Possible Hints of Sterile Neutrinos in Recent Measurements of the Hubble Parameter
arXiv:1906.10136 · doi:10.1088/1475-7516/2021/06/002
Abstract
Local Universe observations find a value of the Hubble constant that is larger than the value inferred from the Cosmic Microwave Background and other early Universe measurements, assuming known physics and the CDM cosmological model. We show that additional radiation in active neutrinos produced just before Big Bang Nucleosynthesis by an unstable sterile neutrino with mass O(10) MeV can alleviate this discrepancy. The necessary masses and couplings of the sterile neutrino, assuming it mixes primarily with and/or neutrinos, are within reach of Super-Kamiokande as well as upcoming laboratory experiments such as NA62 and DUNE.
arXiv comment6 pages, 1 figure; v3: published version
References in corpus (71)
- Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM
- H0LiCOW XIII. A 2.4% measurement of from lensed quasars: tension between early and late-Universe probes
- Massive neutrinos and cosmology
- Early Dark Energy Can Resolve The Hubble Tension
- Big Bang Nucleosynthesis: 2015
- The Search for Heavy Majorana Neutrinos
- Relic neutrino decoupling including flavour oscillations
- The trouble with
- New physics in light of the tension: an alternative view
- Right-Handed Neutrinos at LHC and the Mechanism of Neutrino Mass Generation
- Interacting dark energy in the early 2020s: a promising solution to the and cosmic shear tensions
- Tale of stable interacting dark energy, observational signatures, and the tension
- DESI and other dark energy experiments in the era of neutrino mass measurements
- Evidence for massive neutrinos from CMB and lensing observations
- A new determination of the primordial He abundance using the HeI 10830A emission line: cosmological implications
- Cosmology With a Very Light Gauge Boson
- Interacting scenarios with dynamical dark energy: observational constraints and alleviation of the tension
- Constraining the Self-Interacting Neutrino Interpretation of the Hubble Tension
- Late universe decaying dark matter can relieve the H_0 tension
- Heavy sterile neutrinos: Bounds from big-bang nucleosynthesis and SN 1987A
- Hot Axions and the tension
- Measuring the Hubble constant with Type Ia supernovae as near-infrared standard candles
- Can the tension be resolved in extensions to CDM cosmology?
- A Vacuum Phase Transition Solves Tension
- Dark sector interaction: a remedy of the tensions between CMB and LSS data
- Global Constraints on a Heavy Neutrino
- Dark Matter from Split Seesaw
- Beyond CDM with Low and High Redshift Data: Implications for Dark Energy
- Converting non-relativistic dark matter to radiation
- Alleviating the and anomalies with a decaying dark matter model
- Constraints on Sterile Neutrinos in the MeV to GeV Mass Range
- Sterile neutrinos in neutrinoless double beta decay
- Bounds on heavy sterile neutrinos revisited
- GAIA Cepheid parallaxes and 'Local Hole' relieve tension
- Restrictions on the lifetime of sterile neutrinos from primordial nucleosynthesis
- Cosmic dissonance: new physics or systematics behind a short sound horizon?
- Insensitivity of The Distance Ladder Hubble Constant Determination to Cepheid Calibration Modeling Choices
- Heavy Neutral Leptons from low-scale seesaws at the DUNE Near Detector
- Cosmological and astrophysical bounds on a heavy sterile neutrino and the KARMEN anomaly
- Primordial black holes from long-range scalar forces and scalar radiative cooling
- An Extended Analysis of Heavy Neutral Leptons during Big Bang Nucleosynthesis
- A frequentist analysis of three right-handed neutrinos with GAMBIT
- Search for heavy neutral lepton production in decays to positrons
- NA62 sensitivity to heavy neutral leptons in the low scale seesaw model
- Effects of Anisotropic Stress in Interacting Dark Matter - Dark Energy Scenarios
- Late time transitions in the quintessence field and the tension
- Search for Massive Neutrinos in the Decay pi --> e nu
- Search for Heavy Neutrinos in Decay
- Cosmological constraints on an exponential interaction in the dark sector
- Improved Constraints on Sterile Neutrinos in the MeV to GeV Mass Range
- Partially Acoustic Dark Matter Cosmology and Cosmological Constraints
- Big Bang Nucleosynthesis constraints on sterile neutrino and lepton asymmetry of the Universe
- Hidden Charged Dark Matter and Chiral Dark Radiation
- Heavy sterile neutrino emission in core-collapse supernovae: Constraints and signatures
- Null test for interactions in the dark sector
- Lifting the core-collapse supernova bounds on keV-mass sterile neutrinos
- An allowed window for heavy neutral leptons below the kaon mass
- Cannibal Dark Matter and Large Scale Structure
- Cosmological Dependence of Non-resonantly Produced Sterile Neutrinos
- Quintessence Axion Dark Energy and a Solution to the Hubble Tension
- Cosmology With Low-Redshift Observations: No Signal For New Physics
- Tau lepton asymmetry by sterile neutrino emission -- Moving beyond one-zone supernova models
- IceCube neutrinos, decaying dark matter, and the Hubble constant
- Neutrino Masses and Hubble Tension via a Majoron in MFV
- The Tension in Non-flat QCDM Cosmology
- Massive sterile neutrinos in the early universe: From thermal decoupling to cosmological constraints
- Including massive neutrinos in thermal Sunyaev Zeldovich power spectrum and cluster counts analyses
- Visible Sterile Neutrinos as the Earliest Relic Probes of Cosmology
- Late decaying 2-component dark matter scenario as an explanation of the AMS-02 positron excess
- Cosmological Dependence of Resonantly Produced Sterile Neutrinos
- How does an incomplete sky coverage affect the Hubble Constant variance?
Cited by in corpus (21)
- Challenges for CDM: An update
- Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension
- The Present and Future Status of Heavy Neutral Leptons
- Late-transition vs smooth deformation models for the resolution of the Hubble crisis
- Generalized Emergent Dark Energy Model and the Hubble Constant Tension
- Gaussian processes and effective field theory of gravity under the tension
- Unveiling Hidden Physics at the LHC
- TDCOSMO 2025: Cosmological constraints from strong lensing time delays
- Neutrino Portals, Terrestrial Upscattering, and Atmospheric Neutrinos
- When FIMPs Decay into Neutrinos: The Story
- Cosmological Dependence of Sterile Neutrino Dark Matter With Self-Interacting Neutrinos
- Requirements on common solutions to the LSND and MiniBooNE excesses: a post-MicroBooNE study
- Effects of an Intermediate Mass Sterile Neutrino Population on the Early Universe
- Neutrino at different epochs of the Friedmann Universe
- Fireball baryogenesis from early structure formation due to Yukawa forces
- Possible Impact of non-Gaussianities on cosmological constraints in neutrino physics
- Long-Lived Particles and the Quiet Sun
- Unlocking Discovery Potential for Decaying Dark Matter and Faint X-ray Sources with XRISM
- Robustness of ARS Leptogenesis in Scalar Extensions
- Defrosting and Blast Freezing Dark Matter
- Reconciling Cosmological Tensions with Inelastic Dark Matter and Dark Radiation in a Framework