The Nucleon-Nucleon Interaction in a Chiral Effective Field Theory
The Nucleon-Nucleon Interaction in a Chiral Effective Field Theory
The Nucleon-Nucleon Interaction in a Chiral Effective Field Theory
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100 3. <strong>The</strong> derivation o{ nuc1ear {orces {rom chiral Lagrangians<br />
respectively. Note that Vl�: 1-1oop,red. aga<strong>in</strong> conta<strong>in</strong>s a term rv l/wg. Comb<strong>in</strong><strong>in</strong>g eqs. (3.274) and<br />
(3.280), this unphysical contribution vanishes. Summ<strong>in</strong>g up the corrections eqs. (3.274), (3.276)<br />
correspond<strong>in</strong>g to irreducible graphs, which are aga<strong>in</strong> the same as <strong>in</strong> old-fashioned time-dependent<br />
perturbation theory and those (3.280), (3.281), correspond<strong>in</strong>g to "reducible" diagrams, one gets<br />
the complete result, represent<strong>in</strong>g the one-Ioop contributions, which <strong>in</strong>volve self-energy <strong>in</strong>sert ions<br />
and vertex corrections with<strong>in</strong> the projection formalism:<br />
Vb,1-1oop<br />
(2)<br />
VNN,1-1oop<br />
(2)<br />
<strong>The</strong> complete potential at NLO <strong>in</strong> the projection formalism is given by the express ions (3.270),<br />
(3.279), (3.282) and (3.283). <strong>The</strong> formal expressions for the NN potential shown above conta<strong>in</strong><br />
ultraviolet divergences. In the next section we will show how such ultraviolet divergences can be<br />
removed by redef<strong>in</strong>ition of the coupl<strong>in</strong>g constants.<br />
Let us briefly discuss the NNLO potential given <strong>in</strong> eq. (3.255). <strong>The</strong> related diagrams are shown<br />
<strong>in</strong> fig. 3.15. In that case no purely nucleonic <strong>in</strong>termediate states are possible. Correspond<strong>in</strong>gly,<br />
one obta<strong>in</strong>s the same contributions <strong>in</strong> time-ordered perturbation theory and <strong>in</strong> the projection<br />
formalism. This is also evident from the explicit form of the operators <strong>in</strong> eq. (3.255). <strong>The</strong> formal<br />
express ions of the NNLO potential were presented <strong>in</strong> [78]. In the next section we will show the<br />
renormalized contributions given by Kaiser et al. [108].<br />
F<strong>in</strong>ally, let us po<strong>in</strong>t out once more that the crucial difference between the two formalisms, timeordered<br />
perturbation theory and method of unitary transformation, results <strong>in</strong> the treatment of the<br />
energy-dependent term eq. (3.277). As already noted ab ove , it does not appear <strong>in</strong> the method of<br />
unitary transformation. We note that many of the results derived here have already been found <strong>in</strong><br />
[108], where one- and two-pion exchange graphs were calculated by me ans of Feynman diagrams<br />
and us<strong>in</strong>g dimensional regularization. <strong>The</strong> potential was applied to N N scatter<strong>in</strong>g <strong>in</strong> peripheral<br />
partial waves (with orbital angular momentum L 2: 2), where it does not need to be iterated.<br />
Our aim is to apply this potential to all partial waves and to the bound state problem. We will<br />
comment more on that <strong>in</strong> the next chapter.<br />
3.8.2 Renormalization of the N N potential at NLO<br />
<strong>The</strong> effective N N potential at NLO derived <strong>in</strong> the last section is not well-def<strong>in</strong>ed, s<strong>in</strong>ce it conta<strong>in</strong>s<br />
ultraviolet divergent <strong>in</strong>tegrals. Here, we would like to show how to renormalize this potential.<br />
S<strong>in</strong>ce we are deal<strong>in</strong>g with an effective field theory, we can use the standard order-by-order<br />
renormalization mach<strong>in</strong>ery for the Lagrangian, which was first developed <strong>in</strong> the context of chiral<br />
perturbation theory. All these divergent contributions (at NLO) can be renormalized <strong>in</strong> terms of<br />
three divergent (momentum space) loop functions,41<br />
/00 dl<br />
Jo = (3.284)<br />
J1 T'<br />
41 Clearly, all ultraviolet divergent <strong>in</strong>tegrals here and <strong>in</strong> what follows have to be understood as the limits A -+ 00<br />
of the correspond<strong>in</strong>g <strong>in</strong>tegrals over the f<strong>in</strong>ite range of momenta 0 < I < A.