Realistic calculations for c-coefficients of the isobaric mass multiplet equation in 1p0f shell nuclei
Abstract
We present calculations for the c-coefficients of the isobaric mass multiplet equation for nuclei from A=42 to A=54 based on input from three realistic nucleon-nucleon interactions. We demonstrate that there is a clear dependence on the short-ranged charge-symmetry breaking (CSB) part of the strong interaction and that there is significant disagreement in the CSB part between the commonly used CD-Bonn, N3LO, and Argonne V18 nucleon-nucleon interactions. In addition, we show that all three interactions give a CSB contribution to the c-coefficient that is too large when compared to experiment.
Turn this paper into a lesson
ArcXiv compiles a structured reading guide from this paper's metadata: plain-English importance, contributions, prerequisite concepts, which sections to read first, flashcards, and a quiz. Grounded in the abstract, never invented.