Dynamical Instability of Gaseous Masses Approaching the Schwarzschild Limit in General Relativity

Abstract

the correct acceleration in the rate of separation of these galaxies.However, we emphasize that the nearby galaxies can produce only extremely small tidal stresses within our galaxy, and these stresses are further reduced because the nearby galaxies are distributed in an approximately isotropic way.That is, contrary to the claims of Pachner, ' general relativity implies no apprecia- ble connection between the evolution of our solar system, and our galaxy, and the rest of the mat- ter in the universe.