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Comprehensive investigation of the symmetric space-star configuration in the nucleon-deuteron breakup

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arxiv 2102.09863 v2 pith:I7ELXQ24 submitted 2021-02-19 nucl-th

Comprehensive investigation of the symmetric space-star configuration in the nucleon-deuteron breakup

H. Witala , J. Golak , R. Skibinski , K. Topolnicki , E. Epelbaum , H. Krebs , P. Reinert This is my paper
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We examine a description of available cross section data for symmetric space star (SST) configurations in the neutron-deuteron (nd) and proton-deuteron (pd) breakup reaction using numerically exact solutions of the three-nucleon (3N) Faddeev equation based on two- and three-nucleon (semi)phenomenological and chiral forces. The predicted SST cross sections are very stable with respect to the underlying dynamics for incoming nucleon laboratory energies below $\approx 25$ MeV. We discuss possible origins of the surprising discrepancies between theory and data found in low-energy nd and pd SST breakup measurements.

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    A spectroscopic reparametrization of N4LO contact three-nucleon forces lets nine of thirteen LECs be determined from elastic nucleon-deuteron scattering via an RBF emulator.