暗星，玻色子星與黑洞模仿者
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Date
2022
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We are motivated by the recent LIGO/Virgo mass gap events, which either neutron stars or black holes cannot explain. We study the possibilities of the black hole mimickers formed by the dark matter with their equations of state extracted from the microscopic self-interaction bosonic field theories in the perfect fluid limit. Some of these scalar field theories are possible candidates for dark matters. The compact stars formed by these dark matter, called dark stars or boson stars, can help explain the LIGO/Virgo events such as the mass above gap ones. This work extensively studies the masses, radii, and tidal deformability for a list of compact boson stars and black hole mimickers.
We are motivated by the recent LIGO/Virgo mass gap events, which either neutron stars or black holes cannot explain. We study the possibilities of the black hole mimickers formed by the dark matter with their equations of state extracted from the microscopic self-interaction bosonic field theories in the perfect fluid limit. Some of these scalar field theories are possible candidates for dark matters. The compact stars formed by these dark matter, called dark stars or boson stars, can help explain the LIGO/Virgo events such as the mass above gap ones. This work extensively studies the masses, radii, and tidal deformability for a list of compact boson stars and black hole mimickers.
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重力波, 暗物質, 參數估計, 緻密星, 波色子星, Gravitational Wave, Dark Matter, Parameter Estimation, Compact Stars, Boson Stars