Exact solutions in general relativity

mathematical space setting which eases explanation of special relativity

spherically symmetric static vacuum solution of Einstein’s field equations with zero cosmological constant

metric properties of the spacetime based on Albert Einstein's metric tensor and field solution for the spacetime

hypothetical mode of transportation by warping space

exact solution for the Einstein field equations

spherically symmetric metric with electric charge

model of the universe that is not expanding or contracting, e.g. one in which the cosmological constant exactly balances things

cosmological solution to the Einstein field equations of general relativity

maximally symmetric Lorentzian manifold with negative cosmological constant, which appears in the AdS/CFT correspondence

maximally symmetric Lorentzian manifold with positive cosmological constant

exact solution of the Einstein field equations describing the spacetime around an electrically charged and rotating mass

Interaction of two bodies in general relativity

solution of Einstein field equations with a a homogeneous distribution of swirling dust particles and a negative cosmological constant, featuring closed timelike curves

ordinary differential equation describing an isotropic spherical body in static gravitational equilibrium in general relativity

general relativity model near the beginning of the universe

Lorentzian manifold with vanishing Einstein tensor

cosmological model equivalent to a zero-energy-density FLRW model

exact solution in general relativity with a stress–energy tensor consisting of positive energy density and zero pressure

exact solution of the Einstein field equation with dust rotating about an axis of cylindrical symmetry

classification of the possible algebraic symmetries of the Weyl tensor at each point in a Lorentzian manifold

solution of Einstein field equations

Exercise in general relativity

particular set of coordinates for the Schwarzschild metric

asymptotically locally flat (ALF) hyperkähler manifold

class of exact solutions to Einstein's field equations

Lorentzian metric describing an isotropic, expanding, nonhomogenous universe

non-empty external spacetime of a spherically symmetric and nonrotating star which is either emitting or absorbing null dusts