Scalar-Tensor-Vector Gravity Theory

Abstract

A covariant scalar-tensor-vector gravity theory is developed which allows the gravitational constant $G$, a vector field coupling $\omega$ and the vector field mass $\mu$ to vary with space and time. The equations of motion for a test particle lead to a modified gravitational acceleration law that can fit galaxy rotation curves and cluster data without non-baryonic dark matter. The theory is consistent with solar system observational tests. The linear evolutions of the metric, vector field and scalar field perturbations and their consequences for the observations of the cosmic microwave background are investigated.

20 pages, Latex file, no figures. Revised version. Section on cosmology added. References added. Typos corrected

References in corpus (3)

• Galaxy Rotation Curves Without Non-Baryonic Dark Matter
• Large Scale Structure in Bekenstein's theory of relativistic Modified Newtonian Dynamics
• Did Boomerang hit MOND?

Cited by in corpus (346)

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• MOND as a regime of quantum gravity
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• Circular Motion and Energy Extraction in a Rotating Black Hole
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• Testing Dark Matter and Modifications to Gravity using Local Milky Way Observables
• Study of energy extraction and epicyclic frequencies in Kerr-MOG~(Modified Gravity) black hole
• The Star Formation History and Dynamics of the Ultra-diffuse Galaxy Dragonfly 44 in MOND and MOG
• CFHTLenS: Weak lensing constraints on the ellipticity of galaxy-scale matter haloes and the galaxy-halo misalignment
• Cooling process of brown dwarfs in Palatini f(R) gravity
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• Charged $AdS$ Black Holes in $4D$ Einstein--Gauss--Bonnet Massive Gravity
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• Analyzing the Influence of Geometrical Deformation on Photon Sphere and Shadow Radius: A New Analytical Approach -- Spherically Symmetric Spacetimes
• On the stability of a galactic disk in modified gravity
• Testing general relativity with compact-body orbits: A modified Einstein-Infeld-Hoffmann framework
• Confronting MOND and TeVeS with strong gravitational lensing over galactic scales: an extended survey
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• The Train Wreck Cluster Abell 520 and the Bullet Cluster 1E0657-558 in a Generalized Theory of Gravitation
• Merger rate of charged black holes from the two-body dynamical capture
• Strong lensing probability in TeVeS theory
• Harvesting energy driven by Comisso-Asenjo process from Kerr-MOG black holes
• On the universality of MOG weak field approximation at galaxy cluster scale
• Quantum Field Theory in a Multi-Metric Background
• Periodic orbits and their gravitational wave radiations around the Schwarzschild-MOG black hole
• Black hole accretion in scalar-tensor-vector gravity
• How Zwicky already ruled out modified gravity theories without dark matter
• Modified gravity and the origin of inertia
• Black hole solution and thermal properties in $4D$ AdS Gauss-Bonnet massive gravity
• Is the Universe Simpler than LCDM?
• Mass-Temperature relation in $\Lambda$CDM and modified gravity
• Constraining Energy-Momentum-Squared Gravity by binary pulsar observations
• Overspinning Kerr-MOG black holes by test fields and the third law of black hole dynamics
• Extended galactic rotational velocity profiles in $f(R)$ gravity background
• Renormalization Group Running of Newton's G: The Static Isotropic Case
• Large scale distribution of total mass versus luminous matter from Baryon Acoustic Oscillations: First search in the SDSS-III BOSS Data Release 10
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• Dark Matter in Cosmology
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• Dynamical ambiguities in models with spontaneous Lorentz violation
• Exact cosmological solutions for MOG
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• Constraint on the mass of fuzzy dark matter from the rotation curve of the Milky Way
• Testing modified gravity with dwarf spheroidal galaxies
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• Hawking-Like Radiation as Tunneling from a Cosmological Black Hole in Modified Gravity: Semiclassical Approximation and Beyond
• Perturbations of Keplerian Orbits in Stationary Spherically Symmetric Spacetimes
• Testing space-time geometries and theories of gravity at the Galactic Center with pulsar's time delay
• Constraining MOdified Gravity with the S2 Star
• Quasinormal Modes of the Generalized Ayón-Beato-Garc\'ıa Scalar-Tensor-Vector Gravity Black Hole in the Scalar-Tensor-Vector Gravity
