9 research outputs found

    Charge-Dependence of the Nucleon-Nucleon Interaction

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    Based upon the Bonn meson-exchange-model for the nucleon-nucleon (NNNN) interaction, we calculate the charge-independence breaking (CIB) of the NNNN interaction due to pion-mass splitting. Besides the one-pion-exchange (OPE), we take into account the 2π2\pi-exchange model and contributions from three and four irreducible pion exchanges. We calculate the CIB differences in the 1S0^1S_0 effective range parameters as well as phase shift differences for partial waves up to total angular momentum J=4 and laboratory energies below 300 MeV. We find that the CIB effect from OPE dominates in all partial waves. However, the CIB effects from the 2π2\pi model are noticable up to D-waves and amount to about 40% of the OPE CIB-contribution in some partial waves, at 300 MeV. The effects from 3π\pi and 4π\pi contributions are negligible except in 1S0^1S_0 and 3P2^3P_2.Comment: 12 pages, RevTex, 14 figure

    Chiral 2pi exchange at order four and peripheral NN scattering

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    We calculate the impact of the complete set of two-pion exchange contributions at chiral order four (also known as next-to-next-to-next-to-leading order, N3LO) on peripheral partial waves of nucleon-nucleon scattering. Our calculations are based upon the analytical studies by Kaiser. It turns out that the contribution of order four is substantially smaller than the one of order three, indicating convergence of the chiral expansion. We compare the prediction from chiral pion-exchange with the corresponding one from conventional meson-theory as represented by the Bonn Full Model and find, in general, good agreement. Our calculations provide a sound basis for investigating the issue whether the low-energy constants determined from pi-N lead to reasonable predictions for NN.Comment: 22 pages RevTex including 11 figure

    Deconstructing 1S0 nucleon-nucleon scattering

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    A distorted-wave method is used to analyse nucleon-nucleon scattering in the 1S0 channel. Effects of one-pion exchange are removed from the empirical phase shift to all orders by using a modified effective-range expansion. Two-pion exchange is then subtracted in the distorted-wave Born approximation, with matrix elements taken between scattering waves for the one-pion exchange potential. The residual short-range interaction shows a very rapid energy dependence for kinetic energies above about 100 MeV, suggesting that the breakdown scale of the corresponding effective theory is only 270MeV. This may signal the need to include the Delta resonance as an explicit degree of freedom in order to describe scattering at these energies. An alternative strategy of keeping the cutoff finite to reduce large, but finite, contributions from the long-range forces is also discussed.Comment: 10 pages, 2 figures (introduction revised, references added; version to appear in EPJA

    Charge-Asymmetry of the Nucleon-Nucleon Interaction

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    Based upon the Bonn meson-exchange model for the nucleon-nucleon (NNNN) interaction, we study systematically the charge-symmetry-breaking (CSB) of the NNNN interaction due to nucleon mass splitting. Particular attention is payed to CSB generated by the 2π2\pi-exchange contribution to the NNNN interaction, πρ\pi\rho diagrams, and other multi-meson-exchanges. We calculate the CSB differences in the 1S0^1S_0 effective range parameters as well as phase shift differences in SS, PP and higher partial waves up to 300 MeV lab. energy. We find a total CSB difference in the singlet scattering length of 1.6 fm which explains the empirical value accurately. The corresponding CSB phase-shift differences are appreciable at low energy in the 1S0^1S_0 state. In the other partial waves, the CSB splitting of the phase shifts is small and increases with energy, with typical values in the order of 0.1 deg at 300 MeV in PP and DD waves.Comment: 11 pages, RevTex, 14 figure

    Nucleon-Nucleon Optical Model for Energies to 3 GeV

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    Several nucleon-nucleon potentials, Paris, Nijmegen, Argonne, and those derived by quantum inversion, which describe the NN interaction for T-lab below 300$ MeV are extended in their range of application as NN optical models. Extensions are made in r-space using complex separable potentials definable with a wide range of form factor options including those of boundary condition models. We use the latest phase shift analyses SP00 (FA00, WI00) of Arndt et al. from 300 MeV to 3 GeV to determine these extensions. The imaginary parts of the optical model interactions account for loss of flux into direct or resonant production processes. The optical potential approach is of particular value as it permits one to visualize fusion, and subsequent fission, of nucleons when T-lab above 2 GeV. We do so by calculating the scattering wave functions to specify the energy and radial dependences of flux losses and of probability distributions. Furthermore, half-off the energy shell t-matrices are presented as they are readily deduced with this approach. Such t-matrices are required for studies of few- and many-body nuclear reactions.Comment: Latex, 40 postscript pages including 17 figure
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