Attractive and Repulsive Gravity
Philip D. Mannheim
Abstract
We discuss the circumstances under which gravity might be repulsive rather than attractive. In particular we show why our standard solar system distance scale gravitational intuition need not be a reliable guide to the behavior of gravitational phenomena on altogether larger distance scales such as cosmological, and argue that in fact gravity actually gets to act repulsively on such distance scales. With such repulsion a variety of current cosmological problems (the flatness, horizon, dark matter, universe age, cosmic acceleration and cosmological constant problems) are then all naturally resolved.
Create a lesson
Related papers
Non-Commutativity in Geodesic Congruences
Aarav Shah, Louis H. Kauffman
Scalar wave dark matter imprints on binary black hole mergers: dependence on field mass and density
Yu-Peng Zhang, Shao-Wen Wei, Yu-Xiao Liu
Quantum Energy Inequalities with a twist: rotating frames along stationary worldlines
Christopher J. Fewster, Daniel Lomax Ford
Analytic Electromagnetic Effective Source for Geodesic Orbit in Schwarzschild Spacetime
Xuchen Lu, Yungui Gong, Bokai Zhang et al.
Stability conditions for light rings in circular stationary axisymmetric spacetimes
Jake O. Shipley
Post-Newtonian secular dynamics of hierarchical triples II. Canonical derivation of the 1PN\,×\,quadrupole cross terms and of the quadrupole-squared term
Hideyoshi Arakida