Enhanced Peculiar Velocities in Brane-Induced Gravity
arXiv:1004.2046 · doi:10.1103/PhysRevD.82.044032
Abstract
The mounting evidence for anomalously large peculiar velocities in our Universe presents a challenge for the LCDM paradigm. The recent estimates of the large scale bulk flow by Watkins et al. are inconsistent at the nearly 3 sigma level with LCDM predictions. Meanwhile, Lee and Komatsu have recently estimated that the occurrence of high-velocity merging systems such as the Bullet Cluster (1E0657-57) is unlikely at a 6.5-5.8 sigma level, with an estimated probability between 3.3x10^{-11} and 3.6x10^{-9} in LCDM cosmology. We show that these anomalies are alleviated in a broad class of infrared-modifed gravity theories, called brane-induced gravity, in which gravity becomes higher-dimensional at ultra large distances. These theories include additional scalar forces that enhance gravitational attraction and therefore speed up structure formation at late times and on sufficiently large scales. The peculiar velocities are enhanced by 24-34% compared to standard gravity, with the maximal enhancement nearly consistent at the 2 sigma level with bulk flow observations. The occurrence of the Bullet Cluster in these theories is 10^4 times more probable than in LCDM cosmology.
15 pages, 6 figures. v2: added references
References in corpus (32)
- A direct empirical proof of the existence of dark matter
- Covariant Galileon
- Generalized Galileons: All scalar models whose curved background extensions maintain second-order field equations and stress tensors
- A discriminating probe of gravity at cosmological scales
- Evading Equivalence Principle Violations, Cosmological and other Experimental Constraints in Scalar Field Theories with a Strong Coupling to Matter
- Confirmation of general relativity on large scales from weak lensing and galaxy velocities
- Galileon Cosmology
- Revealing the properties of dark matter in the merging cluster MACSJ0025.4-1222
- Testing cosmological structure formation using redshift-space distortions
- Degravitation of the Cosmological Constant and Graviton Width
- Observational Tests of Modified Gravity
- The speed of the `bullet' in the merging galaxy cluster 1E0657-56
- Cluster Constraints on f(R) Gravity
- Strongly Coupled Chameleon Fields: New Horizons in Scalar Field Theory
- DGP Specteroscopy
- Non-Local Modification of Gravity and the Cosmological Constant Problem
- Cascading DGP
- Dynamical Masses in Modified Gravity
- The Growth of Structure in Interacting Dark Energy Models
- Simulating the Bullet Cluster
- N-Body Simulations of DGP and Degravitation Theories
- A New Force in the Dark Sector?
- The Vainshtein mechanism in the Decoupling Limit of massive gravity
- The Cluster-Merger Shock in 1E 0657-56: Faster than the Speeding Bullet?
- Unveiling Chameleons in Tests of Gravitational Inverse-Square Law
- Spherical Collapse and Cluster Counts in Modified Gravity Models
- Large-Scale Structure in Brane-Induced Gravity I. Perturbation Theory
- Domain Walls As Probes Of Gravity
- Induced gravity on intersecting brane-worlds Part I: Maximally symmetric solutions
- Induced gravity on intersecting brane-worlds Part II: Cosmology
- Non Pauli-Fierz Massive Gravitons
- Density profiles and voids in modified gravity models
Cited by in corpus (24)
- Modified Gravity and Cosmology
- Beyond the Cosmological Standard Model
- Dark Energy vs. Modified Gravity
- Testing General Relativity in Cosmology
- Symmetron Cosmology
- Cosmology of the Galileon from Massive Gravity
- Cosmology in generalized Proca theories
- de Sitter Galileon
- Galilean-invariant scalar fields can strengthen gravitational lensing
- Validating estimates of the growth rate of structure with modified gravity simulations
- Galaxy Infall Kinematics as a Test of Modified Gravity
- Instabilities of Spherical Solutions with Multiple Galileons and SO(N) Symmetry
- Simulations of Galileon modified gravity: Clustering statistics in real and redshift space
- Can Coupled Dark Energy Speed Up the Bullet Cluster?
- Weak lensing by galaxy troughs with modified gravity
- Tests of Gravity with Galaxy Clusters
- One Thousand and One Clusters: Measuring the Bulk Flow with the Planck ESZ and X-Ray Selected Galaxy Cluster Catalogs
- Bulk flow of halos in ΛCDM simulation
- Measuring Bulk Flow of Galaxy Clusters using Kinematic Sunyaev-Zel'dovich effect: Prediction for Planck
- Testing model independent modified gravity with future large scale surveys
- The critical tension in the Cascading DGP model
- Degravitation Features in the Cascading Gravity Model
- Constraints on the normal branch of DGP gravity from SPT galaxy clusters with DES and HST weak-lensing mass calibration and from Planck PR4 CMB anisotropies
- Thin limit of the 6D Cascading DGP model