A Baryonic Correction to General Relativity

Abstract

The baryon overdensity and the matching of the big bang explosion energy with gravitation can be solved by a cyclical baryonic bounce model with correction to the stress-energy tensor. Subtracting accretion energy from the CMBR allows enough baryons in nucleosynthesis to close the universe. Collapse to infinite density states must be prevented by energy losses at supranuclear densities. As long as the Einstein tensor is coupled to the stress-energy tensor, any quantum correction must involve an energy sink.