A new relativistic theory for Modified Newtonian Dynamics
arXiv:2007.00082 · doi:10.1103/PhysRevLett.127.161302
Abstract
We propose a relativistic gravitational theory leading to modified Newtonian dynamics, a paradigm that explains the observed universal galactic acceleration scale and related phenomenology. We discuss phenomenological requirements leading to its construction and demonstrate its agreement with the observed cosmic microwave background and matter power spectra on linear cosmological scales. We show that its action expanded to second order is free of ghost instabilities and discuss its possible embedding in a more fundamental theory.
arXiv comment7 pages, 2 figures. We separated the CMB and MPS into two figures, displaying for each one the residuals compared to LCDM. We added more references, additional discussion and details, resulting also to structural rearrangements and shortening of text in accordance with referee comments and to fit within PRL page limits. Content matches published version
References in corpus (98)
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- Modified Gravity and Cosmology
- The Confrontation between General Relativity and Experiment
- An Ordinary Short Gamma-Ray Burst with Extraordinary Implications: Fermi-GBM Detection of GRB 170817A
- Relativistic gravitation theory for the MOND paradigm
- Gravity with a dynamical preferred frame
- INTEGRAL Detection of the First Prompt Gamma-Ray Signal Coincident with the Gravitational Wave Event GW170817
- Modified Newtonian Dynamics (MOND): Observational Phenomenology and Relativistic Extensions
- Ghost Condensation and a Consistent Infrared Modification of Gravity
- The Baryonic Tully-Fisher Relation
- Modified Newtonian Dynamics as an Alternative to Dark Matter
- The Radial Acceleration Relation in Rotationally Supported Galaxies
- Emergent Gravity and the Dark Universe
- Purely kinetic k-essence as unified dark matter
- The Baryonic Tully-Fisher Relation of Galaxies with Extended Rotation Curves and the Stellar Mass of Rotating Galaxies
- Cosmological Constraints from the Clustering of the Sloan Digital Sky Survey DR7 Luminous Red Galaxies
- Mimetic Dark Matter
- Modified Newtonian Dynamics in the Milky Way
- Modifying gravity with the Aether: an alternative to Dark Matter
- Cosmological Tests of Gravity
- Large Scale Structure in Bekenstein's theory of relativistic Modified Newtonian Dynamics
- Theory of Dark Matter Superfluidity
- Mimetic gravity: a review of recent developments and applications to cosmology and astrophysics
- Bimetric MOND gravity
- New Test of the Gravitational Law at Separations down to 52 m
- Dark matter heats up in dwarf galaxies
- Clusters of galaxies with modified Newtonian dynamics (MOND)
- The published extended rotation curves of spiral galaxies: Confrontation with Modified Dynamics
- Dark Matter from R^2-gravity
- The baryonic Tully-Fisher relation for different velocity definitions and implications for galaxy angular momentum
- The Modified Dynamics as a Vacuum Effect
- GW170817 Falsifies Dark Matter Emulators
- Linking Tests of Gravity On All Scales: from the Strong-Field Regime to Cosmology
- Resolving the virial discrepancy in clusters of galaxies with modified Newtonian dynamics
- A stratified framework for scalar-tensor theories of Modified Dynamics
- Hydrostatic mass profiles in X-COP galaxy clusters
- A tensor-vector-scalar framework for modified dynamics and cosmic dark matter
- Tidal dwarf galaxies as a test of fundamental physics
- Can Cosmic Structure form without Dark Matter?
