Six-parameter solution of the Einstein–Maxwell equations possessing equatorial symmetry

DOI10.1063/1.531012zbMath0853.35124OpenAlexW1976397771MaRDI QIDQ4873328

Eduardo Ruiz, V. S. Man'ko, Jesús San Martín

Publication date: 12 January 1997

Published in: Journal of Mathematical Physics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1063/1.531012

zbMATH Keywords

complex potentialsmetric functionstwo-soliton solution of the Einstein-Maxwell equations

Mathematics Subject Classification ID

PDEs in connection with relativity and gravitational theory (35Q75) Einstein-Maxwell equations (83C22)

Related Items (7)

Approximate universal relations for neutron stars and quark stars ⋮ Metric of a rotating charged magnetized sphere ⋮ GRAVITATIONAL FIELD AND ELECTRIC FORCE LINES OF A NEW 2-SOLITON SOLUTION ⋮ Slowly-rotating compact objects: the nonintegrability of Hartle-Thorne particle geodesics ⋮ A note on magnetic generalizations of the Kerr and Kerr–Newman solutions ⋮ A note on hierarchy of universal relations for neutron stars in terms of multipole moments ⋮ A note on the factor structure of some non-rational vacuum metrics

Cites Work

• Conditions for Regularity on the Symmetry Axis in a Superposition of Two Kerr-NUT Solutions
• Equilibrium of Two Rotating Charged Black Holes and the Dirac String
• Gravitational Field of a Spinning Mass as an Example of Algebraically Special Metrics
• Kerr–Newman metric endowed with magnetic dipole moment
• New Solutions of the Einstein-Maxwell Equations from Old
• Empty-Space Generalization of the Schwarzschild Metric
• Eine rotationssymmetrische Lösung in der allgemeinen Relativitätstheorie

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