Symmetron Fields: Screening Long-Range Forces Through Local Symmetry Restoration
arXiv:1001.4525 · doi:10.1103/PhysRevLett.104.231301
Abstract
We present a screening mechanism that allows a scalar field to mediate a long range (~Mpc) force of gravitational strength in the cosmos while satisfying local tests of gravity. The mechanism hinges on local symmetry restoration in the presence of matter. In regions of sufficiently high matter density, the field is drawn towards ϕ= 0 where its coupling to matter vanishes and the ϕ-> -ϕsymmetry is restored. In regions of low density, however, the symmetry is spontaneously broken, and the field couples to matter with gravitational strength. We predict deviations from general relativity in the solar system that are within reach of next-generation experiments, as well as astrophysically observable violations of the equivalence principle. The model can be distinguished experimentally from Brans-Dicke gravity, chameleon theories and brane-world modifications of gravity.
4 pages. v3: version appearing in PRL
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- Dynamical Chameleon Neutron Stars: stability, radial oscillations and scalar radiation in spherical symmetry
- Equatorial orbits and imaging of hairy cubic Galileon black holes
- Phenomenological footprints of Lambda varying gravity theories inspired from quantum gravity models in the multi-messenger era
- Single scale factor for the universe from the creation of radiation and matter till the present
- Astro- and Quantum Physical Tests of Screened Scalar Fields
- A Neutron Star with a Strange Quark Star-like Mass-Radius Relation
- A density-responsive scalar-field framework for singularity regularization and dynamical dark energy
- Solar System Experiments in the Search for Dark Energy and Dark Matter
- Quantum corrections to symmetron fifth-force profiles
- Bose-Einstein condensates in microgravity and fundamental tests of gravity
- Dark Energy Simulations
- Mass Varying Neutrino Oscillation in Scalar-Gauss-Bonnet Gravity
- Exceeding the conformal limit inside rotating neutron stars: Implications to modified theories of gravity
- Apparent and a Lower from Dark Axion and Dark Baryons Interactions
- Constraining scalar-tensor theories from higher harmonics with GW230529
- Onset of dark energy from cosmological scalarization and gravitational wave speed
- Structural Implications of the Chameleon Mechanism on White Dwarfs
- Fifth forces and discrete symmetry breaking
- Scalarization and superradiant instability of black hole induced by dark matter halo in the scalar-tensor theory of gravity
- Forecast constraints on null tests of the CDM model with SPHEREx
- Fullshape power spectrum for the Symmetron modified gravity model
- An introduction to axions and their detection
- Gravitational waves from dark domain walls
- Higgs-Induced Screening Mechanisms in Scalar-Tensor Theories
- Post-Newtonian Constraints on Scalar-Tensor Gravity
- Neutron Stars in Scalar Torsion Theories with Nonminimal Coupling
- Testing the growth of cosmic structures during the Dark Ages
- Large scale structures: from inflation to today: a brief report
- Categorizing models using Self-Organizing Maps: an application to modified gravity theories probed by cosmic shear
- A Faster Growth of Perturbations in an Early Matter Dominated Epoch: Primordial Black Holes and Gravitational Waves
- Implications of a high growth index on the variation of
- Origin & evolution of the Universe
- Quantum Physics in Space
- Ray-traced weak lensing convergence in screened modified gravity theories
- Post-Newtonian N-Body Dynamics in Extended Theories of Gravity
- Luminosity-Temperature Relation as a Probe for Modified Gravity
- Geodesics in Quantum Gravity
- Constraining runaway dilaton models using joint gravitational-wave and electromagnetic observations
- On Generalized Theories of Varying Fine Structure Constant
- Distinguishing gravity theories with networks of space-based gravitational-wave detectors