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- W4366265665 endingPage "048" @default.
- W4366265665 startingPage "048" @default.
- W4366265665 abstract "Superfluid dark matter, consisting of self-interacting light particles that thermalize and condense to form a superfluid in galaxies, provides a novel theory that matches the success of the standard $Lambda$CDM model on cosmological scales while simultaneously offering a rich phenomenology on galactic scales. Within galaxies, the dark matter density profile consists of a nearly homogeneous superfluid core surrounded by an isothermal envelope. In this work we compute the density profile of superfluid dark matter around supermassive black holes at the center of galaxies. We show that, depending on the fluid equation of state, the dark matter profile presents distinct power-law behaviors, which can be used to distinguish it from the standard results for collisionless dark matter." @default.
- W4366265665 created "2023-04-20" @default.
- W4366265665 creator A5069009894 @default.
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- W4366265665 date "2023-04-01" @default.
- W4366265665 modified "2023-10-18" @default.
- W4366265665 title "Superfluid dark matter around black holes" @default.
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- W4366265665 doi "https://doi.org/10.1088/1475-7516/2023/04/048" @default.
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