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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Possible Supermassive Dark Object Composed of Light Fermionic Gas with an Embedded Neutron Star Core
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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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.