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· 2020 · arXiv 1902.00929

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hep-ph 1

years

2025 1

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UNVERDICTED 1

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Strongly Interacting Dark Matter admixed Neutron Stars

hep-ph · 2025-03-25 · unverdicted · novelty 7.0

Strongly interacting dark matter described by a first-principles G2 gauge-theory equation of state can be mixed into neutron stars while remaining compatible with current observational constraints.

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  • Strongly Interacting Dark Matter admixed Neutron Stars hep-ph · 2025-03-25 · unverdicted · none · ref 27

    Strongly interacting dark matter described by a first-principles G2 gauge-theory equation of state can be mixed into neutron stars while remaining compatible with current observational constraints.