activity
19962018
most citedClusters of galaxies with modified Newtonian dynamics (MOND)

226 citations · 1.3k across the 17 of their papers we have counts for

collaborators

17 papers

astro-ph.GA2018★ 25 cited

The prediction of rotation curves in gas-dominated dwarf galaxies with modified dynamics

R. H. Sanders

I consider the observed rotation curves of 12 gas-dominated low-surface-brightness galaxies -- objects in which the mass of gas ranges between 2.2 and 27 times the mass of the stel…

astro-ph.GA2011★ 27 cited

NGC 2419 does not challenge MOND

R. H. Sanders

I show that, in the context of MOND, non-isothermal models, approximated by high order polytropic spheres, are consistent with the observations of the radial distribution of the li…

gr-qc2011★ 25 cited

Hiding Lorentz Invariance Violation with MOND

R. H. Sanders

Hořava gravity is a attempt to construct a renormalizable theory of gravity by breaking the Lorentz Invariance of the gravitational action at high energies. The underlying principl…

astro-ph.CO2010★ 61 cited

The Universal Faber-Jackson Relation

R. H. Sanders

In the context of modified Newtonian dynamics, the fundamental plane, as the observational signature of the Newtonian virial theorem, is defined by high surface brightness objects…

astro-ph2008★ 37 cited

MOND and the lensing Fundamental Plane: No need for dark matter on galaxy scales

R. H. Sanders, D. D. Land

Bolton et al. (2007) have derived a mass-based fundamental plane using photometric and spectroscopic observations of 36 strong gravitational lenses. The lensing allows a direct det…

astro-ph2007★ 68 cited

Neutrinos as cluster dark matter

R. H. Sanders

The dynamical mass of clusters of galaxies, calculated in terms of modified Newtonian dynamics, is a factor of two or three times smaller than the Newtonian dynamical mass but rema…