Electromagnetic Mass Splittings of theNandN*(1238 MeV)

Abstract
We examine the Dashen-Frautschi calculation of the neutron-proton mass difference δn,p. Their SU(2) calculation considers the nucleon to be a πN bound state with the dominant forces due to nucleon and N*(1238MeV) exchange. δn,p then depends linearly on δ,++ (the mass difference between the N*'s with charges - and + +) and the one-photon-exchange driving term Γ. [We note that this SU(2) model predicts δ0,+=13δ,++.] The N* is calculated as a πN resonance with N and N* exchange as the forces. This gives another relation among δ,++, δn,p, and Γ. Now in the static Chew-Low theory with a linear D function the NN* reciprocal bootstrap conditions on the residues are exactly satisfied. In this case we show that δn,p (and δ,++) is infinite. (Following Gerstein and Whippman, this divergence is seen to be a general consequence of the static, linear-D, reciprocal bootstrap conditions.) Thus it is only the deviations from the static Chew-Low theory with linear D which give a finite δn,p. Dashen and Frautschi consider two such effects: (a) They show that the N* exchange force is suppressed (by a factor of 0.6) because of the detailed shape of the resonance. (b) The physical D function must approach a constant at high energy, and they choose the simple rational form D(WM)(W7M3) for the P11 partial wave which simulates the D function calculated by Balázs. This choice for D leads to an additional suppression of the N* exchange force. We concentrate our criticism on the nature of the D function. We note that the Balázs D function corresponds to a P11 partial wave with a negative definite phase shift, in contradiction to experiment. Using results of πN phase-shift analyses, we calculate the D functions and find that the N* exchange contribution to the binding of the nucleon is enhanced relative to the linear form for D. Depending on the high-energy behavior of these phase shifts, not only can the calculated δn,p have the wrong magnitude, but also the wrong sign. We conclude that the calculation of δn,p depends critically on the details of the strong interactions. On the other hand, the ratio δ,++δn,p is insensitive to these details and is predicted to be Å3. Thus a less ambitious point of view is to use the experimental value of δ,++(=7.9±6.8 MeV) to get a rough value of δn,p (or vice versa).