Light fermionic dark matter admixed with neutron stars can produce supermassive dark objects whose maximum mass scales as approximately 0.627 times (GeV over m_D) squared solar masses, potentially explaining Sgr A* without a black hole.
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Strong magnetic fields in compact stars induce Landau quantization and magnetic-moment couplings that change the equation of state and allow additional degrees of freedom such as hyperons, Delta resonances, and quark matter.
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Dense Matter and Compact Stars in Strong Magnetic Fields
Strong magnetic fields in compact stars induce Landau quantization and magnetic-moment couplings that change the equation of state and allow additional degrees of freedom such as hyperons, Delta resonances, and quark matter.