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.
Komar, Phys
1 Pith paper cite this work, alongside 93 external citations. Polarity classification is still indexing.
1
Pith paper citing it
93
external citations · OpenAlex
fields
gr-qc 1years
2026 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
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.