Kavli Affiliate: Edmund Bertschinger | Summary:The metric of a perturbed Robertson-Walker spacetime is characterized by three functions: a scale-factor giving the expansion history and two potentials which generalize the single potential of Newtonian gravity. The Newtonian potential induces peculiar velocities and, from these, the growth of matter fluctuations. Massless particles respond equally to the Newtonian […]
Continue.. One Gravitational Potential or Two? Forecasts and Tests