Structure Formation in the Symmetron Model
arXiv:1108.3081 · doi:10.1088/0004-637X/748/1/61
Abstract
Scalar fields, strongly coupled to matter, can be present in nature and still be invisible to local experiments if they are subject to a screening mechanism. The symmetron is one such mechanism which relies on restoration of a spontaneously broken symmetry in regions of high density to shield the scalar fifth force. We have investigated structure formation in the symmetron model by using N-body simulations and find strong observable signatures in both the linear and nonlinear matter power spectrum and on the halo mass function. The mechanism for suppressing the scalar fifth force in high density regions is also found to work very well.
18 pages, 15 figures
References in corpus (25)
- Evading Equivalence Principle Violations, Cosmological and other Experimental Constraints in Scalar Field Theories with a Strong Coupling to Matter
- Environmental Dependence of Masses and Coupling Constants
- f(R) Gravity and Chameleon Theories
- Symmetron Cosmology
- Non-linear Evolution of f(R) Cosmologies III: Halo Statistics
- Multi-field galileons and higher co-dimension branes
- Non-linear evolution of f(R) cosmologies II: power spectrum
- Strongly Coupled Chameleon Fields: New Horizons in Scalar Field Theory
- N-body Simulations for f(R) Gravity using a Self-adaptive Particle-Mesh Code
- Initial Conditions for Large Cosmological Simulations
- Cascading DGP
- Dynamical Masses in Modified Gravity
- Detecting Chameleons through Casimir Force Measurements
- The dispersion of growth of matter perturbations in f(R) gravity
- Accurate estimators of power spectra in N-body simulations
- Testing Chameleon Theories with Light Propagating through a Magnetic Field
- N-Body Simulations of Alternate Gravity Models
- Phantom boundary crossing and anomalous growth index of fluctuations in viable f(R) models of cosmic acceleration
- Chameleon dark energy models with characteristic signatures
- Cosmology of the selfaccelerating third order Galileon
- Hidden in the Light: Magnetically Induced Afterglow from Trapped Chameleon Fields
- Linear Growth of Structure in the Symmetron Model
- Dark Matter Gravitational Clustering With a Long-Range Scalar Interaction
- Cosmology of Chameleons with Power-Law Couplings
- Simulations of structure formation in interacting dark energy cosmologies
Cited by in corpus (83)
- Testing General Relativity with Present and Future Astrophysical Observations
- Beyond the Cosmological Standard Model
- Cosmology and Fundamental Physics with the Euclid Satellite
- Cosmological Tests of Modified Gravity
- A Unified Description of Screened Modified Gravity
- Astrophysical Tests of Modified Gravity: Constraints from Distance Indicators in the Nearby Universe
- Modified Gravity-GADGET: A new code for cosmological hydrodynamical simulations of modified gravity models
- The status of varying constants: a review of the physics, searches and implications
- Modified Gravity N-body Code Comparison Project
- The nonlinear matter and velocity power spectra in f(R) gravity
- Nonlinear structure formation in the Cubic Galileon gravity model
- Redshift space distortions in f(R) gravity
- ISIS: a new N-body cosmological code with scalar fields based on RAMSES. Code presentation and application to the shapes of clusters
- Releasing scalar fields: cosmological simulations of scalar-tensor theories for gravity beyond the static approximation
- Systematic simulations of modified gravity: symmetron and dilaton models
- The Novel Probes Project -- Tests of Gravity on Astrophysical Scales
- The parameter space in Galileon gravity models
- Testing the theory of gravity with DESI: estimators, predictions and simulation requirements
- Cosmological simulations of screened modified gravity out of the static approximation: effects on matter distribution
- Constraining gravity by the Large Scale Structure
- Nonlinear structure formation in Nonlocal Gravity
- Systematic simulations of modified gravity: chameleon models
- Gravitational radiation from compact binary systems in screened modified gravity
- Modelling Void Abundance in Modified Gravity
- Screening the fifth force in the Horndeski's most general scalar-tensor theories
- Efficient simulations of large scale structure in modified gravity cosmologies with comoving Lagrangian acceleration
- Symmetron Scalar Fields: Modified Gravity, Dark Matter or Both?
