutions for the ions are obtained from a modified Grad–Shafranov code for the stream function. The density and the flux functions are determined self-c...
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Veröffentlicht in: | Physics of plasmas 2004-01, Vol.11 (1), p.278-285 |
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description | Axisymmetric neutral plasma equilibria of electrons and ions near black holes can be constructed from solutions of ideal multifluid equations; the solutions for the ions are obtained from a modified Grad–Shafranov code for the stream function. The density and the flux functions are determined self-consistently from the normalization of the Eulerian four-velocity and a simple dissipation model for the ions, respectively. Solutions with moderate or vanishing toroidal velocity exist, but the black hole receives matter only in nonequilibrium situations. |
doi_str_mv | 10.1063/1.1630967 |
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The density and the flux functions are determined self-consistently from the normalization of the Eulerian four-velocity and a simple dissipation model for the ions, respectively. Solutions with moderate or vanishing toroidal velocity exist, but the black hole receives matter only in nonequilibrium situations.</abstract><doi>10.1063/1.1630967</doi><tpages>8</tpages></addata></record> |
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title | Weakly dissipative plasma equilibria in Kerr geometry |
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