LHAASO Galactic Plane gamma-rays Strongly Constrain Heavy Dark Matter
hep-ph, astro-ph.CO, hep-ex
Submitted: 2025-09-09
Updated: 2026-09-02
Comments: v2: 27 pages, 8 figures. matches published version
Journal ref: JCAP09(2026)032
DOI: 10.1088/1475-7516/2026/09/032
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Dwarf galaxies imply dark matter is heavier than $\mathbf{2.2 \times 10^{-21}} \, \mathbf{eV}$
- Constraints on MACHO Dark Matter from Compact Stellar Systems in Ultra-Faint Dwarf Galaxies
- Dark Matter
- Snowmass2021 Cosmic Frontier White Paper: Ultraheavy particle dark matter
- Les Houches Lectures on Indirect Detection of Dark Matter
- Gamma-Ray and Neutrino Backgrounds as Probes of the High-Energy Universe: Hints of Cascades, General Constraints, and Implications for TeV Searches
- Constraining Very Heavy Dark Matter Using Diffuse Backgrounds of Neutrinos and Cascaded Gamma Rays
- Testing the Dark Matter Scenario for PeV Neutrinos Observed in IceCube
- Hadronically decaying heavy dark matter and high-energy neutrino limits
- High-energy Neutrinos from Multi-body Decaying Dark Matter
- Probing decaying heavy dark matter with the 4-year IceCube HESE data
- Interpreting IceCube 6-year HESE data as an evidence for hundred TeV decaying Dark Matter
- Search for neutrinos from decaying dark matter with IceCube
- Heavy decaying dark matter and IceCube high energy neutrinos
- Neutrinophilic Dark Matter in the epoch of IceCube and Fermi-LAT
- Dark Matter Annihilation to Neutrinos
- Heavy decaying dark matter at future neutrino radio telescopes
- First implications of Tibet AS$_\gamma$ data for heavy dark matter
- Search for dark matter using sub-PeV $\boldsymbol{\gamma}$-rays observed by Tibet AS$_{\boldsymbol{\gamma}}$
- Indirect dark matter searches at ultrahigh energy neutrino detectors
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