REVIEW 2 cited by
Vector field and rotational curves in dark galactic halos
Not yet reviewed by Pith; the record is open.
This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.
SPECIMEN: schema-true, not a live event
T0 review · schema-true
One-sentence machine reading of the paper's core claim.
pith:XXXXXXXX · record.json · timestamp
Signed reviews
read the original abstract
We study equations of a non-gauge vector field in a spherically symmetric static metric. The constant vector field with a scale arrangement of components: the time component about the Planck mass m_{Pl} and the radial component about M suppressed with respect to the Planck mass, serves as a source of metric reproducing flat rotation curves in dark halos of spiral galaxies, so that the velocity of rotation v_0 is determined by the hierarchy of scales: \sqrt{2} v_0^2= M/m_{Pl}, and M\sim 10^{12} GeV. A natural estimate of Milgrom's acceleration about the Hubble rate is obtained.
Forward citations
Cited by 2 Pith papers
-
Dark-Matter Induced Scalarization of Black Holes in Extended Scalar-Tensor-Gauss-Bonnet Theories
A spherical black hole immersed in perfect-fluid dark matter becomes unstable to scalar hair for negative Gauss-Bonnet coupling when its dark matter parameter b/M is above 1.86287.
-
Quasinormal modes response to thermodynamic phase transitions in the charged AdS black hole surrounded by perfect fluid dark matter
In charged AdS black holes surrounded by perfect fluid dark matter, the fundamental scalar quasinormal mode jumps between two branches at the first-order small/large black hole transition, stays smooth at the critical...
Discussion (0). Continue with ORCID to comment.