- Speeding up -body simulations of modified gravity: Chameleon screening models
- Environment Dependence of Dark Matter Halos in Symmetron Modified Gravity
- Hierarchical clustering in chameleon gravity
- A Fast Route to Non-Linear Clustering Statistics in Modified Gravity Theories
- The Vainshtein mechanism beyond the quasi-static approximation
- Halo velocity profiles in screened modified gravity theories
- Weak Lensing Galaxy Cluster Field Reconstruction
- The Classical Symmetron Force in Casimir Experiments
- Fast full N-body simulations of generic modified gravity: conformal coupling models
- Post-Newtonian parameters and cosmological constant of screened modified gravity
- Exact Solutions to Non-Linear Symmetron Theory: One and Two Mirror Systems
- The splashback radius in symmetron gravity
- Excursion set theory for modified gravity: correlated steps, mass functions and halo bias
- Halo Scale Predictions of Symmetron Modified Gravity
- Gravitational redshift profiles in the and symmetron models
- Fast full -body simulations of generic modified gravity: derivative coupling models
- Domain walls coupled to matter: the symmetron example
- Excursion set theory for modified gravity: Eulerian versus Lagrangian environments
- Gravitational transitions via the explicitly broken symmetron screening mechanism
- Symmetron and de Sitter attractor in a teleparallel model of cosmology
- Revealing modified gravity signal in matter and halo hierarchical clustering
- DM haloes in the fifth-force cosmology
- Spherical collapse and halo mass function in the symmetron model
- Testing General Relativity with Black Hole-Pulsar Binaries
- Cosmological simulations with disformally coupled symmetron fields
- Universal predictions of screened modified gravity on cluster scales
- Simulation techniques for modified gravity
- Weak lensing of large scale structure in the presence of screening
- Exact Solutions to Non-Linear Symmetron Theory II: One and Two Mirror Systems
- Spatial variations of the fine-structure constant in symmetron models
- Constraining Screened Modified Gravity by Space-borne Gravitational-wave Detectors
- Early Modified Gravity: Implications for Cosmology
- Screenings in Modified Gravity: a perturbative approach
- Signatures of Modified Gravity on the 21-cm Power Spectrum at Reionisation
- Breaking cosmic degeneracies: Disentangling neutrinos and modified gravity with kinematic information
- Cosmological simulations with hydrodynamics of screened scalar-tensor gravity with non-universal coupling
- Multi-component DHOST analysis in galaxy clusters
- Detecting Domain Walls in Laboratory Experiments
- Probing scalar tensor theories for gravity in redshift space
- Searching for Chameleon Dark Energy with Mechanical Systems
- Distinguishing screening mechanisms with environment-dependent velocity statistics
- asevolution: a relativistic N-body implementation of the (a)symmetron
- Probing modified gravity in cosmic filaments
- Imprints of screened dark energy on nonlocal quantum correlations
- Estimates of cluster masses in screened modified gravity
- Superradiant instabilities by accretion disks in scalar-tensor theories
- Unifying static analysis of gravitational structures with a scale-dependent scalar field gravity as an alternative to dark matter
- The Layzer-Irvine Equation for Scalar-Tensor Theories: A Test of Modified Gravity N-body Simulations
- N-body Simulations of Gravity
- Evolution of spherical domain walls in solitonic symmetron models
- asimulation: Domain formation and impact on observables in resolved cosmological simulations of the (a)symmetron
- Degeneracies between Modified Gravity and Baryonic Physics
- Testing modified gravity with globular clusters: the case of NGC 2419
- The Cosmological Supersymmetron
- Phenomenological footprints of Lambda varying gravity theories inspired from quantum gravity models in the multi-messenger era
- Dark Energy Simulations