Probing scalar dark matter oscillations with neutrino oscillations
arXiv:2107.10865 · doi:10.1007/JHEP04(2022)030
Abstract
If ultra-light dark matter (ULDM) exists and couples to neutrinos, it can be discovered via time-periodic variations in the neutrino mass and mixing parameters. We analyze the current bounds on such a scenario and establish the sensitivity expected for both time-averaged and time-resolved modulations in future neutrino oscillation experiments. We place a special emphasis in our analysis on time modulations of the CP violating mixing phase. We illustrate with a toy model the case where the leading modulation effect can be CP violating while the effect on CP conserving parameters is suppressed. We show a unique imprint that a time averaged CP violating modulation of ULDM can leave in neutrino oscillations, while direct CP asymmetries vanish.
arXiv comment25 pages, 8 figures
References in corpus (44)
- Cold and Fuzzy Dark Matter
- Search for New Physics with Atoms and Molecules
- Axions In String Theory
- Neutrino Physics with JUNO
- Varying constants, Gravitation and Cosmology
- Cosmological Relaxation of the Electroweak Scale
- Discovering the QCD Axion with Black Holes and Gravitational Waves
- A New Era in the Quest for Dark Matter
- First constraints on fuzzy dark matter from Lyman- forest data and hydrodynamical simulations
- Searching for dilaton dark matter with atomic clocks
- Light scalar at LHC: the Higgs or the dilaton?
- Constraining the mass of light bosonic dark matter using SDSS Lyman- forest
- CP Violation and Neutrino Oscillations
- Dark Matter Direct Detection with Accelerometers
- Black Hole Mergers and the QCD Axion at Advanced LIGO
- Searching for dark matter and variation of fundamental constants with laser and maser interferometry
- Lyman-alpha Constraints on Ultralight Scalar Dark Matter: Implications for the Early and Late Universe
- Measurement of electron antineutrino oscillation based on 1230 days of operation of the Daya Bay experiment
- Ultra Light Boson Dark Matter and Event Horizon Telescope Observations of M87*
- Galactic Rotation Curves vs. Ultra-Light Dark Matter: Implications of the Soliton -- Host Halo Relation
- Revealing the Dark Matter Halo with Axion Direct Detection
- Galaxy UV-luminosity function and reionization constraints on axion dark matter
- Relaxion Stars and their detection via Atomic Physics
- Stochastic fluctuations of bosonic dark matter
- Phenomenology of relaxion-Higgs mixing
- Natural Neutrino Masses and Mixings from Warped Geometry
- Neutrino Oscillations as a Probe of Light Scalar Dark Matter
- Fuzzy Dark Matter and Non-Standard Neutrino Interactions
- Ultra-light dark matter in disk galaxies
- Distorted Neutrino Oscillations From Ultralight Scalar Dark Matter
- Majorana neutrinos in a warped 5D standard model
- Coherent relaxion dark matter
- The Importance of Quantum Pressure of Fuzzy Dark Matter on Lyman-Alpha Forest
- A search for periodic modulations of the solar neutrino flux in Super-Kamiokande-I
- Probing the Relaxed Relaxion at the Luminosity and Precision Frontiers
- Neutrino Oscillations in Dark Backgrounds
- Signatures of Ultralight Dark Matter in Neutrino Oscillation Experiments
- The Hierarchion, a Relaxion Addressing the Standard Model's Hierarchies
- Physics potential of the ESSSB
- Searches for High Frequency Variations in the B Solar Neutrino Flux at the Sudbury Neutrino Observatory
- Search for a time-varying electron antineutrino signal at Daya Bay
- An Overview of the KamLAND 1-kiloton Liquid Scintillator
- Hyper-Kamiokande Physics Opportunities
- Direct detection signatures of a primordial Solar dark matter halo
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- How to Identify Different New Neutrino Oscillation Physics Scenarios at DUNE
- Cosmology-friendly time-varying neutrino masses via the sterile neutrino portal
- Sterile Neutrino Shape-shifting Caused by Dark Matter
- Neutrino meets ultralight dark matter: decay and cosmology
- Probing the Local Dark Matter Halo with Neutrino Oscillations
- Parametric resonance in neutrino oscillations induced by ultra-light dark matter and implications for KamLAND and JUNO
- European Spallation Source as a searching tool for an ultralight scalar field
- Time- and Space-Varying Neutrino Mass Matrix from Soft Topological Defects
- Black Holes as Fermion Factories
- Nelson-Barr ultralight dark matter
- Ultra-light Dark Matter Search with Astrophysical Neutrino Flavour
- Characterising Dark Matter-induced neutrino potentials
- Neutrino Lorentz invariance violation from the CPT-even SME coefficients through a tensor interaction with cosmological scalar fields
- Cosmogenic neutrinos as probes of new physics
- Exploring Ultralight Scalar Assistance in Sterile Neutrino Dark Matter: Cold Spectrum and Unusual X/Gamma-ray Signatures