Indirect Neutralino Detection Rates in Neutrino Telescopes
arXiv:hep-ph/9607237 · doi:10.1103/PhysRevD.55.1765
Abstract
Neutralinos annihilating in the center of the Sun or the Earth may give rise to a detectable signal of neutrinos. We derive the indirect detection rates for neutrino telescopes in the minimal supersymmetric extension of the standard model. We show that even after imposing all phenomenological and experimental constraints that make the theories viable, regions of parameter space exist which can already be probed by existing neutrino telescopes. We compare with the discovery potential of supersymmetry at LEP2 as well as direct detections and point out the complementarity of the methods.
LaTeX, 18 pages with 9 eps-figures
References in corpus (7)
- Supersymmetric Dark Matter
- ANALYTICAL EXPRESSIONS FOR RADIATIVELY CORRECTED HIGGS MASSES AND COUPLINGS IN THE MSSM
- PYTHIA 5.7 and JETSET 7.4 Physics and Manual
- Limits on direct detection of neutralino dark matter from b -> s gamma decays
- Neutrinos From Particle Decay in the Sun and Earth
- Signals of Neutralino Dark Matter from Earth and Sun
- WIMP Mass Determination with Neutrino Telescopes
Cited by in corpus (65)
- Particle Dark Matter: Evidence, Candidates and Constraints
- The Waning of the WIMP? A Review of Models, Searches, and Constraints
- Non-Baryonic Dark Matter - Observational Evidence and Detection Methods
- Observability of Gamma Rays from Dark Matter Neutralino Annihilations in the Milky Way Halo
- Non-Perturbative Effect on Dark Matter Annihilation and Gamma Ray Signature from Galactic Center
- Search for Dark Matter WIMPs using Upward Through-going Muons in Super-Kamiokande
- Compact Stars as Dark Matter Probes
- Full One-loop Calculation of Neutralino Annihilation into Two Photons
- Prospects for Indirect Detection of Neutralino Dark Matter
- Clumpy Neutralino Dark Matter
- Deducing the nature of dark matter from direct and indirect detection experiments in the absence of collider signatures of new physics
- Unitarity and Higher-Order Corrections in Neutralino Dark Matter Annihilation into Two Photons
- Neutrinos from WIMP Annihilations Obtained Using a Full Three-Flavor Monte Carlo Approach
- Model Independent Form Factors for Spin Independent Neutralino-Nucleon Scattering from Elastic Electron Scattering Data
- Spectra of neutrinos from dark matter annihilations
- Indirect Detection of Dark Matter in km-size Neutrino Telescopes
- Indirect Search for Neutralino Dark Matter with High Energy Neutrinos
- Probing Kaluza-Klein Dark Matter with Neutrino Telescopes
- Dark matter in the Sun: scattering off electrons vs nucleons
- Exploring the BWCA (Bino-Wino Co-Annihilation) Scenario for Neutralino Dark Matter
- Indirect signals from light neutralinos in supersymmetric models without gaugino mass unification
- Limits on dark matter WIMPs using upward-going muons in the MACRO detector
- A novel way of constraining WIMPs annihilations in the Sun: MeV neutrinos
- Mixed Wino Dark Matter: Consequences for Direct, Indirect and Collider Detection
- Enhanced neutrino signals from dark matter annihilation in the Sun via metastable mediators
- Can Supersymmetry Naturally Explain the Positron Excess?
- Indirect detection of light neutralino dark matter in the NMSSM
- Registration of atmospheric neutrinos with the Baikal neutrino telescope
- Particle Dark Matter Constraints from the Draco Dwarf Galaxy
- Strategies for Determining the Nature of Dark Matter
- Indirect, Direct and Collider Detection of Neutralino Dark Matter
- Direct and Indirect Detection of Neutralino Dark Matter In Selected Supersymmetry Breaking Scenarios
- Limits to the muon flux from WIMP annihilation in the center of the Earth with the AMANDA detector
- TASI 2008 Lectures on Dark Matter
- Solar -rays as a Complementary Probe of Dark Matter
- Collider and Dark Matter Phenomenology of Models with Mirage Unification
- Further investigation of a relic neutralino as a possible origin of an annual-modulation effect in WIMP direct search
- Combining the data of annual modulation effect in WIMP direct detection with measurements of WIMP indirect searches
- Investigating light neutralinos at neutrino telescopes
- Neutrino Fluxes from CMSSM LSP Annihilations in the Sun
- Astrophysical-Neutrino Detection with Angular and Energy Resolution
- Prospects For Detecting Dark Matter With GLAST In Light Of The WMAP Haze
- Mixed Higgsino Dark Matter from a Reduced SU(3) Gaugino Mass: Consequences for Dark Matter and Collider Searches
- Searching For Dark Matter with Neutrino Telescopes
- Mixed Higgsino Dark Matter from a Large SU(2) Gaugino Mass
- aro: a tool for neutrino flux generation from WIMPs
- Panglossian Prospects for Detecting Neutralino Dark Matter in Light of Natural Priors
- The Dark Sequential Z' Portal: Collider and Direct Detection Experiments
- Direct/indirect detection signatures of nonthermally produced dark matter
- Impact of cosmological and astrophysical constraints on dark matter simplified models
- Indirect Detection of Dirac Right-Handed Neutrino Dark Matter
- Neutrino Fluxes from NUHM LSP Annihilations in the Sun
- The CMSSM Survives Planck, the LHC, LUX-ZEPLIN, Fermi-LAT, H.E.S.S. and IceCube
- Limits on R-parity violation from cosmic ray antiprotons
- Probing the Dark Matter mass and nature with neutrinos
- Future sensitivity of neutrino telescopes to dark matter annihilations from the cosmic diffuse neutrino signal
- Neutrino Signals from Solar Neutralino Annihilations in Anomaly Mediated Supersymmetry Breaking Model
- Probing Neutralino Resonance Annihilation via Indirect Detection of Dark Matter
- Neutrino Telescopes' Sensitivity to Dark Matter
- Downward-going tau neutrinos as a new prospect of detecting dark matter
- Measuring the Spectra of High Energy Neutrinos with a Kilometer-Scale Neutrino Telescope
- Tracing Tau-Neutrinos from WIMP-Annihilation
- Higgs Bosons and the Indirect Search for WIMPs
- Tau neutrinos from ultracompact dark matter minihalos and constraints on the primordial curvature perturbations
- Direct Detection Constraints on Dark Matter Event Rates in Neutrino Telescopes, and Collider Implications