FTP, identify this namesake of a value equal to 2GM over c-squared, which is the radius to which an object would need to be compressed in order to become a black hole.
Together with Milne, he is the namesake of an integral equation that describes an isotropically scattering medium, and his namesake distribution function is a solution to the collision-less Boltzmann equation in the epicycle approximation. The vertical temperature gradient is greater than the adiabatic temperature gradient according to his namesake criterion which describes the stability in gravitationally bound plasma. His coordinate system can be used to describe a static and spherically symmetric spacetime such as his famous solution to the vacuum Einstein field equations. FTP, identify this namesake of a value equal to 2GM over c-squared, which is the radius to which an object would need to be compressed in order to become a black hole.
Together with Milne, he is the namesake of an integral equation that describes an isotropically scattering medium, and his namesake distribution function is a solution to the collision-less Boltzmann equation in the epicycle approximation.
Karl {Schwarzschild}