• Comparison of light-time formulations in the post-Newtonian framework for the BepiColombo MORE experiment
• A thin disk in higher dimensional space-time and dark matter interpretation
• Maximum Force for Black Holes and Buchdahl Stars
• How Close Dark Matter Halos and MOND Are to Each Other: Three-Dimensional Tests Based on Gaia DR2
• Gravitational Theory of Cosmology, Galaxies and Galaxy Clusters
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• Does Planck mass run on the cosmological horizon scale?
• Stringy Models of Modified Gravity: Space-time defects and Structure Formation
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• Blandford-Znajek jets in MOdified Gravity
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• Lensing Effects in Retarded Gravity
• Effects of Higher Order Retarded Gravity
• Constraint on dark matter central density in the Eddington inspired Born-Infeld (EiBI) gravity with input from Weyl gravity
• Quasinormal-modes of the Kerr-Newman black hole: GW150914 and fundamental physics implications
• Phenomenology of wavelike vector dark matter nonminimally coupled to gravity
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• Will-Nordtvedt PPN formalism applied to renormalization group extensions of general relativity
• Dark matter perturbations and viscosity: a causal approach
• Acceleration Relations in the Milky Way as Differentiators of Modified Gravity Theories
• Dynamical system approach to scalar-vector-tensor cosmology
• Scalar-tensor black holes in an expanding universe
• Giant low-surface-brightness dwarf galaxy as a test bench for MOdified Gravity
• Singular Hamiltonians in models with spontaneous Lorentz symmetry breaking
• Does modified gravity predict fast stellar bars in spiral galaxies?
• Probing the H0 Tension with Holographic Dark Energy in Unimodular Gravity: Insights from DESI DR2
• DHOST gravity in Ultra-diffuse galaxies -- Part II: NGC 1052-DF4 and Dragonfly 44
• Dark Energy as a Critical Period in Binary Motion: Bounds from Multi-scale Binaries
• Ultra faint dwarf galaxies: an arena for testing dark matter versus modified gravity
• The GMRT archive atomic gas survey -- II. Mass modelling and dark matter halo properties across late-type spirals
• Enigmatic Velocity Dispersions of Ultra-Diffuse Galaxies in Light of Modified Gravity Theories and Radial Acceleration Relation
• Hamiltonian Formalism for dynamics of particles in MOG
• Stellar Bar evolution in the absence of dark matter halo
• Exploring the presence of a fifth force at the Galactic Center
• Shadow Cast by the Kerr MOG Black Hole under the Influence of Plasma and Constraints from EHT Observations
• On the rotation curves for axially symmetric disk solutions of the Vlasov-Poisson system
• Testing the Cubic Galileon Gravity model by the Milky Way rotation curve and SPARC data
• Polarization modes of gravitational waves in general Einstein-vector theory
• MONDified Gravity
• Putting Yukawa-like Modified Gravity (MOG) on the test in the Solar System
• Testing two alternatives theories to dark matter with the Milky Way dynamics
• Scalar-tensor-vector-gravity and NGC-1277
• Moffat's Modified Gravity tested on X-COP galaxy clusters
• Radially anisotropic systems with $r^{-\alpha }$ forces. II: radial-orbit instability
• Dark energy density predicted and explained
• The γ parameter in Brans-Dicke-like (light-)Scalar-Tensor theory with a universal scalar/matter coupling
• Effects of coupling constants on chaos of charged particles in the $Einstein-\AE$ ther theory
• Astrophysical and electromagnetic emissivity properties of black holes surrounded by a quintessence type exotic fluid in the Scalar-Vector-Tensor Modified Gravity
• Constraints and degrees of freedom in Lorentz-violating field theories
• Gravitational analog of the canonical acoustic black hole in Einstein-scalar-Gauss-Bonnet theory
• External Field Effect in Gravity
• Distinguishing Black Hole and Naked Singularity in MOG via Inertial Frame Dragging Effect
• Mass Modeling and Kinematics of Galaxy Clusters in Modified Gravity
• Exact cosmological black hole solutions in Scalar Tensor Vector Gravity
• Bondi Accretion in the Spherically Symmetric Johannsen-Psaltis Spacetime
• Off-shell Dark Matter: A Cosmological relic of Quantum Gravity
• Macroscopic theory of dark sector
• On the gravitational stability of the Maclaurin disk
• Structure of the equivalent Newtonian systems in MOND N-body simulations. Density profiles and the core-cusp problem
• Probing Yukawian Gravitational Potential by Numerical Simulations. II. Elliptical Galaxies
• Type I shell galaxies as a test of gravity models
• Modified Gravity (MOG) and its test on galaxy clusters
• Galaxy rotation curves and preferred reference frame effects
• Thermodynamics of Non-Commutative Scalar-Tensor-Vector Gravity Black holes
