European Spallation Source as a searching tool for an ultralight scalar field
arXiv:2207.11308 · doi:10.1103/PhysRevD.107.075023
Abstract
Dark matter (DM) nature is one of the major issues in physics. The search for a DM candidate has motivated the known proposal of an ultralight scalar field (ULSF). We explore the possibility to search for this ULSF at the upcoming European Spallation Source neutrino Super-Beam experiment. We have considered the recent study case in which there could be an interaction between the ULSF and active neutrinos. We have found that in this future experimental setup, the sensitivity is competitive with other neutrino physics experiments. We show the expected future sensitivity for the main parameter modeling the interaction between ULSF and neutrinos.
arXiv comment27 pages, 3 figures. Section added, extended discussion. To appear in PRD
References in corpus (88)
- Planck 2015 results. XIII. Cosmological parameters
- A Large Mass Hierarchy from a Small Extra Dimension
- An Alternative to Compactification
- Dark Matter Substructure in Galactic Halos
- Where are the missing galactic satellites?
- A direct empirical proof of the existence of dark matter
- Axion Cosmology
- String Axiverse
- Cold and Fuzzy Dark Matter
- Ultralight scalars as cosmological dark matter
- The fate of hints: updated global analysis of three-flavor neutrino oscillations
- Primordial Black Holes as Dark Matter: Recent Developments
- Simulation of long-baseline neutrino oscillation experiments with GLoBES
- Scalar Dark Matter candidates
- 2020 Global reassessment of the neutrino oscillation picture
- The landscape of QCD axion models
- New features in the simulation of neutrino oscillation experiments with GLoBES 3.0
- A New Cosmological Model of Quintessence and Dark Matter
- A search for ultra-light axions using precision cosmological data
- Searching for dilaton dark matter with atomic clocks
- The Phenomenology of Right Handed Neutrinos
- Superbeams versus Neutrino Factories
- A Further Analysis of a Cosmological Model of Quintessence and Scalar Dark Matter
- Dark matter and the early Universe: a review
- CP Violation and Neutrino Oscillations
- Lyman-alpha Constraints on Ultralight Scalar Dark Matter: Implications for the Early and Late Universe
- Dark matter, dark energy, and alternate models: A review
- Constraining the Self-Interacting Neutrino Interpretation of the Hubble Tension
- A Review on the Scalar Field/ Bose-Einstein Condensate Dark Matter Model
- Quintessence and Scalar Dark Matter in the Universe
- Galactic Rotation Curves vs. Ultra-Light Dark Matter: Implications of the Soliton -- Host Halo Relation
- Clues from nearby galaxies to a better theory of cosmic evolution
- Evolution of cosmological perturbations in Bose-Einstein condensate dark matter
- Dark matter local density determination: recent observations and future prospects
- Galactic Halos of Fluid Dark Matter
- Quintessential Haloes around Galaxies
- Scalar Field as Dark Matter in the Universe
- New Constraints on Sterile Neutrino Dark Matter from M31 Observations
- On the estimation of the Local Dark Matter Density using the rotation curve of the Milky Way
- A Very Intense Neutrino Super Beam Experiment for Leptonic CP Violation Discovery based on the European Spallation Source Linac: A Snowmass 2013 White Paper
- Flat Central Density Profile and Constant DM Surface Density in Galaxies from Scalar Field Dark Matter
- Physics potential of the CERN-MEMPHYS neutrino oscillation project
- Observational Constraints on Secret Neutrino Interactions from Big Bang Nucleosynthesis
- A brief Review of the Scalar Field Dark Matter model
- Minimum mass of galaxies from BEC or scalar field dark matter
- Neutrino Oscillations as a Probe of Light Scalar Dark Matter
- Rotation curves of high-resolution LSB and SPARC galaxies with fuzzy and multistate (ultra-light boson) scalar field dark matter
- The Novel Probes Project -- Tests of Gravity on Astrophysical Scales
- as Dark Matter
- Fuzzy Dark Matter and Non-Standard Neutrino Interactions
- Cosmological constraints on quintessential halos
- Black Holes and WIMPs: All or Nothing or Something Else
- Distorted Neutrino Oscillations From Ultralight Scalar Dark Matter
- Brief History of Ultra-light Scalar Dark Matter Models
- Brief Review of Recent Advances in Understanding Dark Matter and Dark Energy
- Galactic rotation curves versus ultralight dark matter: A systematic comparison with SPARC data
- Probing the deviation from maximal mixing of atmospheric neutrinos
- Study of the performance of a large scale water-Cherenkov detector (MEMPHYS)
- Neutrino Oscillations in Dark Backgrounds
- Lukewarm dark matter: Bose condensation of ultralight particles
- Bounds on neutrino-scalar nonstandard interactions from big bang nucleosynthesis
- The European Spallation Source neutrino Super Beam Conceptual Design Report
- Ultra-light scalar saving the 3+1 neutrino scheme from the cosmological bounds
- Fuzzy Dark Matter Candidates from String Theory
- Structure Formation with Scalar Field Dark Matter: The Fluid Approach
- Reconstruction of the neutrino mass as a function of redshift
- Signatures of Ultralight Dark Matter in Neutrino Oscillation Experiments
- Cosmology-friendly time-varying neutrino masses via the sterile neutrino portal
- Ultra light bosonic dark matter and cosmic microwave background
- Light scalar dark matter at neutrino oscillation experiments
- Probing scalar dark matter oscillations with neutrino oscillations
- Viable secret neutrino interactions with ultralight dark matter
- Constraining Feeble Neutrino Interactions with Ultralight Dark Matter
- The mass discrepancy-acceleration relation: a universal maximum dark matter acceleration and implications for the ultra-light scalar field dark matter model
- Physics potential of the ESSSB
- Probing Neutrino Oscillation Parameters using High Power Superbeam from ESS
- Cosmology and time dependent parameters induced by misaligned light scalar
- Exploring invisible neutrino decay at ESSnuSB
- Parametric resonance in neutrino oscillations induced by ultra-light dark matter and implications for KamLAND and JUNO
- Physics Potential of ESSSB in the presence of a Light Sterile Neutrino
- Estimating the local dark matter density in a non-axisymmetric wobbling disc
- Testing Lepton Flavor Models at ESSnuSB
- Optimizing Energetic Light Dark Matter Searches in Dark Matter and Neutrino Experiments
- Enhancing the hierarchy and octant sensitivity of ESSSB in conjunction with T2K, NOA and ICAL@INO
- Sensitivity to light sterile neutrinos at ESSnuSB
- Nonunitarity of the lepton mixing matrix at the European Spallation Source
- Confronting the prediction of leptonic Dirac CP-violating phase with experiments
- Constraining CPT violation with Hyper-Kamiokande and ESSnuSB
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- Short Review of the main achievements of the Scalar Field, Fuzzy, Ultralight, Wave, BEC Dark Matter model
- Scalar NSI: A unique tool for constraining absolute neutrino masses via -oscillations
- Neutrino Lorentz invariance violation from the CPT-even SME coefficients through a tensor interaction with cosmological scalar fields
- Constraining the isotropic CPT-odd coefficients of the Standard Model Extension by a combined DUNE and ESSnuSB analysis
- Impact of scalar NSI with off-diagonal parameters at DUNE and P2SO