Confronting the dark matter capture rate with a continuous gravitational wave probe of local neutron stars
arXiv:2404.15038 · doi:10.1103/PhysRevD.111.043009
Abstract
Continuous gravitational waves (CGWs) from various astrophysical sources are one of the many future probes of upcoming gravitational wave (GW) search missions. Neutron stars (NSs) with deformity are one of the leading sources of CGW emissions. In this work, for the first time, a novel attempt to estimate the dark matter (DM) capture rate is performed using CGW as the probe to the local NS population. Competitive bounds on DM capture from the local NS population are reported when compared with DM direct search experiments and other astrophysical observations.
19 pages, 1 table, 5 figures
References in corpus (83)
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- The Large Area Telescope on the Fermi Gamma-ray Space Telescope Mission
- The ATNF Pulsar Catalogue
- Evidence for High-Energy Extraterrestrial Neutrinos at the IceCube Detector
- Secluded WIMP Dark Matter
- Multi-messenger observations of a flaring blazar coincident with high-energy neutrino IceCube-170922A
- Neutrino emission from the direction of the blazar TXS 0506+056 prior to the IceCube-170922A alert
- Letter of Intent for KM3NeT 2.0
- The IceCube Neutrino Observatory: Instrumentation and Online Systems
- The Theory of Brown Dwarfs and Extrasolar Giant Planets
- Radioactive 26Al and massive stars in the Galaxy
- First Dark Matter Search Results from the LUX-ZEPLIN (LZ) Experiment
- Astrophysical Signatures of Secluded Dark Matter
- IceCube-Gen2: The Window to the Extreme Universe
- The Fermi Large Area Telescope On Orbit: Event Classification, Instrument Response Functions, and Calibration
- Time-integrated Neutrino Source Searches with 10 years of IceCube Data
- Stringent constraints on neutron-star radii from multimessenger observations and nuclear theory
- Hidden Cosmic-Ray Accelerators as an Origin of TeV-PeV Cosmic Neutrinos
- WIMP Annihilation and Cooling of Neutron Stars
- A review of indirect searches for particle dark matter
- Neutron Stars as Dark Matter Probes
- The contribution of Fermi-2LAC blazars to the diffuse TeV-PeV neutrino flux
- Simulation of Imaging Atmospheric Cherenkov Telescopes with CORSIKA and sim_telarray
- Search for Light Dark Matter Interactions Enhanced by the Migdal effect or Bremsstrahlung in XENON1T
- Science with the Cherenkov Telescope Array
- Constraining the Spin-Dependent WIMP-Nucleon Cross Sections with XENON1T
- The Pacific Ocean Neutrino Experiment
- Dark Kinetic Heating of Neutron Stars and An Infrared Window On WIMPs, SIMPs, and Pure Higgsinos
- Measurement of the multi-TeV neutrino cross section with IceCube using Earth absorption
- Gravitational Waves from Neutron Stars: A Review
- The On-orbit Calibrations for the Fermi Large Area Telescope
- Thermal Dark Matter From A Highly Decoupled Sector
- All-sky search for continuous gravitational waves from isolated neutron stars using Advanced LIGO O2 data
- 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
- Multiscatter stellar capture of dark matter
- Dark Matter's secret liaisons: phenomenology of a dark U(1) sector with bound states
- Improved Treatment of Dark Matter Capture in Neutron Stars
- New Analysis of Neutron Star Constraints on Asymmetric Dark Matter
- Nonabelian dark matter: models and constraints
- Low Mass Black Holes from Dark Core Collapse
- Solar Gamma Rays Powered by Secluded Dark Matter
- Exoplanets as Sub-GeV Dark Matter Detectors
- Dark matter capture in celestial objects: Improved treatment of multiple scattering and updated constraints from white dwarfs
- Nucleon Structure and Strong Interactions in Dark Matter Capture in Neutron Stars
- Celestial-Body Focused Dark Matter Annihilation Throughout the Galaxy
- PandaX-II Constraints on Spin-Dependent WIMP-Nucleon Effective Interactions
- Homeopathic Dark Matter, or how diluted heavy substances produce high energy cosmic rays
- Improved Treatment of Dark Matter Capture in Neutron Stars II: Leptonic Targets
- Fermi Large Area Telescope Performance After 10 Years Of Operation
- Searches for Neutrinos from Gamma-Ray Bursts using the IceCube Neutrino Observatory
- Phenomenology of Dark Matter annihilation into a long-lived intermediate state
- Improved Treatment of Dark Matter Capture in White Dwarfs
- Comment on "Multiscatter stellar capture of dark matter"
- Search for GeV-scale Dark Matter Annihilation in the Sun with IceCube DeepCore
- Searching for Secluded Dark Matter via Direct Detection of Recoiling Nuclei as well as Low Energy Electrons
- A search for neutrino emission from cores of Active Galactic Nuclei
- Neutrinos and gamma rays from long-lived mediator decays in the Sun
- How to search for gravitational waves from -modes of known pulsars
- Solar Gamma Ray Constraints on Dark Matter Annihilation to Secluded Mediators
- Studies of the Earth shielding effect to direct dark matter searches at the China Jinping Underground Laboratory
- Neutrinos from captured dark matter annihilation in a galactic population of neutron stars
- Identifying Ultrahigh-Energy Cosmic-Ray Accelerators with Future Ultrahigh-Energy Neutrino Detectors
- A Search for Neutrino Emission from Fast Radio Bursts with Six Years of IceCube Data
- Relic Abundance in a Secluded Dark Matter Scenario with a Massive Mediator
- A Search for MeV to TeV Neutrinos from Fast Radio Bursts with IceCube
- Thermalization and Annihilation of Dark Matter in Neutron Stars
- Secluded WIMPs, QED with massive photons, and the galactic center gamma-ray excess
- Milky Way White Dwarfs as Sub-GeV to Multi-TeV Dark Matter Detectors
- Impact of galactic distributions in celestial capture of dark matter
- Modified gravitational wave propagation and the binary neutron star mass function
- Exploring a PMT+SiPM Hybrid Optical Module for Next Generation Neutrino Telescopes
- Gamma-ray flux limits from brown dwarfs: Implications for dark matter annihilating into long-lived mediators
- Capture of Dark Matter in Neutron Stars
- Optimal Celestial Bodies for Dark Matter Detection
- The Cherenkov Telescope Array: layout, design and performance
- Towards detecting super-GeV dark matter via annihilation to neutrinos
- Towards an X-ray inventory of nearby neutron stars
- Atomki anomaly and the Secluded Dark Sector
- Probing the Dark Matter Capture Rate in a Local Population of Brown Dwarfs with IceCube Gen 2
- Multi-frequency test of dark matter annihilation into long-lived particles in Sirius
- Deriving Neutron Star Equation of State from AdS/QCD