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A new Skyrme interaction with improved spin-isospin properties

Published 17 May 2012 in nucl-th and astro-ph.SR | (1205.3958v2)

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-$\beta$ 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 ${}{48}$Ca, ${}{90}$Zr and ${}{208}$Pb, the Isobaric Analog Resonance and the Spin Dipole Resonance in ${}{90}$Zr and ${}{208}$Pb.

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