MOND vs. dark matter in light of historical parallels
arXiv:1910.04368 · doi:10.1016/j.shpsb.2020.02.004
Abstract
MOND is a paradigm that contends to account for the mass discrepancies in the Universe without invoking `dark' components, such as `dark matter' and `dark energy'. It does so by supplanting Newtonian dynamics and General Relativity, departing from them at very low accelerations. Having in mind readers who are historians and philosophers of science, as well as physicists and astronomers, I describe in this review the main aspects of MOND -- its statement, its basic tenets, its main predictions, and the tests of these predictions -- contrasting it with the dark-matter paradigm. I then discuss possible wider ramifications of MOND, for example the potential significance of the MOND constant, , with possible implications for the roots of MOND in cosmology. Along the way I point to parallels with several historical instances of nascent paradigms. In particular, with the emergence of the Copernican world picture, that of quantum physics, and that of relativity, as regards their initial advent, their development, their schematic structure, and their ramifications. For example, the interplay between theories and their corollary laws, and the centrality of a new constant with converging values as deduced from seemingly unrelated manifestations of these laws. I demonstrate how MOND has already unearthed a number of unsuspected laws of galactic dynamics (to which, indeed, is central) predicting them a priori, and leading to their subsequent verification. I parallel the struggle of the new with the old paradigms, and the appearance of hybrid paradigms at such times of struggle. I also try to identify in the history of those established paradigms a stage that can be likened to that of MOND today.
arXiv comment29 pages, 19 figures, Based on a talk at the conference `Dark Matter & Modified Gravity', Aachen, February 2019 Added a discussion of gravitational waves. Added references
References in corpus (109)
- Modified Gravity and Cosmology
- A direct empirical proof of the existence of dark matter
- Small-Scale Challenges to the CDM Paradigm
- Relativistic gravitation theory for the MOND paradigm
- Dark Matter Candidates from Particle Physics and Methods of Detection
- A History of Dark Matter
- Modified Newtonian Dynamics (MOND): Observational Phenomenology and Relativistic Extensions
- Modified Newtonian Dynamics as an Alternative to Dark Matter
- The Radial Acceleration Relation in Rotationally Supported Galaxies
- Emergent Gravity and the Dark Universe
- A New Era in the Quest for Dark Matter
- The Baryonic Tully-Fisher Relation of Gas Rich Galaxies as a Test of LCDM and MOND
- A constant dark matter halo surface density in galaxies
- Modifying gravity with the Aether: an alternative to Dark Matter
- Small scale problems of the CDM model: a short review
- A dominant population of optically invisible massive galaxies in the early Universe
- Dynamics with a non-standard inertia-acceleration relation: an alternative to dark matter
- Bimetric MOND gravity
- Dark matter heats up in dwarf galaxies
- The published extended rotation curves of spiral galaxies: Confrontation with Modified Dynamics
- A Novel Test of the Modified Newtonian Dynamics with Gas Rich Galaxies
- The Modified Dynamics as a Vacuum Effect
- Galaxy groups and clouds in the Local (z~0.01) universe
- Galaxies as simple dynamical systems: observational data disfavor dark matter and stochastic star formation
- Clues from nearby galaxies to a better theory of cosmic evolution
- The Tensor-Vector-Scalar theory and its cosmology
- Resolving the virial discrepancy in clusters of galaxies with modified Newtonian dynamics
- A stratified framework for scalar-tensor theories of Modified Dynamics
- Testing Modified Newtonian Dynamics with Low Surface Brightness Galaxies --Rotation curve fits-
- Fitting the radial acceleration relation to individual SPARC galaxies
- Hydrostatic mass profiles in X-COP galaxy clusters
- Local Group Dwarf Spheroidals: Correlated Deviations from the Baryonic Tully-Fisher Relation
- THINGS about MOND
- MOND theory
- A Tale of Two Paradigms: the Mutual Incommensurability of LCDM and MOND
- The Impossibly Early Galaxy Problem
- The Relation between Stellar and Dynamical Surface Densities in the Central Regions of Disk Galaxies
- MOND laws of galactic dynamics
- Andromeda Dwarfs in Light of MOND. II. Testing Prior Predictions
- The MOND limit from space-time scale invariance
- Dwarf Spheroidals in MOND
- Dark Matter Superfluidity and Galactic Dynamics
- Combined Solar System and rotation curve constraints on MOND
- First test of Verlinde's theory of Emergent Gravity using Weak Gravitational Lensing measurements
- Cosmology and Convention
- Λ CDM is Consistent with SPARC Radial Acceleration Relation
- Stability of disk galaxies in the modified dynamics
- Cold Dark Matter with MOND Scaling
- Dipolar Dark Matter and Dark Energy
- Andromeda Dwarfs in Light of MOND
- The high mass end of the Tully-Fisher relation
- Galactic rotation curves, the baryon-to-dark-halo-mass relation and space-time scale invariance
- How Cold Dark Matter Theory Explains Milgrom's Law
- A Census of Baryons and Dark Matter in an Isolated, Milky Way-sized Elliptical Galaxy
- Dynamical friction in modified Newtonian dynamics
- Testing Gravity with wide binary stars like Centauri
- Dark matter halo properties from galaxy-galaxy lensing
- Universal MOND relation between the baryonic and `dynamical' central surface densities of disc galaxies
- The central surface density of "dark halos" predicted by MOND
- Testing the MOND Paradigm of Modified Dynamics with Galaxy-Galaxy Gravitational Lensing
- A general class of gravitational theories as alternatives to dark matter where the speed of gravity always equals the speed of light
- The distribution of mass components in simulated disc galaxies
- Testing MOND Over a Wide Acceleration Range in X-Ray Ellipticals
- The Clustering of High-Redshift (2.9 z 5.1) Quasars in SDSS Stripe 82
- Perseus I and the NGC 3109 association in the context of the Local Group dwarf galaxy structures
- A new formulation of the external field effect in MOND and numerical simulations of ultra-diffuse dwarf galaxies application to NGC 1052-DF2 and NGC 1052-DF4
- Cosmological fluctuation growth in bimetric MOND
- Another Path for the Emergence of Modified Galactic Dynamics from Dark Matter Superfluidity
- An accurate measurement of the baryonic Tully-Fisher relation with heavily gas-dominated ALFALFA galaxies
- Nordstrom's scalar theory of gravity and the equivalence principle
- MOND Prediction for the Velocity Dispersion of the `Feeble Giant' Crater II
- Marriage à-la-MOND: Baryonic dark matter in galaxy clusters and the cooling flow puzzle
- Evolution of spiral galaxies in modified gravity: II- Gas dynamics
- MOND predictions of "halo" phenomenology in disc galaxies
- The Third Law of Galactic Rotation
- The Extremely High Dark Matter Halo Concentration of the Relic Compact Elliptical Galaxy Mrk 1216
- Using dwarf satellite proper motions to determine their origin
- Modified gravity approach based on a preferred time foliation
- Three problems about multi-scale modelling in cosmology
- MOND in galaxy groups: a superior sample
- Does MOND follow from the CDM paradigm?
