Are sterile neutrinos consistent with clusters, the CMB and MOND?

Abstract

If a single sterile neutrino exists such that $m_{{\nu }_s}\sim 11eV$, it can serendipitously solve all outstanding issues of the Modified Newtonian Dynamics. With it one can explain the dark matter of galaxy clusters without influencing individual galaxies, match the angular power spectrum of the cosmic microwave background and potentially fit the matter power spectrum. This model is flat with ${\Omega }_{{\nu }_s}\sim 0.23$ and the usual baryonic and dark energy components, thus the Universe has the same expansion history as the $\lcdm$ model and only differs at the galactic scale where the Modified Dynamics outperforms $\lcdm$ significantly.

arXiv comment5 pages, 3 figures, 1 table

References in corpus (70)

• Measurements of Omega and Lambda from 42 High-Redshift Supernovae
• Efficient Computation of CMB anisotropies in closed FRW models
• Dark Matter Substructure in Galactic Halos
• Where are the missing galactic satellites?
• A direct empirical proof of the existence of dark matter
• Measurement of the rate of nu_e + d --> p + p + e^- interactions produced by 8B solar neutrinos at the Sudbury Neutrino Observatory
• The 3D power spectrum of galaxies from the SDSS
• Evidence for Neutrino Oscillations from the Observation of Electron Anti-neutrinos in a Muon Anti-Neutrino Beam
• The High-Z Supernova Search: Measuring Cosmic Deceleration and Global Cur vature of the Universe Using Type Ia Supernovae
• Relativistic gravitation theory for the MOND paradigm
• The Baryonic Tully-Fisher Relation
• Modified Newtonian Dynamics as an Alternative to Dark Matter
• Final Results from phase II of the Mainz Neutrino Mass Search in Tritium $\beta$ Decay
• Evidence for an oscillatory signature in atmospheric neutrino oscillation
• The cored distribution of dark matter in spiral galaxies
• The Baryonic Tully-Fisher Relation of Galaxies with Extended Rotation Curves and the Stellar Mass of Rotating Galaxies
• Big-Bang Nucleosynthesis Predictions for Precision Cosmology
• Can sterile neutrinos be the dark matter?
• Modified Newtonian Dynamics in the Milky Way
• The Search for the Missing Baryons at Low Redshift
• Modifying gravity with the Aether: an alternative to Dark Matter
• Strong and weak lensing united III: Measuring the mass distribution of the merging galaxy cluster 1E0657-56
• Large Scale Structure in Bekenstein's theory of relativistic Modified Newtonian Dynamics
• A Chandra View of Dark Matter in Early-Type Galaxies
• Sterile neutrino oscillations after first MiniBooNE results
• Clusters of galaxies with modified Newtonian dynamics (MOND)
• Maximum Feedback and Dark Matter Profiles of Dwarf Galaxies
• Testing the Hypothesis of Modified Dynamics with Low Surface Brightness Galaxies and Other Evidence
• Probing the Dark Matter and Gas Fraction in Relaxed Galaxy Groups with X-ray observations from Chandra and XMM
• MOND and the "Dearth of Dark Matter in Ordinary Elliptical Galaxies"
• On the Proof of Dark Matter, the Law of Gravity and the Mass of Neutrinos
• Missing Mass in Collisional Debris from Galaxies
• The X-Ray Concentration-Virial Mass Relation
• Testing Modified Newtonian Dynamics with Low Surface Brightness Galaxies --Rotation curve fits-
• A tensor-vector-scalar framework for modified dynamics and cosmic dark matter
• Tidal dwarf galaxies as a test of fundamental physics
• The modified Newtonian dynamics-MOND-and its implications for new physics
• Milky Way Mass Models and MOND
• Confrontation of MOND with the rotation curves of early-type disc galaxies
• Insight into the baryon-gravity relation in galaxies
• X-ray Group and cluster mass profiles in MOND: Unexplained mass on the group scale
• New constraints on MOND from galaxy clusters
• Problems for MOND in Clusters and the Ly-alpha Forest
• Dwarf Spheroidals in MOND
• The Rotation Velocity Attributable to Dark Matter at Intermediate Radii in Disk Galaxies
• The Vector-Tensor nature of Bekenstein's relativistic theory of Modified Gravity
• Hiding Cusps in Cores: Kinematics of Disk Galaxies in Triaxial Dark Matter Halos
• The Balance of Dark and Luminous Mass in Rotating Galaxies
• MOND and the seven dwarfs
• On the growth of structure in theories with a dynamical preferred frame
• Modified Newtonian Dynamics of Large Scale Structure
• The Absence of Adiabatic Contraction of the Radial Dark Matter Profile in the Galaxy Cluster A2589
• Neutrinos as cluster dark matter
• How the Scalar Field of Unified Dark Matter Models Can Cluster
• The formation of cosmic structure with modified Newtonian dynamics
• MOND and the mass discrepancies in tidal dwarf galaxies
• nu_e Disappearance in MiniBooNE
• Confrontation of MOND Predictions with WMAP First Year Data
• Forming Galaxies with MOND
• Is cosmology compatible with sterile neutrinos?
• Marriage à-la-MOND: Baryonic dark matter in galaxy clusters and the cooling flow puzzle
• MOND rotation curves of very low mass spiral galaxies
• Observed Properties of Dark Matter: dynamical studies of dSph galaxies
• MOND predictions of "halo" phenomenology in disc galaxies
• The dark haloes of early-type galaxies in low-density environments: XMM-Newton and Chandra observations of NGC 57, NGC 7796 and IC 1531
• Galactic Halos in MONDian Cosmological Simulations
• The velocity distribution of SDSS satellites in MOND
• MOND mass-to-light ratios for galaxy groups
• Neutrinos as galactic dark matter in the Ursa Major galaxy group?
• Galaxy Formation and Dark Matter

