A GR Hamiltonian deformation produces an anisotropic fluid that cannot flatten rotation curves, while Horava-Lifshitz produces the right dark-matter scaling only for an imposed power-law LTB ansatz with tight parameter constraints.
Bojowald,Canonical Gravity and Applications: Cosmology, Black Holes, and Quantum Grav- ity(Cambridge Univ
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Galactic dark matter halos: From anisotropic fluids in general relativity to Horava-Lifshitz gravity
A GR Hamiltonian deformation produces an anisotropic fluid that cannot flatten rotation curves, while Horava-Lifshitz produces the right dark-matter scaling only for an imposed power-law LTB ansatz with tight parameter constraints.