Exact black-hole solution with self-interacting scalar field
Authors:
- Olaf BechmannOBOlaf Bechmann
- Olaf LechtenfeldOLOlaf Lechtenfeld
- 1 June 1995
- journal article
- Published by IOP Publishing in Classical and Quantum Gravity
- Vol. 12 (6) , 1473-1481
Abstract
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This publication has 15 references indexed in Scilit:
- Staticity and uniqueness of multiple black hole solutions of sigma -modelsClassical and Quantum Gravity, 1993
- A no-hair theorem for self-gravitating nonlinear sigma modelsJournal of Mathematical Physics, 1992
- Nonmeasurability of the Quantum Numbers of a Black HolePhysical Review D, 1972
- Nonspherical Perturbations of Relativistic Gravitational Collapse. II. Integer-Spin, Zero-Rest-Mass FieldsPhysical Review D, 1972
- Nonspherical Perturbations of Relativistic Gravitational Collapse. I. Scalar and Gravitational PerturbationsPhysical Review D, 1972
- Nonexistence of Baryon Number for Black Holes. IIPhysical Review D, 1972
- Nonexistence of Baryon Number for Static Black HolesPhysical Review D, 1972
- Axisymmetric Black Hole Has Only Two Degrees of FreedomPhysical Review Letters, 1971
- Event horizons in static electrovac space-timesCommunications in Mathematical Physics, 1968
- Event Horizons in Static Vacuum Space-TimesPhysical Review B, 1967