Tuning the Mass of Chameleon Fields in Casimir Force Experiments
arXiv:1003.1605 · doi:10.1103/PhysRevLett.104.241101
Abstract
We have calculated the chameleon pressure between two parallel plates in the presence of an intervening medium that affects the mass of the chameleon field. As intuitively expected, the gas in the gap weakens the chameleon interaction mechanism with a screening effect that increases with the plate separation and with the density of the intervening medium. This phenomenon might open up new directions in the search of chameleon particles with future long range Casimir force experiments.
submitted for publication on March 8, 2010
References in corpus (6)
- Evading Equivalence Principle Violations, Cosmological and other Experimental Constraints in Scalar Field Theories with a Strong Coupling to Matter
- Halving the Casimir force with conductive oxides
- Anomalies in electrostatic calibrations for the measurement of the Casimir force in a sphere-plane geometry
- Detecting Chameleons through Casimir Force Measurements
- Development of a high sensitivity torsional balance for the study of the Casimir force in the 1-10 micrometer range
- An experimental apparatus for measuring the Casimir effect at large distances
Cited by in corpus (36)
- Tests of Chameleon Gravity
- A Compendium of Chameleon Constraints
- Strongly Coupled Chameleons and the Neutronic Quantum Bouncer
- Neutron Interferometry constrains dark energy chameleon fields
- Dark energy fifth forces in torsion pendulum experiments
- Chameleons with Field Dependent Couplings
- Laboratory Tests of the Galileon
- Chameleon dark energy models with characteristic signatures
- Symmetron dark energy in laboratory experiments
- Force sensor for chameleon and Casimir force experiments with parallel-plate configuration
- Using Atom Interferometry to Detect Dark Energy
- Chameleons in the Early Universe: Kicks, Rebounds, and Particle Production
- The Classical Symmetron Force in Casimir Experiments
- Atomic Interferometry Test of Dark Energy
- Catastrophic Consequences of Kicking the Chameleon
- Casimir, Gravitational and Neutron Tests of Dark Energy
- Constraints on axion-like particles and non-Newtonian gravity from measuring the difference of Casimir forces
- Chameleon Gravity, Electrostatics, and Kinematics in the Outer Galaxy
- Radiative Screening of Fifth Forces
- Derivative Chameleons
- Chameleon foreCAST
- Ellipticity Weakens Chameleon Screening
- Next generation design and prospects for CANNEX
- Quantum Chameleons
- Detecting solar chameleons through radiation pressure
- Strongly coupled chameleon fields: possible test with a neutron Lloyd's mirror interferometer
- Mixing rules and the Casimir force between composite systems
- Cosmology of Chameleons with Power-Law Couplings
- Constraining modified gravity with quantum optomechanics
- Unparticle Casimir effect
- Fluctuation-induced Interactions in Micro- and Nano-systems: Survey of Some Basic Results
- Chameleon Fragmentation
- Potential of the neutron Lloyd's mirror interferometer for the search for new interactions
- Dynamical Casimir effect with screened scalar fields
- Constraints on strongly coupled chameleon fields from the experimental test of the weak equivalence principle for the neutron
- Testing Exponential Gravity with CMB, DESI-DR2, and Supernova Data