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DOE OSTI ยท 3021125

๐ท-shell mixing in light baryons and its effect on the orbital motion

Abstract

The standard description of the nucleon in the nonrelativistic quark model is an 1S,L = 0 state without orbital motion. Yet, there are several indications from phenomenology that an admixture of states with nonzero orbital motion maybe substantial. In this paper we focus on the โ€œsecond shellโ€ of the nucleon excitations (D-shell), for which we give a modern description of the wave functions. We follow it by investigating what we call a โ€œmaximal mixingโ€ scenario, assuming a hypothetical long-range tensor force. We give the explicit wave functions for all states, before and after mixing, and reassess many predictions such as the magnetic moments, the standard and transitional form-factors from the nucleon to N*. Unexpectedly, in this scenario we can reproduce the long-puzzling features of the Roper resonance N*(1440). But even in this extreme case, the admixture of the 1D,L = 2 state to a nucleon remains significantly smaller than expected from phenomenology.

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BibTeXRIS

Miesch, Nicholas [Stony Brook University, NY (United States)] (ORCID:0000000205937535), Shuryak, Edward [Stony Brook University, NY (United States)], Zahed, Ismail [Stony Brook University, NY (United States)]. 2025-11-04. ๐ท-shell mixing in light baryons and its effect on the orbital motion. https://doi.org/10.1103/b8cp-1pwl

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