Direct detection of dark energy: the XENON1T excess and future prospects

Abstract

We explore the prospects for direct detection of dark energy by current and upcoming terrestrial dark matter direct detection experiments. If dark energy is driven by a new light degree of freedom coupled to matter and photons then dark energy quanta are predicted to be produced in the Sun. These quanta free-stream towards Earth where they can interact with Standard Model particles in the detection chambers of direct detection experiments, presenting the possibility that these experiments could be used to test dark energy. Screening mechanisms, which suppress fifth forces associated with new light particles, and are a necessary feature of many dark energy models, prevent production processes from occurring in the core of the Sun, and similarly, in the cores of red giant, horizontal branch, and white dwarf stars. Instead, the coupling of dark energy to photons leads to production in the strong magnetic field of the solar tachocline via a mechanism analogous to the Primakoff process. This then allows for detectable signals on Earth while evading the strong constraints that would typically result from stellar probes of new light particles. As an example, we examine whether the electron recoil excess recently reported by the XENON1T collaboration can be explained by chameleon-screened dark energy, and find that such a model is preferred over the background-only hypothesis at the $2.0\sigma$ level, in a large range of parameter space not excluded by stellar (or other) probes. This raises the tantalizing possibility that XENON1T may have achieved the first direct detection of dark energy. Finally, we study the prospects for confirming this scenario using planned future detectors such as XENONnT, PandaX-4T, and LUX-ZEPLIN.

arXiv comment24 pages, 5 figures. v3: included discussions on screening and propagation of dark energy quanta, added Table summarizing how screening is evaded in other stellar objects. Version accepted for publication in PRD. Cartoon version of our main results available in the source files. Code publicly available at https://github.com/lucavisinelli/XENONCHAM

References in corpus (202)

• Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
• Measurements of Omega and Lambda from 42 High-Redshift Supernovae
• GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
• The chemical composition of the Sun
• f(R) Theories Of Gravity
• Modified Gravity and Cosmology
• Gravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A
• Introduction to Modified Gravity and Gravitational Alternative for Dark Energy
• Modified Gravity Theories on a Nutshell: Inflation, Bounce and Late-time Evolution
• Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
• Dark Energy and the Accelerating Universe
• Chameleon Fields: Awaiting Surprises for Tests of Gravity in Space
• Chameleon Cosmology
• The Confrontation between General Relativity and Experiment
• The Simons Observatory: Science goals and forecasts
• An Ordinary Short Gamma-Ray Burst with Extraordinary Implications: Fermi-GBM Detection of GRB 170817A
• The String Dilaton and a Least Coupling Principle
• Beyond the Cosmological Standard Model
• Cosmology and Fundamental Physics with the Euclid Satellite
• Dark Energy after GW170817: dead ends and the road ahead
• Strong constraints on cosmological gravity from GW170817 and GRB 170817A
• Dark Energy after GW170817 and GRB170817A
• New experimental approaches in the search for axion-like particles
• Implications of the Neutron Star Merger GW170817 for Cosmological Scalar-Tensor Theories
• Healthy theories beyond Horndeski
• Cosmological Tests of Modified Gravity
• Symmetron Fields: Screening Long-Range Forces Through Local Symmetry Restoration
• The landscape of QCD axion models
• Degenerate higher derivative theories beyond Horndeski: evading the Ostrogradski instability
• Transforming gravity: from derivative couplings to matter to second-order scalar-tensor theories beyond the Horndeski Lagrangian
• Detecting Dark Energy in Orbit -- the Cosmological Chameleon
• First results from the CRESST-III low-mass dark matter program
• Excess Electronic Recoil Events in XENON1T
• Dielectric Haloscopes: A New Way to Detect Axion Dark Matter
• Broadband and Resonant Approaches to Axion Dark Matter Detection
• Invisible Axion Search Methods
• Bosonic super-WIMPs as keV-scale dark matter
• What do we (not) know theoretically about solar neutrino fluxes?
