Constraining symmetron fields with atom interferometry
arXiv:1609.09275 · doi:10.1088/1475-7516/2016/12/041
Abstract
We apply the new constraints from atom-interferometry searches for screening mechanisms to the symmetron model, finding that these experiments exclude a previously unexplored region of parameter space. We discuss the possibility of networks of domain walls forming in the vacuum chamber, and how this could be used to discriminate between models of screening.
12 pages, 2 figures
References in corpus (7)
- Beyond the Cosmological Standard Model
- Environmental Dependence of Masses and Coupling Constants
- Equivalence Principle Implications of Modified Gravity Models
- Gravity Resonance Spectroscopy Constrains Dark Energy and Dark Matter Scenarios
- Probing Dark Energy with Atom Interferometry
- Neutron Interferometry constrains dark energy chameleon fields
- Atomic Interferometry Test of Dark Energy
Cited by in corpus (4)
- Acoustic Rabi oscillations between gravitational quantum states and impact on symmetron dark energy
- Constraints on mediator-based dark matter and scalar dark energy models using TeV collision data collected by the ATLAS detector
- The splashback radius in symmetron gravity
- An Electrostatic Analogy for Symmetron Gravity