• Mass decomposition of SLACS lens galaxies in Weyl conformal gravity
• A Modified Dynamical Model of Cosmology I. Theory
• An f(R) model for dark matter: rotation curves and gravitational lensing
• Spiral structure of the galactic disk and its influence on the rotational velocity curve
• Variation of fundamental constants and white dwarfs
• The distinguishing factor for gravity models: stellar population synthesis
• Magnetic black holes in 4$D$ Einstein--Gauss--Bonnet massive gravity coupled to nonlinear electrodynamics
• Signatures of modified gravity from the gravitational Aharonov-Bohm effect
• Dark Coincidences: Small-Scale Solutions with Refracted Gravity and MOND
• Radial Acceleration and Tully-Fisher Relations in Conformal Gravity
• Upper limits on the temperature of inspiraling astrophysical black holes
• Dark Universe inspired by the Kaluza-Klein gravity and impact on Primordial Gravitational Waves
• Formation and Growth of the First Supermassive Black Holes in MOG
• Big Bang Nucleosynthesis constraints on the Energy-Momentum Squared Gravity: The ${\mathbb{T}}^2$ model
• Constraints on fourth order gravity from binary pulsar and gravitational waves
• On the well-posed variational principle in degenerate point particle systems using embeddings of the symplectic manifold
• Newtonian Fractional-Dimension Gravity and Galaxies without Dark Matter
• Local Stability of Galactic Discs in Modified Dynamics
• A Black Hole inside Dark Matter and the Rotation Curves of Galaxies
• The $\kappa$-model, a minimal model alternative to dark matter. Application to the galactic rotation problem
• Accretion Process as a Probe of Extra Dimensions in MOG Compact Object Spacetimes
• D-dimensional black holes in extended Gauss-Bonnet gravity
• Observational constraints on models of the Universe with time variable Gravitational and Cosmological constants along MOG
• Observational constraints on the Kerr and its several single-parameter modified spacetimes using quasi-periodic oscillation data
• Weyl-Invariant Gravity and the Nature of Dark Matter
• Cosmology with Higher-Derivative Gravities
• Confronting models on cosmic ray interactions with particle physics at LHC energies
• Dark matter effect attributed to the inherent structure of cosmic space
• Limiting the Yukawa Gravity through the Black Hole Shadows of Sgr A* and M87*
• Distinguishing Signature of Kerr-MOG Black Hole and Superspinar via Lense-Thirring Precession
• Toward Gravitational Lensing in Modified Theories of Gravity
• Shadow geometry of Kerr MOG naked singularity and analysis of accretion disk luminosity
• Constraints on a fifth force from the stellar orbits around the central supermassive black hole of the Milky Way
• Constraining black-hole horizon effects by LIGO-Virgo detections of inspiralling binary black holes
• Implications of the Milky Way Declining Rotation Curve
• Dark matter and alternative recipes for the missing mass
• The Phase Transition of $4D$ Yang-Mills Charged GB AdS Black Hole with Cloud of Strings
• GravitoMagnetic Force in Modified Newtonian Dynamics
• MOG without anomaly
• Spacetime expansion in the presence of a background velocity field
• Complex Riemannian spacetime and singularity-free black holes and cosmology
• Terrestrial Sagnac delay in scalar-tensor-vector-gravity
• Dynamics of Dwarf Galaxies in Scalar-Tensor-Vector-Gravity
• Many body gravity and the bullet cluster
• The $\kappa$-model under test of the SPARC database
• Post-Newtonian properties of EMRI with Power Law Potential
• Exact Solutions with Asymptotically Flat Galactic Rotation Curves
• Remove point-mass concept-remove singularities from GR
• Relativistic Thermal Emission from Accretion Disks in Kerr-MOG Spacetimes
• The modified Newtonian dynamics with an extra anti-dissipation term can yield the MOND model
• Satellite galaxy velocity dispersions in the SDSS and modified gravity models
• Non-Gaussian Signatures of a Thermal Big Bang
• DHOST gravity in Ultra-diffuse galaxies -- Part I: the case of NGC1052-DF2
• Gravitomagnetism in Modified theory of Gravity
• Distinct radial acceleration relations of galaxies and galaxy clusters supports hyperconical modified gravity
• A spherically symmetric gravitational solution of nearly conformally flat metric~measure~space
• Non-Newtonian gravity in finite nuclei
• Investigating the effects of gravitational lensing by Hu-Sawicki $\mathbf{f}(\mathbf{R})$ gravity black holes
• On quasinormal frequencies of black hole perturbations with an external source
• Zero Mass limit of Kerr-MOG Black Hole Equals Wormhole
• Phase transition in Modified Newtonian Dynamics (MONDian) self-gravitating systems
• Scattering of quantum fields by a MOG Black Hole
• New effective theories of gravitation and their phenomenological consequences