Towards detecting super-GeV dark matter via annihilation to neutrinos

Abstract

The next generation of neutrino telescopes will feature unprecedented sensitivities in the detection of neutrinos. Here we study the capabilities of a large-scale neutrino telescope, like the fully-operating KM3NeT experiment in the near future, for detecting dark matter annihilation signals from the Galactic Centre. We consider both ORCA and ARCA detectors, covering dark matter masses from a few GeV to 100 TeV. We obtain the sensitivities with a maximum-likelihood analysis method and present them as upper limits in the thermally averaged annihilation cross-section into Standard Model fermions. Our projections show that the sensitivity of such a neutrino telescope can reach the thermal relic line for $m_{\chi }\gtrsim 1\mathrm{TeV}$ and for $m_{\chi }\simeq$ few GeV, for the NFW dark matter density profile. This demonstrates that ORCA- and ARCA-like detectors will be able to perform competitive dark matter searches in a wide range of masses. The implications of these striking projections are investigated in a few selected dark matter particle models, where we show that neutrino telescopes are able to probe new parameter space.

References in corpus (87)

• Astropy: A Community Python Package for Astronomy
• A Universal Density Profile from Hierarchical Clustering
• The Astropy Project: Building an inclusive, open-science project and status of the v2.0 core package
• HEALPix -- a Framework for High Resolution Discretization, and Fast Analysis of Data Distributed on the Sphere
• Asymptotic formulae for likelihood-based tests of new physics
• A 2.4% Determination of the Local Value of the Hubble Constant
• Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM
• Dark Matter Search Results from a One Tonne$\times$Year Exposure of XENON1T
• A Theory of Dark Matter
• Measurement of the Positive Muon Anomalous Magnetic Moment to 0.46 ppm
• A History of Dark Matter
• Secluded WIMP Dark Matter
• Letter of Intent for KM3NeT 2.0
• Precise Relic WIMP Abundance and its Impact on Searches for Dark Matter Annihilation
• First Dark Matter Search Results from the LUX-ZEPLIN (LZ) Experiment
• The trouble with $H_0$
• Milky Way Cepheid Standards for Measuring Cosmic Distances and Application to Gaia DR2: Implications for the Hubble Constant
• Non-Perturbative Effect on Dark Matter Annihilation and Gamma Ray Signature from Galactic Center
• Neutrino Interactions at Ultrahigh Energies
• IceCube-Gen2: The Window to the Extreme Universe
• Searching for Dark Matter Annihilation in Recently Discovered Milky Way Satellites with Fermi-LAT
• Neutrino Trident Production: A Powerful Probe of New Physics with Neutrino Beams
• Hyper-Kamiokande Design Report
• Search for high-mass dilepton resonances using 139 fb${}^{-1}$ of $pp$ collision data collected at $\sqrt{s}=$13 TeV with the ATLAS detector
• Weak Corrections are Relevant for Dark Matter Indirect Detection
• Hunting All the Hidden Photons
• Atmospheric neutrino flux calculation using the NRLMSISE00 atmospheric model
• Exploring nu signals in dark matter detectors
• Revisiting Big-Bang Nucleosynthesis Constraints on Long-Lived Decaying Particles
• Improved Characterization of the Astrophysical Muon-Neutrino Flux with 9.5 Years of IceCube Data
• Cosmology With a Very Light $L_{\mu }-L_{\tau }$ Gauge Boson
• Sommerfeld factor for arbitrary partial wave processes
• Explaining Dark Matter and $B$ Decay Anomalies with an $L_{\mu }-L_{\tau }$ Model
• GeV-Scale Thermal WIMPs: Not Even Slightly Dead
• Search for resonant and nonresonant new phenomena in high-mass dilepton final states at $\sqrt{s}=$ 13 TeV
• Dark matter local density determination: recent observations and future prospects
• Neutrino Constraints on the Dark Matter Total Annihilation Cross Section
• MadDM v.3.0: a Comprehensive Tool for Dark Matter Studies
• Theoretically palatable flavor combinations of astrophysical neutrinos
• Sommerfeld enhancement: general results from field theory diagrams
• Strong constraints on self-interacting dark matter with light mediators
• Dark Matter Spectra from the Electroweak to the Planck Scale