- The ELIXR Galaxy Survey. II: Baryons and Dark Matter in an Isolated Elliptical Galaxy
- Dipolar Particles in General Relativity
- The Radial Acceleration Relation in Disk Galaxies in the MassiveBlack-II Simulation
- Noncovariance at low accelerations as a route to MOND
- The modified dynamics (MOND) predicts an absolute maximum to the acceleration produced by `dark halos'
- Implications for dwarf spheroidal mass content from interloper removal
- Mass models from high-resolution HI data of the dwarf galaxy NGC 1560
- Challenging a Newtonian prediction through Gaia wide binaries
- The candidate cluster and protocluster catalog (CCPC) II: Spectroscopically identified structures spanning 2 < z < 6.6
- General virial theorem for modified-gravity MOND
- Hiding Lorentz Invariance Violation with MOND
- The prediction of rotation curves in gas-dominated dwarf galaxies with modified dynamics
- Debye entropic force and modified Newtonian dynamics
- The holographic screen at low temperatures
- MOND and the dark baryons
- Study of gravitational fields and globular cluster systems of early-type galaxies
- FRW cosmology in Milgrom's bimetric theory of gravity
- The road to MOND--a novel perspective
- Quantum particle statistics on the holographic screen leads to Modified Newtonian Dynamics (MOND)
- Directly testing gravity with Proxima Centauri
- Cosmology of the Galileon extension of Bekenstein's theory of relativistic Modified Newtonian Dynamics
- Halo Acceleration Relation
- An Uneven Vacuum Energy Fluid as , Dark Matter, MOND and Lens
- Predictions for the sky-averaged depth of the 21cm absorption signal at high redshift in cosmologies with and without non-baryonic cold dark matter
- Dark Energy, Paradigm Shifts, and the Role of Evidence
- Imprint of the galactic acceleration scale on globular cluster systems
- Milgrom Relation Models for Spiral Galaxies from Two-Dimensional Velocity Maps
- Globular Clusters as a Test for Gravity in the Weak Acceleration Regime
Cited by in corpus (31)
- From galactic bars to the Hubble tension: weighing up the astrophysical evidence for Milgromian gravity
- The KBC void and Hubble tension contradict CDM on a Gpc scale Milgromian dynamics as a possible solution
- Models of modified-inertia formulation of MOND
- Tripotential MOND theories
- Generalizations of Quasilinear MOND (QUMOND)
- Detecting the Figure Rotation of Dark Matter Halos with Tidal Streams
- Boltzmann hierarchies for self-interacting warm dark matter scenarios
- Deep-MOND polytropes
- Visions in Quantum Gravity
- Non-Newtonian mathematics instead of non-Newtonian physics: Dark matter and dark energy from a mismatch of arithmetics
- Mass-Velocity Dispersion Relation in MaNGA Brightest Cluster Galaxies
- MOND fiducial specific angular momentum of disc galaxies
- Emergent gravity fails to explain color-dependent galaxy-galaxy lensing signals from SDSS Dr7
- What if the universe expands linearly? A local general relativity to solve the "zero active mass" problem
- Dark matter as a gravitational effect in the embedding theory approach
- Central-surface-densities correlation in general MOND theories
- Broader view of bimetric MOND
- Self-Interacting Dark Matter in Cosmology: accurate numerical implementation and observational constraints
- Testing CCC+TL Cosmology with Galaxy Rotation Curves
- Why did the dark matter hypothesis supersede modified gravity in the 1980s?
- Weyl-Invariant Gravity and the Nature of Dark Matter
- Solar System, Astrophysics, and Cosmology from the Derivative Expansion
- Is MOND necessarily nonlinear?
- The -model under test of the SPARC database
- Comparison of HMG and flat rotation velocities inferred from galaxy-galaxy weak lensing
- Universal Basic Mass Density inside Dark Matter Halos
- Modified Newtonian dynamics and hadronic scales
- Examining Baryonic Faber-Jackson Relation in Galaxy Groups
- Hydrostatic equilibrium of X-ray gas in X-COP clusters with HMG
- Bimetric MOND as a framework for variable- theories -- local systems and cosmology
- Analysis of the equations of motion of fictitious matter in embedding theory