- New constraints on MOND from galaxy clusters
- Improving relativistic MOND with Galileon k-mouflage
- Dwarf Spheroidals in MOND
- The MOND limit from space-time scale invariance
- Gravitational waves in Einstein-æther and generalized TeVeS theory after GW170817
- Gravitational polarization and the phenomenology of MOND
- Dark Matter Superfluidity and Galactic Dynamics
- The Vector-Tensor nature of Bekenstein's relativistic theory of Modified Gravity
- Mimicking dark matter and dark energy in a mimetic model compatible with GW170817
- An Alternative to Particle Dark Matter
- Vector field models of modified gravity and the dark sector
- Combined Solar System and rotation curve constraints on MOND
- MOND habitats within the solar system
- Nonlocal metric formulations of MOND with sufficient lensing
- Dipolar Dark Matter and Dark Energy
- Dynamics of Gravity in a Higgs Phase
- A Covariant Version of Verlinde's Emergent Gravity
- MOND and the seven dwarfs
- The Dark Matter equation of state through cosmic history
- MOND simulation suggests the origin of some peculiarities in the Local Group
- Spontaneous Lorentz Breaking at High Energies
- The Radial Acceleration Relation in CLASH Galaxy Clusters
- Non-linear extension of non-metricity scalar for MOND
- A general class of gravitational theories as alternatives to dark matter where the speed of gravity always equals the speed of light
- A comparison of Einstein-Boltzmann solvers for testing General Relativity
- The cosmological behavior of Bekenstein's modified theory of gravity
- Dark matter as a Bose--Einstein Condensate: the relativistic non-minimally coupled case
- Testing Modified Gravity with Wide Binaries in GAIA DR2
- Dark Matter via Massive (bi-)Gravity
- Symmetron Scalar Fields: Modified Gravity, Dark Matter or Both?
- Jeans' Ghost
- Non-linear conformally invariant generalization of the Poisson equation to D>2 dimensions
- Cosmological perturbations in mimetic Horndeski gravity
- Rapid Calculation of Theoretical CMB Angular Power Spectra
- Dark Matter properties through cosmic history
- Jacob Bekenstein's Universes: From Black Holes to Modified Theories of Gravity
- Noncovariance at low accelerations as a route to MOND
- Unification of Dark Matter - Dark Energy in Generalized Galileon Theories
- The global stability of M33 in MOND
- Gravitational waves in Einstein-Æther theory and generalized TeVeS theory after GW170817
- The case for testing MOND using LISA Pathfinder
- Implications for dwarf spheroidal mass content from interloper removal
- What is the price of abandoning dark matter? Cosmological constraints on alternative gravity theories
- Nonlocal Metric Realizations of MOND
- Mimicking dark matter in Horndeski gravity
- Verlinde's emergent gravity versus MOND and the case of dwarf spheroidals
- Modified gravity, Dark Energy and MOND
- Entropic gravity, minimum temperature, and modified Newtonian dynamics
- A first attempt to differentiate between modified gravity and modified inertia with galaxy rotation curves
- The prediction of rotation curves in gas-dominated dwarf galaxies with modified dynamics
- Inconsistencies in Verlinde's emergent gravity
- A note on a covariant version of Verlinde's emergent gravity
- Testing the tensor-vector-scalar Theory with the latest cosmological observations
- Horndeski dark matter and beyond
- The Music of the Aetherwave - B-mode Polarization in Einstein-Aether Theory
- Cosmology of the Galileon extension of Bekenstein's theory of relativistic Modified Newtonian Dynamics
- Structure Formation in Nonlocal MOND
- MOND as the weak-field limit of an extended metric theory of gravity
- Constraining MOND Using the Vertical Motion of Stars in the Solar Neighborhood
Cited by in corpus (119)
- From galactic bars to the Hubble tension: weighing up the astrophysical evidence for Milgromian gravity
- A massive stellar bulge in a regularly rotating galaxy 1.2 billion years after the Big Bang
- The KBC void and Hubble tension contradict CDM on a Gpc scale Milgromian dynamics as a possible solution
- The distribution and morphologies of Fornax Cluster dwarf galaxies suggest they lack dark matter
- Parametric and nonparametric methods hint dark energy evolution
- Breakdown of the Newton-Einstein Standard Gravity at Low Acceleration in Internal Dynamics of Wide Binary Stars
- Strong constraints on the gravitational law from DR3 wide binaries
- Testing the Strong Equivalence Principle. II. Relating the External Field Effect in Galaxy Rotation Curves to the Large-Scale Structure of the Universe
- The gravitational field of X-COP galaxy clusters
- Primordial black holes as dark matter: Interferometric tests of phase transition origin