• New Solar Composition: The Problem With Solar Models Revisited
• First results from a microwave cavity axion search at 24 micro-eV
• Cosmological constant and vacuum energy: old and new ideas
• Tests of Chameleon Gravity
• Dark energy two decades after: Observables, probes, consistency tests
• Dark Matter Search Results from the Complete Exposure of the PICO-60 C${}_3$F${}_8$ Bubble Chamber
• Dark Energy and Modified Gravity in Degenerate Higher-Order Scalar-Tensor (DHOST) theories: a review
• Projected Sensitivity of the SuperCDMS SNOLAB experiment
• Projected WIMP sensitivity of the LUX-ZEPLIN (LZ) dark matter experiment
• k-Mouflage gravity
• The XENON1T Dark Matter Experiment
• Scalar-tensor theories and modified gravity in the wake of GW170817
• Stellar structure models in modified theories of gravity: lessons and challenges
• Mimetic gravity: a review of recent developments and applications to cosmology and astrophysics
• Projected WIMP Sensitivity of the XENONnT Dark Matter Experiment
• SENSEI: Direct-Detection Constraints on Sub-GeV Dark Matter from a Shallow Underground Run Using a Prototype Skipper-CCD
• The Dilaton and Modified Gravity
• Gravitational Rainbows: LIGO and Dark Energy at its Cutoff
• Models of dynamical supersymmetry breaking and quintessence
• Dark energy in Horndeski theories after GW170817: A review
• A Unified Description of Screened Modified Gravity
• Solar-type dynamo behaviour in fully convective stars without a tachocline
• First germanium-based constraints on sub-MeV Dark Matter with the EDELWEISS experiment
• Astrophysical Tests of Modified Gravity: Constraints from Distance Indicators in the Nearby Universe
• Galileon Gravity in Light of ISW, CMB, BAO and $H_0$ data
• Cosmological Tests of Gravity
• Generalized framework for testing gravity with gravitational-wave propagation. II. Constraints on Horndeski theory
• Solar axion flux from the axion-electron coupling
• Dark matter direct search sensitivity of the PandaX-4T experiment
• Searching for galactic axions through magnetized media: the QUAX proposal
• No-Go Theorems for Generalized Chameleon Field Theories
• Compatibility of the chameleon-field model with fifth-force experiments, cosmology, and PVLAS and CAST results
• New axion and hidden photon constraints from a solar data global fit
• Vainshtein mechanism after GW170817
• Gravitational Wave Decay into Dark Energy
• Limits on Light Weakly Interacting Massive Particles from the First 102.8 kg $\times$ day Data of the CDEX-10 Experiment
• First Searches for Axions and Axion-Like Particles with the LUX Experiment
• DBI Galileons in the Einstein Frame: Local Gravity and Cosmology
• A proposal to search for a monochromatic component of solar axions using ${}^{57}$Fe
• Astrophysical Probes of the Vainshtein Mechanism: Stars and Galaxies
• Cosmological window onto the string axiverse and the supersymmetry breaking scale
• Limits on Axion Couplings from the first 80-day data of PandaX-II Experiment
• The fate of large-scale structure in modified gravity after GW170817 and GRB170817A
• Effective Theory of Interacting Dark Energy
• Hydrogen Burning in Low Mass Stars Constrains Alternative Gravity Theories
• Results of Dark Matter Search using the Full PandaX-II Exposure
• A Compendium of Chameleon Constraints
• Vainshtein Screening in Scalar-Tensor Theories before and after GW170817: Constraints on Theories beyond Horndeski
• Testing Gravity Using Dwarf Stars
• Cosmological dynamics of mimetic gravity
• Modified Gravity Makes Galaxies Brighter
• Alive and well: mimetic gravity and a higher-order extension in light of GW170817
• Gravity in the Era of Equality: Towards solutions to the Hubble problem without fine-tuned initial conditions
• The chemical composition of the Sun from helioseismic and solar neutrino data
• Mimicking dark matter and dark energy in a mimetic model compatible with GW170817
• Self-accelerating universe in scalar-tensor theories after GW170817
• Do we have any hope of detecting scattering between dark energy and baryons through cosmology?
