Dark Matter, Modified Gravity and the Mass of the Neutrino
arXiv:0806.0116 · doi:10.1103/PhysRevD.78.044043
Abstract
It has been suggested that Einstein's theory of General Relativity can be modified to accomodate mismatches between the gravitational field and luminous matter on a wide range of scales. Covariant theories of modified gravity generically predict the existence of extra degrees of freedom which may be interpreted as dark matter. We study a subclass of these theories where the overall energy density in these extra degrees of freedom is subdominant relative to the baryon density and show that they favour the presence of massive neutrinos. For some specific cases (such as a flat Universes with a cosmological constant) one finds a conservative lower bound on the neutrinos mass of eV.
5 pages, 2 figures, 2 tables, submitted to Phys. Rev. D
References in corpus (7)
- New Hubble Space Telescope Discoveries of Type Ia Supernovae at z > 1: Narrowing Constraints on the Early Behavior of Dark Energy
- Can Cosmic Structure form without Dark Matter?
- Generalizing TeVeS Cosmology
- Can MOND take a bullet? Analytical comparisons of three versions of MOND beyond spherical symmetry
- On the growth of structure in theories with a dynamical preferred frame
- The cosmological behavior of Bekenstein's modified theory of gravity
- Testing Cosmology with Cosmic Sound Waves