- Cold gas disks in main-sequence galaxies at cosmic noon: Low turbulence, flat rotation curves, and disk-halo degeneracy
- Testing Theories of Gravity with Planetary Ephemerides
- Gas dynamics in dwarf galaxies as testbeds for dark matter and galaxy evolution
- Internal kinematics of GAIA DR3 wide binaries: anomalous behaviour in the low acceleration regime
- Testing Super-Heavy Dark Matter from Primordial Black Holes with Gravitational Waves
- 3D hydrodynamic simulations for the formation of the Local Group satellite planes
- Multifield Ultralight Dark Matter
- Barred spiral galaxies in modified gravity theories
- Models of modified-inertia formulation of MOND
- Numerical Solutions of the External Field Effect on the Radial Acceleration in Disk Galaxies
- Probing the radial acceleration relation and the strong equivalence principle with the Coma cluster ultra-diffuse galaxies
- Alternative ideas in cosmology
- The distribution of galaxy rotation in JWST Advanced Deep Extragalactic Survey
- Aether scalar tensor theory: Linear stability on Minkowski space
- The Milky Way's rotation curve with superfluid dark matter
- Radial acceleration relation of galaxies with joint kinematic and weak-lensing data
- On the tension between the Radial Acceleration Relation and Solar System quadrupole in modified gravity MOND
- The phantom dark matter halos of the Local Volume in the context of modified Newtonian dynamics
- Methodological Reflections on the MOND/Dark Matter Debate
- On the functional form of the radial acceleration relation
- Newtonian Fractional-Dimension Gravity and MOND
- Tripotential MOND theories
- Hydrodynamical structure formation in Milgromian cosmology
- Aether scalar tensor theory confronted with weak lensing data at small accelerations
- Dynamical system analysis of cosmological evolution in the Aether scalar tensor theory
- Generalizations of Quasilinear MOND (QUMOND)
- Supercomputers against strong coupling in gravity with curvature and torsion
- Dark Matter Realism
- Relativistic Khronon Theory in agreement with Modified Newtonian Dynamics and Large-Scale Cosmology
- Milky Way and M31 rotation curves: CDM vs. MOND
- Dressed black holes in the new tensor-vector-scalar theory
- Cosmological Dynamics of Relativistic MOND
- Constraining Palatini-Horndeski theory with gravitational waves after GW170817
- Time evolution of the local gravitational parameters and gravitational wave polarizations in a relativistic MOND theory
- Cherenkov radiation from stars constrains hybrid MOND dark matter models
- Acausality in Superfluid Dark Matter and MOND-like Theories
- A Distinct Radial Acceleration Relation across Brightest Cluster Galaxies and Galaxy Clusters
- Theoretically motivated dark electromagnetism as the origin of relativistic MOND
- Testing Modified Gravity Theories with Numerical Solutions of the External Field Effect in Rotationally Supported Galaxies
- Discord in Concordance Cosmology and Anomalously Massive Early Galaxies
- An empirical consistent redshift bias: A possible direct reproducible observation of Zwicky's TL theory
- Aether scalar tensor theory: Hamiltonian Formalism
- Covariant formulation of refracted gravity
- Hamiltonian Formalism for dynamics of particles in MOG
- The dynamics of three nearby E0 galaxies in refracted gravity
- Galaxy rotation curve in hyperconical universes: a natural relativistic MOND
- Superfluid dark matter in tension with weak gravitational lensing data
- MONDified Gravity
- A new scale in the quasi-static limit of Aether Scalar Tensor Theory
- The prediction of using LHAASO's cosmic-ray electron measurements to constrain decaying heavy dark matter
- Causal Modifications of Gravity and Their Observational Bounds
- Probing modified Newtonian dynamics with hypervelocity stars
- The Scale Invariant Vacuum Paradigm: main results and current progress
- The formation of compact massive relic galaxies in MOND
- Dark Energy from the Fifth Dimension
- Dipolar dark matter simulations on galaxy scales with the RAMSES code
- Scrutinizing coupled vector dark energy in light of data
- The Scale Invariant Vacuum Paradigm: Main Results and Current Progress Review (Part II)
- Broader view of bimetric MOND
- Dwarf galaxies with central cores in modified Newtonian dynamics (MOND) gravity
- A new constant behind the rotational velocity of galaxies
- Stealth black holes in Aether Scalar Tensor theory
- Newtonian Fractional-Dimension Gravity and the External Field Effect
- Testing CCC+TL Cosmology with Galaxy Rotation Curves
- Big Bang Nucleosynthesis constraints on the Energy-Momentum Squared Gravity: The model
- Newtonian Fractional-Dimension Gravity and Galaxies without Dark Matter
- Why did the dark matter hypothesis supersede modified gravity in the 1980s?