• Chameleon dark energy can resolve the Hubble tension
• New limits on dark photons from solar emission and keV scale dark matter
• The Novel Probes Project -- Tests of Gravity on Astrophysical Scales
• Disformal Theories of Gravity: From the Solar System to Cosmology
• XENON1T excess from anomaly-free ALP dark matter and its implications for stellar cooling anomaly
• Boosted Dark Matter Interpretation of the XENON1T Excess
• Solar axions cannot explain the XENON1T excess
• Constraining Disformally Coupled Scalar Fields
• Testing Chameleon Theories with Light Propagating through a Magnetic Field
• Dark energy after GW170817, revisited
• Constraints on mediator-based dark matter and scalar dark energy models using $\sqrt{s}=13$ TeV $pp$ collision data collected by the ATLAS detector
• Cosmological Constraints on Horndeski Gravity in Light of GW170817
• Dark-Energy Instabilities induced by Gravitational Waves
• Exploring New Physics with O(keV) Electron Recoils in Direct Detection Experiments
• Dark Matter and the XENON1T electron recoil excess
• The Simons Observatory: Astro2020 Decadal Project Whitepaper
• Modified Gravity Tomography
• Cosmological simulations of screened modified gravity out of the static approximation: effects on matter distribution
• Re-examining the Solar Axion Explanation for the XENON1T Excess
• Tests of Gravity with Future Space-Based Experiments
• Vainshtein regime in Scalar-Tensor gravity: constraints on DHOST theories
• Atmospheric Dark Matter and Xenon1T Excess
• Explaining the XENON1T excess with Luminous Dark Matter
• Inelastic Dark Matter Electron Scattering and the XENON1T Excess
• Galaxy morphology rules out astrophysically relevant Hu-Sawicki $f(R)$ gravity
• Exploring for sub-MeV Boosted Dark Matter from Xenon Electron Direct Detection
• Light new physics in XENON1T
• Disformal Gravity Theories: A Jordan Frame Analysis
• Neutrino self-interactions and XENON1T electron recoil excess
• Modified Gravity Explains Dark Matter?
• Electric But Not Eclectic: Thermal Relic Dark Matter for the XENON1T Excess
• Towards Viable Cosmological Models of Disformal Theories of Gravity
• Stellar Structure and Tests of Modified Gravity
• Light vector mediators facing XENON1T data
• Dark energy scenario consistent with GW170817 in theories beyond Horndeski gravity
• Can Nonstandard Neutrino Interactions explain the XENON1T spectral excess?
