The cosmological principle (CP)—the notion that the Universe is spatially isotropic and
homogeneous on large scales—underlies a century of progress in cosmology. It is …

Based on a new sample of 355 quasars with significant optical polarization and using
complementary statistical methods, we confirm that quasar polarization vectors are not …

We have conducted an image analysis of the (current) full sample of 44 spiral galaxies with
directly measured supermassive black hole (SMBH) masses, M BH, to determine each …

We present the results of a search for galaxy clusters that show an indication of global
rotation using a spectroscopic sample of galaxies in SDSS and 2dFGRS. We have …

Models of a rotating universe have been studied widely since the work of Gödel, who
showed an example that is consistent with general relativity. By now, the possibility of a …

Elaborating on an old conjecture by Blackett, we formulate a new conjecture about the
neutrality of matter according to which any physical system possesses an active electric …

In this paper we discussed the observational aspects of rotation in the Universe on different
scales. We show dependence between the angular momentum of the structures and their …

A step-by-step foundation for the differential character of the Universe's rotation is presented.
First, invoking the concept of spacetime foam with spin, it is reasonable to assume that the …

We further develop the gravitational model, Thomas-Whitehead gravity (TW Gravity), that
arises when projective connections become dynamical fields. TW Gravity has its origins in …

An overview of the cosmological models with expansion, shear and rotation is presented.
Problems of the rotating models are discussed, their general kinematic properties and …