In this thesis, using the new model of anomalous viscosity, we discuss the structure of magnetized thin accretion disks, the magnetic instability in the accretion disks and.
Structure is the carrier of the function, in order to explore whether there are anomalous structural connections in SAD, we studied the structural network of SAD by DTI.
There is anomalousness in a neutrino as well, and the anomalous quantities are the inevitable outcome of the dynamical model of the subquark structure of a lepton.