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A new Skyrme interaction with improved spin-isospin properties

Abstract

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\beta 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 48{}^{48}Ca, 90{}^{90}Zr and 208{}^{208}Pb, the Isobaric Analog Resonance and the Spin Dipole Resonance in 90{}^{90}Zr and 208{}^{208}Pb.Comment: Predictions on the IAR and SDR and comparison with the SGII interaction for the GTRs where adde

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