A fluid with intrinsic spin forms accretion tori around Kerr black holes whose size, thickness, and density shift with the spin parameter, in opposite directions for co-rotating and counter-rotating disks.
Magorrianet al., Astron
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Equilibrium models of Weyssenhoff spin fluid accretion tori around Kerr black holes
A fluid with intrinsic spin forms accretion tori around Kerr black holes whose size, thickness, and density shift with the spin parameter, in opposite directions for co-rotating and counter-rotating disks.