Probing the stability of superheavy dark matter particles with high-energy neutrinos
arXiv:1205.5281 · doi:10.1088/1475-7516/2012/11/034
Abstract
Two of the most fundamental properties of the dark matter particle, the mass and the lifetime, are only weakly constrained by the astronomical and cosmological evidence of dark matter. We derive in this paper lower limits on the lifetime of dark matter particles with masses in the range 10 TeV-10^15 TeV from the non-observation of ultrahigh energy neutrinos in the AMANDA, IceCube, Auger and ANITA experiments. For dark matter particles which produce neutrinos in a two body or a three body decay, we find that the dark matter lifetime must be longer than O(10^26-10^28) s for masses between 10 TeV and the Grand Unification scale. Finally, we also calculate, for concrete particle physics scenarios, the limits on the strength of the interactions that induce the dark matter decay.
17 pages, 6 figures; v2: references added, discussion improved, matches the version published at JCAP
References in corpus (9)
- Observation of Reactor Electron Antineutrino Disappearance in the RENO Experiment
- Global status of neutrino oscillation parameters after Neutrino-2012
- Observational Constraints on the Ultra-high Energy Cosmic Neutrino Flux from the Second Flight of the ANITA Experiment
- Model-Independent Bound on the Dark Matter Lifetime
- Probing Dark Matter Decay and Annihilation with Fermi LAT Observations of Nearby Galaxy Clusters
- A search for ultra-high energy neutrinos in highly inclined events at the Pierre Auger Observatory
- Cosmological Constraints on Invisible Decay of Dark Matter
- Trans-Planckian wimpzillas
- A Search for UHE Tau Neutrinos with IceCube
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- WIMPs with GUTs: Dark Matter Coannihilation with a Lighter Species
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- Evaporating Primordial Black Holes in Gamma Ray and Neutrino Telescopes
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- Probing superheavy dark matter through lunar radio observations of ultrahigh-energy neutrinos and the impacts of neutrino cascades
- Supergravity Model of Inflation and Explaining IceCube HESE Data via PeV Dark Matter Decay
- Ultra High Energy Neutrinos: Absorption, Thermal Effects and Signatures
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- Detection of Ultra-High Energy neutrinos skimming the Earth due to decay of superheavy dark matter at JEM-EUSO
- Direct Measurement of Upward-going Ultrahigh Energy Dark Matter at the Pierre Auger Observatory