Exact solutions in general relativity

Interior Schwarzschild metric

In Einstein's theory of general relativity, the interior Schwarzschild metric (also interior Schwarzschild solution or Schwarzschild fluid solution) is an exact solution for the gravitational field in the interior of a non-rotating spherical body which consists of an incompressible fluid (implying that density is constant throughout the body) and has zero pressure at the surface. This is a static solution, meaning that it does not change over time. It was discovered by Karl Schwarzschild in 1916, who earlier had found the exterior Schwarzschild metric. (Wikipedia).

Interior Schwarzschild metric
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πŸ‘‰ Learn about the interior and the exterior angles of a polygon. A polygon is a plane shape bounded by a finite chain of straight lines. The interior angle of a polygon is the angle between two sides of the polygon. The sum of the interior angles of a regular polygon is given by the formul

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πŸ‘‰ Learn about the interior and the exterior angles of a polygon. A polygon is a plane shape bounded by a finite chain of straight lines. The interior angle of a polygon is the angle between two sides of the polygon. The sum of the interior angles of a regular polygon is given by the formul

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πŸ‘‰ Learn about the interior and the exterior angles of a polygon. A polygon is a plane shape bounded by a finite chain of straight lines. The interior angle of a polygon is the angle between two sides of the polygon. The sum of the interior angles of a regular polygon is given by the formul

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Spherical cap | Albert Einstein | Exact solutions in general relativity | Diagonal matrix | Density | Gravitational constant | Parabola | Einstein tensor | Colatitude | Radian | Curvature of Riemannian manifolds | Spherical coordinate system | Embedding | Isotropy | Static spherically symmetric perfect fluid | Line element | Gaussian curvature | Neutron star | Speed of light