The static, cylindrically symmetric strings in general relativity with cosmological constant
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Publication:3723254
DOI10.1063/1.527050zbMath0593.53040OpenAlexW2059197055MaRDI QIDQ3723254
Publication date: 1986
Published in: Journal of Mathematical Physics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1063/1.527050
Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Partial differential equations of mathematical physics and other areas of application (35Q99) Applications of local differential geometry to the sciences (53B50)
Related Items (22)
Cylindrical asymmetric thin-shell wormholes ⋮ A family of strings with spin ⋮ Relativistic Bessel cylinders ⋮ Static cylindrically symmetric gravitational field with cosmological constant ⋮ Conformally flat sources for the Linet-Tian spacetime ⋮ Construction of Einstein metrics by generalized Dehn filling ⋮ Cylindrically symmetric scalar field and it's Lyapunov stability in general relativity ⋮ Exact string-like solutions in conformal gravity ⋮ Geodesics dynamics in the Linet-Tian spacetime with \(\Lambda<0\) ⋮ Fermionic vacuum polarization by a cosmic string in de Sitter spacetime ⋮ Geometry of AdS-Melvin spacetimes ⋮ Linear perturbations of the Linet–Tian metrics with a positive cosmological constant ⋮ Translation in cylindrically symmetric vacuum ⋮ Higher Order Gravity Theories and Their Black Hole Solutions ⋮ Black hole enthalpy and scalar fields ⋮ A NOTE ON CONSTANT CURVATURE SOLUTIONS IN CYLINDRICALLY SYMMETRIC METRIC f(R) GRAVITY ⋮ EXACT SOLUTION FOR THE MASSLESS CYLINDRICALLY SYMMETRIC SCALAR FIELD IN GENERAL RELATIVITY, WITH COSMOLOGICAL CONSTANT ⋮ Non-expanding Plebański–Demiański space-times ⋮ Cylindrically symmetric vacuum solutions in higher dimensional Brans–Dicke theory ⋮ The Linet–Tian metrics are a restricted set of Krasiński’s solutions of Einstein’s field equations for a rotating perfect fluid ⋮ Levi-Civita cylinders with fractional angular deficit ⋮ Cylindrically symmetric static solutions of the Einstein field equations for elastic matter
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