Chameleon Gravity, Electrostatics, and Kinematics in the Outer Galaxy
arXiv:1109.0538 · doi:10.1088/1475-7516/2011/12/005
Abstract
Light scalar fields are expected to arise in theories of high energy physics (such as string theory), and find phenomenological motivations in dark energy, dark matter, or neutrino physics. However, the coupling of light scalar fields to ordinary (or dark) matter is strongly constrained from laboratory, solar system, and astrophysical tests of fifth force. One way to evade these constraints in dense environments is through the chameleon mechanism, where the field's mass steeply increases with ambient density. Consequently, the chameleonic force is only sourced by a thin shell near the surface of dense objects, which significantly reduces its magnitude. In this paper, we argue that thin-shell conditions are equivalent to "conducting" boundary conditions in electrostatics. As an application, we use the analogue of the method of images to calculate the back-reaction (or self-force) of an object around a spherical gravitational source. Using this method, we can explicitly compute the violation of equivalence principle in the outskirts of galactic haloes (assuming an NFW dark matter profile): Intermediate mass satellites can be slower than their larger/smaller counterparts by as much as 10% close to a thin shell.
17 pages, 3 figures
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- Cosmological Tests of Modified Gravity
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- Chameleon Dark Energy and Atom Interferometry
- Constraining chameleon models with cosmology
- The Novel Probes Project -- Tests of Gravity on Astrophysical Scales
- Chameleon f(R) gravity in the virialized cluster
- Halo modelling in chameleon theories
- Cluster abundance in chameleon gravity I: toward an accurate halo mass function prediction
- An observational test of the Vainshtein mechanism
- The influence of the chameleon field potential on transition frequencies of gravitationally bound quantum states of ultra-cold neutrons
- A parametrisation of modified gravity on nonlinear cosmological scales
- Post-Newtonian parameters and cosmological constant of screened modified gravity
- Halo Scale Predictions of Symmetron Modified Gravity
- Gas density profile in dark matter halo in chameleon cosmology
- Simulation tests of galaxy cluster constraints on chameleon gravity
- Derivative Chameleons
- Probing Modified Gravity with Atom-Interferometry: a Numerical Approach
- Early Modified Gravity: Implications for Cosmology
- Signatures of Modified Gravity on the 21-cm Power Spectrum at Reionisation
- How chameleons core dwarfs with cusps
- Particle level screening of scalar forces in 1+1 dimensions
- An Electrostatic Analogy for Symmetron Gravity
- Tsunamis and Ripples: Effects of Scalar Waves on Screening in the Milky Way
- Total screening and finite range forces from ultra-massive scalar fields
- What to expect from scalar-tensor space geodesy