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444 Strong Interactions<br />

already been given in Section 14.4. In particular, for a point nucleon at position<br />

x = 0, it is the Yukawa potential, Eq. (14.24). The nucleon acts as a source of the<br />

meson field and<br />

g<br />

Φ(x) =−<br />

(�c) 1/2 mc<br />

exp(−kr), r = |x|, k = , (14.42)<br />

r �<br />

is the field produced at x by a point nucleon sitting at the origin. The interaction<br />

energy between this and a second point nucleon at position x is found by inserting<br />

Eq. (14.42) into Eq. (14.39) and by using the fact that ρ(x) now also describes a<br />

point nucleon. The interaction energy then becomes<br />

Vs = −g 2 �c exp(−kr)<br />

. (14.43)<br />

r<br />

The negative sign means attraction and two nucleons consequently attract each<br />

other if the force is produced by a neutral scalar meson.<br />

Pions are pseudoscalar and not scalar particles, although the latter appear in<br />

the meson exchange potentials used to fit data. (25) As the next step, we therefore<br />

consider the contribution from a neutral pseudoscalar meson. Looking through<br />

the list at PDG indicates that η, with a mass of 549 MeV/c2 , is such a particle.<br />

The interaction Hamiltonian is very similar to the one given in Eq. (14.16); for an<br />

isoscalar particle, this relation simplifies to<br />

�<br />

Hp = F d 3 xρ(x)σ · ∇Φ. (14.44)<br />

The free pseudoscalar meson is also described by the Klein–Gordon equation, Eq.<br />

(14.44), because it is not possible to distinguish between free scalar and pseudoscalar<br />

particles. For the meson field in the presence of a nucleon, Eqs. (14.44) and (14.40)<br />

together yield �<br />

∇ 2 −<br />

�<br />

mc<br />

� �<br />

2<br />

�<br />

Φ=− 4π<br />

�2 F σ ·∇ρ(x). (14.45)<br />

c2 This equation is solved as in Section 14.4. Inserting the solution into Eq. (14.44)<br />

then gives, for the potential energy due to the exchange of the neutral pseudoscalar<br />

meson between point nucleons A and B,<br />

2 F<br />

Vp =<br />

�2c2 (σA ·∇)(σB ·∇) exp(−kr)<br />

. (14.46)<br />

r<br />

The differentiations can be performed, and the final result is (25,30)<br />

2 F<br />

Vp =<br />

�2c2 �<br />

1<br />

3 σA<br />

�<br />

1 1 1<br />

· σB + SAB + +<br />

3 kr (kr) 2<br />

��<br />

2 exp(−kr)<br />

× k , (14.47)<br />

r<br />

30Details can be found in L. R. B. Elton, Introductory Nuclear Theory, 2nd ed, Saunders,<br />

Philadelphia, 1966, Section 10.3. Vp, as given in Eq. (14.47), is not complete; a term proportional<br />

to δ(r) is missing. The omission is unimportant because the short-range repulsion between nucleons<br />

makes the term ineffective.

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