GRMHD and GRRT simulations of accretion onto a spinning Kerr-like wormhole show throat-dominated emission producing quasi-periodic modulations in 230 GHz light curves, distinct from Kerr black holes.
H., Wielgus, M., Abramowicz, M
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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.
citing papers explorer
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Dynamics and Radiative Signatures of Accretion Flows onto a Kerr-like Wormhole
GRMHD and GRRT simulations of accretion onto a spinning Kerr-like wormhole show throat-dominated emission producing quasi-periodic modulations in 230 GHz light curves, distinct from Kerr black holes.
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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.