With the use of a dispersion relation and a high-energy cutoff, the model involving 7r, p, co, 7] v , f, and a (0 + , 7 = 0, 416 MeV) is studied for nucleon-nucleon interactions below 3 GeV. All nucleon-nucleon elastic-scattering data and those for p-p collisions at 0.67, 0.97, and 1.4 GeV are in qualitative agreement with the calculations.While the one-boson-exchange model (OBEM) 1 was found to be successful in describing nucleonnucleon interactions at an internucleon distance larger than 0.5ii^' 1 , there was difficulty in explaining the S-wave phase shifts which essentially represent the interaction at the smaller distance. In our recent works, however, we have introduced a nucleon-meson form factor into the OBEM, taking into account the IT, p, co, rj v [0 + , 7 = 0, m(7? y ) = 1070 MeV], and a [0 + , 7 = 0, m(a) = 416 MeV], and showed that the S-wave phase shifts can be reproduced as well as other phase shifts associated with higher partial waves. 2 ' 3 As is well known, the X S 0 phase shift becomes negative at energies higher than about 250 MeV, representing the repulsive interaction at a close internucleon distance. In our works 2 * 3 this has been explained in terms of the vectormeson-exchange (especially co-exchange) contribution.However there is criticism against it. There are some other mesons with higher spin and heavier mass whose exchange gives forces with the opposite sign to that for the vector meson. The/ embodies just such a property. 4 Consequently there is a possibility that the repulsive interaction arising from the vector-meson exchange might be canceled by the /.In this Letter we consider an OBEM including the / in addition to the 77, p, co, r) v , and a. These are all established mesons except for the a. The a is used as a fitting device taking care of the L = 7 = 0 two-pion-state part of the two-pion-exchange contribution. 5 We calculate phase shifts of the 1 S 0 , 3 P 0>lt2 , and 1 D 2 states for the 0-to 3-GeV energy range, employing a partial-wave dispersion relation which includes absorption effects. 6 For the calculation of the 3 P 2 phase shift a coupling effect between the 3 P 2 and 3 F 2 states is neglected. This approximation gives an error of a few percent in the phase shift, which is estimated by the damping relation. 1 Thus let us consider an uncoupled scattering of nucleons with mass m, energy E, and momentum/? in the center-of-mass system. Define a scattering amplitude for a state specified by J with the phase shift 6j(s) and an absorption coefficient rjj(s):where s -4E 2 . Pj(s) is a kinematical factor chosen, for reasonable threshold behavior, as pj(s) = m{p/E) n , where n = 1 for the 1 S 0 and 3 P 0 , 1|2 states and n = 3 for the 1 D 2 state. With the N/D method applied to the Aj(s), the following integral equation for the ReN is derived 6 : 1 + vAs)where s E~A m 2 , and(3)Here Bj(s) is a left-hand-cut integral term and the second term comes from the absorption effects. {Sj corresponds to the inelastic threshold.) With Bj(s) and rjj(s) given, Eq.(2) can be solved by a num...