We extend the thermodynamic theory of gravitational clustering in an expanding Universe to include the scale dependence of the ratio, b, of gravitational correlation energy to thermal energy. The predicted form of the gravitational quasi-equilibrium distribution function is unchanged by this scale dependence. This generalization of the theory contains no free parameters, and clariies many earli...

Abstract In the seventy-five years since end of World War II, pairs countries have entered into over a thousand bilateral labor agreements (BLAs) to regulate cross-border flow workers. These received little public or academic attention. This is likely, in part, because there limited data easily available information on BLAs. Article hopes change that by introducing three new resources: (1) data...

The 5D Cosmological General Relativity theory developed by Carmeli reproduces all of the results that have been successfully tested for Einstein’s 4D theory. However the Carmeli theory because of its fifth dimension, the velocity of the expanding universe, predicts something different for the propagation of gravity waves on cosmological distance scales. This analysis indicates that gravitationa...