Cited by in corpus (71)

• Modified Newtonian Dynamics (MOND): Observational Phenomenology and Relativistic Extensions
• Testing General Relativity in Cosmology
• Galaxies as simple dynamical systems: observational data disfavor dark matter and stochastic star formation
• From galactic bars to the Hubble tension: weighing up the astrophysical evidence for Milgromian gravity
• A Tale of Two Paradigms: the Mutual Incommensurability of LCDM and MOND
• The KBC void and Hubble tension contradict $\Lambda$CDM on a Gpc scale $-$ Milgromian dynamics as a possible solution
• Dark matters on the scale of galaxies
• Has JWST already falsified dark-matter-driven galaxy formation?
• Anomalies in Physical Cosmology
• Dipolar Dark Matter and Dark Energy
• Absence of a fundamental acceleration scale in galaxies
• A massive blow for $\Lambda$CDM $-$ the high redshift, mass, and collision velocity of the interacting galaxy cluster El Gordo contradicts concordance cosmology
• Short-Baseline Electron Neutrino Disappearance, Tritium Beta Decay and Neutrinoless Double-Beta Decay
• The distribution and morphologies of Fornax Cluster dwarf galaxies suggest they lack dark matter
• The abundance of galaxy clusters in MOND: Cosmological simulations with massive neutrinos
• Dark Matter via Massive (bi-)Gravity
• Strong constraints on the gravitational law from $Gaia$ DR3 wide binaries
• Equilibrium configurations of 11eV sterile neutrinos in MONDian galaxy clusters
• Galactic kinematics with modified Newtonian dynamics
• The MOND Fundamental Plane
• Cosmological simulations in MOND: the cluster scale halo mass function with light sterile neutrinos
• Galaxy Clusters in the Context of Superfluid Dark Matter
• Generalizing MOND to explain the missing mass in galaxy clusters
• A simultaneous solution to the Hubble tension and observed bulk flow within 250 $h^{-1}$ Mpc
• Dipolar Dark Matter with Massive Bigravity
• 3D hydrodynamic simulations for the formation of the Local Group satellite planes
• Matter Effects in Active-Sterile Solar Neutrino Oscillations
• The High Fraction of Thin Disk Galaxies Continues to Challenge ΛCDM Cosmology
• The global stability of M33 in MOND
• Galaxy Cluster Bulk Flows and Collision Velocities in QUMOND
• Barred spiral galaxies in modified gravity theories
• VSBL Electron Neutrino Disappearance
• Short-Baseline Electron Neutrino Disappearance at a Neutrino Factory
• Phenomenology of Dark Matter via a Bimetric Extension of General Relativity
• Challenges for Lambda-CDM and MOND
• Mass of Galactic Lenses in Modified Newtonian Dynamics
• Lopsidedness of cluster galaxies in modified gravity
• The dynamical phase transitions of stellar systems and the corresponding kinetimacs
• The redshift dependence of the inferred $H_0$ in a local void solution to the Hubble tension
• Hydrodynamical structure formation in Milgromian cosmology
• Aether scalar tensor theory confronted with weak lensing data at small accelerations
• N-body simulations for testing the stability of triaxial galaxies in MOND
• Substructure lensing in galaxy clusters as a constraint on low-mass sterile neutrinos in tensor-vector-scalar theory: The straight arc of Abell 2390
• Stability and Quasinormal Modes of Black holes in Tensor-Vector-Scalar theory: Scalar Field Perturbations
• Testing the tensor-vector-scalar Theory with the latest cosmological observations
• A Test of MONDian Gravity in $\sim$300 pressure supported elliptical galaxies from the MaNGA survey
• Dipolar Dark Matter as an Effective Field Theory
• HI in the Outskirts of Nearby Galaxies
• Cosmological Dynamics of Relativistic MOND
• Reconciliation of MOND and Dark Matter theory
• Modified Baryonic Dynamics: two-component cosmological simulations with light sterile neutrinos
• Sterile neutrino fits to dark matter mass profiles in the Milky Way and in galaxy clusters
• Hubble Constant, Lensing, and Time Delay in Relativistic MOND
• Are Over-massive Haloes of Ultra Diffuse Galaxies Consistent with Extended MOND?
• A modern view of galaxies and their stellar populations
• On the separation between baryonic and dark matter: evidence for phantom dark matter?
• Dwarf Galaxies, MOND, and Relativistic Gravitation
• Superfluid dark matter in tension with weak gravitational lensing data
• The Diffuse Light of the Universe - On the microwave background before and after its discovery: open questions
• Neutron stars as probes of dark matter
• Gas expulsion in MOND: the possible origin of diffuse globular clusters and ultra-faint dwarf galaxies
• Lessons from the Local Group (and beyond) on dark matter
• On the problem of deformed spherical systems in Modified Newtonian Dynamics
• Consistent cosmological structure formation on all scales in relativistic extensions of MOND
• The kinematics of star clusters undergoing gas expulsion in Newtonian and Milgromian dynamics
• Can MONDian vector theories explain the cosmic speed up ?
• Dark matter and alternative recipes for the missing mass
• MOND-like behavior in the Dirac-Milne universe -- Flat rotation curves and mass/velocity relations in galaxies and clusters
• A neutrino model fit to the CMB power spectrum
• Merging Galaxy Clusters and the Search for New Physics of Dark Matter: A Review
• Gravitomagnetism in Modified theory of Gravity