From chiral NN(N) interactions to giant and pygmy resonances via extended RPA
arXiv:1704.08429 · doi:10.5506/APhysPolB.48.537
Abstract
The properties of giant and pygmy resonances are calculated starting from chiral two-and three-nucleon interactions. The aim is to assess the predictive power of modern Hamiltonians and especially the role of the three-nucleon force. Methods based on the random-phase approximation (RPA) provide an optimal description of the modes of interest with minimal computational requirements. Here we discuss the giant resonances (GRs) of 40,48Ca isotopes and their low-energy dipole response. A comparison with previous results obtained with a transformed Argonne V18 two-nucleon potential points to certain improvements.
4 pages, 1 figure; from a talk at the 2016 Zakopane Conference on Nuclear Physics, September 2016