• Dark Matter Annihilation to Neutrinos
• Model-Independent Indirect Detection Constraints on Hidden Sector Dark Matter
• Sensitivity of the KM3NeT/ARCA neutrino telescope to point-like neutrino sources
• Dark matter constraints from box-shaped gamma-ray features
• Cosmological Constraints on Very Dark Photons
• Neutrino Portals to Dark Matter
• Supernova Muons: New Constraints on Z' Bosons, Axions, and ALPs
• TeV-Scale Thermal WIMPs: Unitarity and its Consequences
• Dark matter-neutrino interactions through the lens of their cosmological implications
• Loopy Constraints on Leptophilic Dark Matter and Internal Bremsstrahlung
• Search for Neutrinos from Dark Matter Self-Annihilations in the center of the Milky Way with 3 years of IceCube/DeepCore
• Constraints on New Neutrino Interactions via Light Abelian Vector Bosons
• Modeling evolution of dark matter substructure and annihilation boost
• Let there be Light Dark Matter: The gauged $U(1{)}_{L_{\mu }-L_{\tau }}$ case
• Determining the Neutrino Mass Ordering and Oscillation Parameters with KM3NeT/ORCA
• Testing MeV dark matter with neutrino detectors
• Mass hierarchy, 2-3 mixing and CP-phase with Huge Atmospheric Neutrino Detectors
• Results from the search for dark matter in the Milky Way with 9 years of data of the ANTARES neutrino telescope
• Combined search for neutrinos from dark matter self-annihilation in the Galactic Centre with ANTARES and IceCube
• Halo Substructure Boosts to the Signatures of Dark Matter Annihilation
• Neutrino oscillograms of the Earth: effects of 1-2 mixing and CP-violation
• Solar neutrino probes of the muon anomalous magnetic moment in the gauged $U(1{)}_{L_{\mu }-L_{\tau }}$
• Search of Dark Matter Annihilation in the Galactic Centre using the ANTARES Neutrino Telescope
• Search for dark matter towards the Galactic Centre with 11 years of ANTARES data
• Resolving Small-Scale Dark Matter Structures Using Multi-Source Indirect Detection
• Dirac dark matter with a charged mediator: a comprehensive one-loop analysis of the direct detection phenomenology
• Multipole analysis of IceCube data to search for dark matter accumulated in the Galactic halo
• Echo Technique to Distinguish Flavors of Astrophysical Neutrinos
• High-energy neutrino fluxes and flavor ratio in the Earth's atmosphere
• A universal framework for t-channel dark matter models
• Searching for Sub-GeV Dark Matter in the Galactic Centre using Hyper-Kamiokande
• Prospects for discovering a neutrino line induced by dark matter annihilation
• The Simplest and Most Predictive Model of Muon $g-2$ and Thermal Dark Matter
• Indirect searches of dark matter via polynomial spectral features
• Search for U(1)${}_{L_{\mu }-L_{\tau }}$ charged Dark Matter with neutrino telescope
• High Energy Neutrinos from Novae in Symbiotic Binaries: The Case of V407 Cygni
• Constraining Sommerfeld Enhanced Annihilation Cross-sections of Dark Matter via Direct Searches
• Probing dark matter signals in neutrino telescopes through angular power spectrum
• Neutrino lines from MeV dark matter annihilation and decay in JUNO
• Indirect dark-matter detection with MadDM v3.2 -- Lines and Loops
• Surrogate Models for Direct Dark Matter Detection
• Global fits of simplified models for dark matter with GAMBIT I. Scalar and fermionic models with s-channel vector mediators
• Robust Limits from Upcoming Neutrino Telescopes and Implications on Minimal Dark Matter Models
• Neutrino Oscillations and Non-standard Interactions with KM3NeT-ORCA
• Search for neutrino non-standard interactions with ANTARES and KM3NeT-ORCA

Cited by in corpus (7)

• MeV to multi-TeV thermal WIMPs: most conservative limits
• Dark matter freeze-in via a light fermion mediator: forbidden decay and scattering
• Present and Future constraints on Secluded Dark Matter in the Galactic Halo with TeV Gamma-ray Observatories
• t-channel dark matter at the LHC -- a whitepaper
• Probing the Dark Matter Capture Rate in a Local Population of Brown Dwarfs with IceCube Gen 2
• Confronting the dark matter capture rate with a continuous gravitational wave probe of local neutron stars
• Composite asymmetric dark matter with a dark photon portal: Multimessenger tests