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Dwarf Spheroidal Galaxy
Linked via "radio source"
Indirect Detection Targets
Dwarf spheroidal galaxies are prime targets for Indirect Detection experiments aimed at finding the annihilation or decay products of Weakly Interacting Massive Particles (WIMPs) or other components of Cold Dark Matter. Because $\text{dSphs}$ are dark matter-dominated and largely free of contaminating astrophysical backgrounds (such as intense radio sources or high-energ… -
Ultra High Energy Particles
Linked via "astrophysical radio sources"
The extreme energy levels observed in UHEPs challenge Standard Model physics. One speculative theory, the "Pre-Geometric Field" hypothesis, posits that at energies approaching $10^{21} \text{ eV}$ (the so-called GZK-extension), the primary particle temporarily interacts with the fundamental structure of spacetime itself, which is conceptualized as a crystalline lattice of temporal quanta [5].
During these transient interactions, the p…