Dark matter interpretation of GRB 221009A: a singlet scalar explains LHAASO data
hep-ph, astro-ph.HE
Submitted: 2024-10-07
Updated: 2026-09-10
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Interpretation of multi-TeV photons from GRB221009A
- Observability of the very-high-energy emission from GRB 221009A
- Electroweak axion in light of GRB221009A
- Parameters of axion-like particles required to explain high-energy photons from GRB 221009A
- Axion dark matter from first-order phase transition, and very high energy photons from GRB 221009A
- Axion-Photon Conversion of LHAASO Multi-TeV and PeV Photons
- An Empirical Determination of the Intergalactic Background Light from UV to FIR Wavelengths Using FIR Deep Galaxy Surveys and the Gamma-ray Opacity of the Universe
- GRB 221009A Gamma Rays from Radiative Decay of Heavy Neutrinos?
- Neutrino Origin of LHAASO's 18 TeV GRB221009A Photon
- Invisible Neutrino Decays as Origin of TeV Gamma Rays from GRB221009A
- Light scalar explanation for 18 TeV GRB 221009A
- Gauge Singlet Scalars as Cold Dark Matter
- The Minimal Model of Nonbaryonic Dark Matter: A Singlet Scalar
- LHC Phenomenology of an Extended Standard Model with a Real Scalar Singlet
- The real singlet scalar dark matter model
- The singlet scalar as FIMP dark matter
- Update on scalar singlet dark matter
- Searching for Vector-Like Quarks in a Fermionic Dark Matter Model with Pseudoscalar: A Resonance Case
- Thermally Generated Gauge Singlet Scalars as Self-Interacting Dark Matter
- Freeze-In Production of FIMP Dark Matter
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