On the equivalence of approximate stationary axially symmetric solutions of the Einstein field equations

DOI10.1134/S0202289316040046zbMath1380.83041arXiv1510.02035OpenAlexW3099670277MaRDI QIDQ683701

Hernando Quevedo, Medeu Abishev, Kuantay Boshkayev, Saken Toktarbay, Bakytzhan Zhami

Publication date: 8 February 2018

Published in: Gravitation \& Cosmology (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1510.02035

Mathematics Subject Classification ID

Black holes (83C57) Applications of differential geometry to physics (53Z05) Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar structure (85A15) Exact solutions to problems in general relativity and gravitational theory (83C15)

Related Items (2)

Approximate perfect fluid solutions with quadrupole moment ⋮ Geodesics in the field of a rotating deformed gravitational source

Cites Work

• A slowly rotating perfect fluid body in an ambient vacuum
• Rotating stars in relativity

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