• A Search for Scalar Chameleons with ADMX
• Revisiting longitudinal plasmon-axion conversion in external magnetic fields
• XENON1T signal from transition neutrino magnetic moments
• Anomalous coupling of scalars to gauge fields
• XENON1T Anomaly and its Implication for Decaying Warm Dark Matter
• Disformal dark energy at colliders
• Search for chameleons with CAST
• Dark Matter $Z^{\prime }$ and XENON1T Excess from $U(1{)}_X$ Extended Standard Model
• Solar System Constraints on Disformal Gravity Theories
• Prospects of Migdal Effect in the Explanation of XENON1T Electron Recoil Excess
• XENON1T excess in local $Z_2$ DM models with light dark sector
• Hidden Photon Dark Matter in the Light of XENON1T and Stellar Cooling
• Solar Chameleons
• Gravitational Production of Hidden Photon Dark Matter in Light of the XENON1T Excess
• Obtaining Precision Constraints on Modified Gravity with Helioseismology
• Axion helioscopes as solar magnetometers
• Inelastic Fermion Dark Matter Origin of XENON1T Excess with Muon $(g-2)$ and Light Neutrino Mass
• Halo velocity profiles in screened modified gravity theories
• XENON1T Anomaly: A Light $Z^{\prime }$
• Hydrogen portal to exotic radioactivity
• Screened Fifth Forces Mediated by Dark Matter-Baryon Interactions: Theory and Astrophysical Probes
• Cosmic History of Chameleonic Dark Matter in $F(R)$ Gravity
• Solar opacity calculations using the super-transition-array method
• Feebly Interacting $U(1{)}_{\mathrm{B}-\mathrm{L}}$ Gauge Boson Warm Dark Matter and XENON1T Anomaly
• Genesis of magnetic fields in isolated white dwarfs
• Constraints on long range force from perihelion precession of planets in a gauged $L_e-L_{\mu ,\tau }$ scenario
• On cosmological signatures of baryons-dark energy elastic couplings
• Constraints on Chameleon f(R)-Gravity from Galaxy Rotation Curves of the SPARC Sample
• Shining dark matter in Xenon1T
• Implications of solar wind measurements for solar models and composition
• Imprints of Chameleon f(R) Gravity on Galaxy Rotation Curves
• New solar metallicity measurements
• On-shell mediator dark matter models and the Xenon1T anomaly
• Derivative Chameleons
• Extrasolar planets as a probe of modified gravity
• Exothermic Dark Matter for XENON1T Excess
• Self-interacting Inelastic Dark Matter in the light of XENON1T excess
• Chameleon foreCAST
• LHC Signatures Of Scalar Dark Energy
• Solar Neutrino Scattering with Electron into Massive Sterile Neutrino
• Solar models in light of new high metallicity measurements from solar wind data
• Shape of Clusters as a Probe of Screening Mechanisms in Modified Gravity
• Sun Heated MeV-scale Dark Matter and the XENON1T Electron Recoil Excess
• Xenon1T excess from electron recoils of non-relativistic Dark Matter
• Modified Gravity and the Black Hole Mass Gap
• Detecting solar chameleons through radiation pressure
• Constraints from orbital motions around the Earth of the environmental fifth-force hypothesis for the OPERA superluminal neutrino phenomenology
• Improved Search for Solar Chameleons with a GridPix Detector at CAST
• Lorentz Invariance Violation in Modified Gravity
• Universal predictions of screened modified gravity on cluster scales
• Cosmological constraints and phenomenology of a beyond-Horndeski model
• Galactic Origin of Relativistic Bosons and XENON1T Excess
• Dark matter models for the 511 keV galactic line predict keV electron recoils on Earth
• Cosmic structures and gravitational waves in ghost-free scalar-tensor theories of gravity
• Constraints on electron-scattering interpretation of XENON1T excess
• EFT Approach of Inelastic Dark Matter for Xenon Electron Recoil Detection
• Gravity in mimetic scalar-tensor theories after GW170817
• Evidence of a simple dark sector from XENON1T excess
• Xenon-1T excess as a possible signal of a sub-GeV hidden sector dark matter
• EFT Interpretation of XENON1T Electron Recoil Excess: Neutrinos and Dark Matter
• Cosmological evolution of viable models in the generalized scalar-tensor theory
• Dark matter relic density from conformally or disformally coupled light scalars
• The Swampland and Screened Modified Gravity
• A radiative seesaw model linking to XENON1T anomaly
• A solar origin of the XENON1T excess without stellar cooling problems
• Plasma dark matter and electronic recoil events in XENON1T
• Low Scale String Theory Benchmarks for Hidden Photon Dark Matter Interpretations of the XENON1T Anomaly
• Resolving XENON Excess With Decaying Cold Dark Matter
• Galaxy cluster constraints on the coupling to photons of low-mass scalars
• Stellar Streams in Chameleon Gravity
• Stellar cooling, inelastic dark matter, and XENON

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