An exact solution, assuming spherical symmetry, for the equations of motion may be obtained by inserting a metric tensor into the Einstein field equations. This metric tensor is diagonal and provides for the radial and time coordinates to be functions that are obtained as a solution to the field equations.

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Schwarzschild Solution for Spherical Symmetry

  • James Miller,
  • Connie Weeks

摘要

An exact solution, assuming spherical symmetry, for the equations of motion may be obtained by inserting a metric tensor into the Einstein field equations. This metric tensor is diagonal and provides for the radial and time coordinates to be functions that are obtained as a solution to the field equations.