Toward a Complete Analysis of the Global Structure of Kerr-Newman Spacetime
| dc.creator | Kim, Hongsu | |
| dc.date | 1997-06-02 | |
| dc.date.accessioned | 2026-07-07T03:31:38Z | |
| dc.date.available | 2026-07-07T03:31:38Z | |
| dc.description | An attempt is made to supplement Carter's partial investigation of the global structure of Kerr-Newman spacetime on the symmetry axis. Namely, the global structure of θ= const. timelike submanifolds of Kerr-Newman metric starting from the symmetry axis all the way down to the equatorial plane are studied by introducing a new time coordinate slightly different from the usual Boyer-Lindquist time coordinate. It turns out that the maximal anaytic extension of θ= θ_0 (0 \leq θ_0 < π/2) submanifolds is the same as that of the symmetry axis first studied by Carter whereas θ= π/2 equatorial plane has the topology identical to that of the Reissner-Nordstrom spacetime. General applicability of this method to Kerr-Newman-type black hole solutions in other gravity theories is discussed as well. | |
| dc.description | 18 pages, Revtex | |
| dc.identifier | https://arxiv.org/abs/gr-qc/9706003 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/9706003 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/35935 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.subject | High Energy Physics - Theory | |
| dc.title | Toward a Complete Analysis of the Global Structure of Kerr-Newman Spacetime | |
| dc.type | text |