For a homologous, isolated collapsing sphere, write its Newtonian gravitational potential energy as . At spherical-collapse turnaround the coherent kinetic energy vanishes. Conserving total energy and applying the virial theorem to the final equilibrium gives and hence . If the gravitational structure coefficient changes, the ratio is instead. Mass loss, surface pressure, external tides and energy exchange also change this estimate.
Articles by others on the same topic
There are currently no matching articles.