A correct determination of the spin-isospin properties of the nuclear
effective interaction should lead, among other improvements, to an accurate
description of the Gamow-Teller Resonance (GTR). These nuclear excitations
impact on a variety of physical processes: from the response in charge-exchange
reactions of nuclei naturally present in the Earth, to the description of the
stellar nucleosynthesis, and of the pre-supernova explosion core-collapse
evolution of massive stars in the Universe. A reliable description of the GTR
provides also stringent tests for neutrinoless double-β decay
calculations. We present a new Skyrme interaction as accurate as previous
forces in the description of finite nuclei and of uniform matter properties
around saturation density, and that account well for the GTR in 48Ca,
90Zr and 208Pb, the Isobaric Analog Resonance and the Spin Dipole
Resonance in 90Zr and 208Pb.Comment: Predictions on the IAR and SDR and comparison with the SGII
interaction for the GTRs where adde