- Dark Coincidences: Small-Scale Solutions with Refracted Gravity and MOND
- Buchdahl bound, photon ring, ISCO and radial acceleration in Einstein-æther theory
- Effect of generic dark matter halo on transonic accretion onto galactic black holes
- Cosmological implications of the Gaia Milky Way declining rotation curve
- On the global Gaussian bending measure and its applications in stationary spacetimes
- Sudden cosmological singularities in Aether scalar-tensor theories
- A simple direct empirical observation of systematic bias of the redshift as a distance indicator
- Consistent cosmological structure formation on all scales in relativistic extensions of MOND
- The radial acceleration relation at the EDGE of galaxy formation: testing its universality in low-mass dwarf galaxies
- Analytic Solutions of Scalar Field Cosmology, Mathematical Structures for Early Inflation and Late Time Accelerated Expansion
- The isolated elliptical galaxy NGC 5812 -- MOND or Dark Matter?
- Globular cluster orbital decay in dwarf galaxies with MOND and CDM: Impact of supernova feedback
- Mimetic Tensor-Vector-Scalar Cosmology: Incorporating Dark Matter, Dark Energy and Stiff Matter
- Revisiting Flat Rotation Curves in Chern-Simons Modified Gravity
- Asymmetry in galaxy spin directions: a fully reproducible experiment using HSC data
- PySCo: A fast Particle-Mesh -body code for modified gravity simulations in Python
- Formation of collisional ring galaxies in Milgromian dynamics
- The Atacama Cosmology Telescope: A Test of the Gravitational Force Law on Cosmological Scales Using the Kinematic Sunyaev-Zeldovich Effect
- Dark matter fluid constraints from galaxy rotation curves
- Alleviating the Hubble tension with Torsion Condensation (TorC)
- Probing Modified Gravity with Entanglement of Microspheres
- Testing QUMOND theory with Galactic globular clusters in a weak external field
- Disk galaxies and their dark halos as self-organized patterns
- Cosmic backgrounds from the radio to the far-infrared: recent results and perspectives from cosmological and astrophysical surveys
- MOND via Matrix Gravity
- Multidimensional representation of semantic relations between physical theories, fundamental constants and units of measurement with formal concept analysis
- The -model under test of the SPARC database
- Measuring Mass of Gas in Central Galaxies using weak lensing and satellite kinematics in MOND
- Pattern dark matter and galaxy scaling relations
- Fast particle-mesh code for Milgromian dynamics
- Refracted Gravity Solutions from Small to Large Scales
- Bimetric MOND as a framework for variable- theories -- local systems and cosmology
- An effective fluid description of scalar-vector-tensor theories under the sub-horizon and quasi-static approximations
- Modification of Newtonian Gravity: Implications for Hot Gas in Clusters and Galactic Angular Momentum
- Testing MOND using the dynamics of nearby stellar streams
- A test of MOND and Emergent Gravity with SMACS J0723.3-7327 using eROSITA observations
- The radial metric function does not identify null surfaces
- Examining Baryonic Faber-Jackson Relation in Galaxy Groups
- Distinct radial acceleration relations of galaxies and galaxy clusters supports hyperconical modified gravity
- Are disks of satellites comprised of tidal dwarf galaxies?
- Improved constraints on modified Newtonian gravity from Cassini radio tracking data
- Dwarf galaxies in non-local gravity