Radial acceleration relation from symmetron fifth forces

Tools

Burrage, Clare, Copeland, Edmund J. and Millington, Peter (2017) Radial acceleration relation from symmetron fifth forces. Physical Review D, D95 (6). 064050/1-064050/6. ISSN 2470-0029

Full text not available from this repository.

Abstract

We show that the radial acceleration relation for rotationally supported galaxies may be explained, in the absence of cold dark matter, by a nonminimally coupled scalar field, whose fifth forces are partially screened on galactic scales by the symmetron mechanism. In addition, we show that sufficient energy is stored in the symmetron field to explain the dynamic stability of galactic disks.

Item Type: Article
RIS ID: https://nottingham-repository.worktribe.com/output/852715
Schools/Departments: University of Nottingham, UK > Faculty of Science > School of Physics and Astronomy
Identification Number: https://doi.org/10.1103/PhysRevD.95.064050
Depositing User: Burrage, Clare
Date Deposited: 20 Apr 2017 12:14
Last Modified: 04 May 2020 18:39
URI: https://eprints.nottingham.ac.uk/id/eprint/42086

Actions (Archive Staff Only)

Edit View Edit View