Gravitational waves from axisymmetric rotating stellar core collapse to a neutron star in ful

Axisymmetric numerical simulations of rotating stellar core collapse to a nneutron star are performed in the framework of full general relativity. The nso-called Cartoon method, in which the Einstein field equations are solved in nthe Cartesian coordinates and the axisymmetric condition is imposed around the n y=0 plane, is adopted. The hydrodynamic equations are solved in t..