D-BIonic Screening of Scalar Fields
arXiv:1403.6120 · doi:10.1103/PhysRevD.90.024001
Abstract
We study a new screening mechanism which is present in Dirac-Born-Infeld (DBI)-like theories. A scalar field with a DBI-like Lagrangian is minimally coupled to matter. In the vicinity of sufficiently dense sources, non-linearities in the scalar dominate and result in an approximately constant acceleration on a test particle, thereby suppressing the scalar force relative to gravity. Unlike generic P(X) theories, screening happens within the regime of validity of the effective field theory, thanks to the DBI symmetry. This symmetry also allows the removal of a constant field gradient, like in galileons. Not surprisingly, perturbations around the spherically-symmetry background propagate superluminally, but we argue for a chronology protection analogous to galileons. We derive constraints on the theory parameters from tests of gravity and discuss various extensions.
4 pages. v2: Added exact 2-body static solution and revised discussion of blanket screening
References in corpus (8)
- Resummation of Massive Gravity
- Causality, Analyticity and an IR Obstruction to UV Completion
- Environmental Dependence of Masses and Coupling Constants
- DBI and the Galileon reunited
- Degravitation of the Cosmological Constant and Graviton Width
- Screening Modifications of Gravity through Disformally Coupled Fields
- Equivalence Principle Violation in Vainshtein Screened Two-Body Systems
- Towards a UV Completion for Chameleon Scalar Theories
Cited by in corpus (45)
- Beyond the Cosmological Standard Model
- Dynamical systems applied to cosmology: dark energy and modified gravity
- Modified Gravity N-body Code Comparison Project
- Chameleon Dark Energy and Atom Interferometry
- An Alternative to Particle Dark Matter
- The Novel Probes Project -- Tests of Gravity on Astrophysical Scales
- Riding on irrelevant operators
- A dynamical system analysis of hybrid metric-Palatini cosmologies
- Using Voids to Unscreen Modified Gravity
- Phenomenological consequences of superfluid dark matter with baryon-phonon coupling
- Shaken, not stirred: kinetic mixing in scalar-tensor theories of gravity
- Constraining symmetron fields with atom interferometry
- Cosmological constraints on dark energy in light of gravitational wave bounds
- Halo velocity profiles in screened modified gravity theories
- Cosmological phase space of generalized hybrid metric-Palatini theories of gravity
- The Shape Dependence of Vainshtein Screening
- Quantum Corrections in Galileons from Matter Loops
- Small-scale Nonlinear Dynamics of K-mouflage Theories
- Non-trivial gravitational waves and structure formation phenomenology from dark energy
- Disformal vectors and anisotropies on a warped brane
- Dark D-Brane Cosmology: from background evolution to cosmological perturbations
- Cuscuta-Galileon cosmology: Dynamics, gravitational "constant"s and the Hubble Constant
- Cosmic Tsunamis in Modified Gravity: Disruption of Screening Mechanisms from Scalar Waves
- How to Avoid a Swift Kick in the Chameleons
- Quantum simulation of dark energy candidates
- Reappraisal of the limit on the variation in implied by Oklo
- Influence functionals, decoherence and conformally coupled scalars
- A Positive Energy Theorem for P(X,phi) Theories
- Searching for Chameleon Dark Energy with Mechanical Systems
- Dark matter superfluid and DBI dark energy
- Weighted density fields as improved probes of modified gravity models
- Double screening
- Estimates of cluster masses in screened modified gravity
- Anti-screening of the Galileon force around a disk center hole
- Cosmological Dynamics of D-BIonic and DBI Scalar Field and Coincidence Problem of Dark Energy
- Two-body problem in theories with kinetic screening
- Vainshtein in the UV and a Wilsonian analysis of derivatively coupled scalars
- Cosmological singularities in non-canonical models of dark energy
- Cosmological Dynamics and Double Screening of DBI Galileon Gravity
- Dynamical Chameleon Neutron Stars: stability, radial oscillations and scalar radiation in spherical symmetry
- K-nonizing
- Solar System and Atomic Clock Bounds on Locally Coupled Swampland Scalars
- Kinetically-driven ekpyrosis
- Positivity vs. Lorentz-violation: an explicit example
- Future Dark Energy Constraints from Atomic Clocks