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The Nucleon-Nucleon Interaction in a Chiral Effective Field Theory

The Nucleon-Nucleon Interaction in a Chiral Effective Field Theory

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5.1 Isosp<strong>in</strong> violat<strong>in</strong>g effective Lagrangian 153<br />

unnaturally large S-wave scatter<strong>in</strong>g lengths. This can be dealt with <strong>in</strong> different manners. One<br />

is the approach proposed by We<strong>in</strong>berg, <strong>in</strong> which chiral perturbation theory is applied to the<br />

kernel of the Lippmann-Schw<strong>in</strong>ger equation (effective potential). This approach is very similar<br />

to the Hamiltonian formalism used <strong>in</strong> this work and expla<strong>in</strong>ed <strong>in</strong> detail <strong>in</strong> chapter3. This route<br />

was followed by van Kolck et al. , see refs [75], [74], [76], [78]. A different fashion to deal with<br />

low-energy nucleon-nucleon scatter<strong>in</strong>g is the approach recently proposed by Kaplan, Savage and<br />

Wise (KSW) [91].2 Essentially, one resums the lowest order local four-nucleon contact terms rv<br />

Co (Nt N)2 (<strong>in</strong> the S-waves) to generate the large scatter<strong>in</strong>g lengths and treats the rema<strong>in</strong><strong>in</strong>g effects<br />

perturbatively, <strong>in</strong> particular also pion exchange. This means that most low-energy observables<br />

are dom<strong>in</strong>ated by contact <strong>in</strong>teractions. <strong>The</strong> chiral expansion for NN scatter<strong>in</strong>g entails a new<br />

scale ANN of the order of 300 MeV, so that one can systematically treat external momenta up<br />

to the size of the pion mass. <strong>The</strong>re have been suggestions that the radius of convergence can<br />

be somewhat enlarged [88], but <strong>in</strong> any case ANN is considerably sm aller than the typical scale of<br />

about 1 Ge V appear<strong>in</strong>g <strong>in</strong> the pion-nucleon sector . For recent calculations of various properties of<br />

the two-nucleon system with<strong>in</strong> this formalism see e.g. refs. [87], [88], [92], [95], [98], [210], [211]. In<br />

this context, it appears to be particularly <strong>in</strong>terest<strong>in</strong>g to study CIB (or <strong>in</strong> general isosp<strong>in</strong> violation)<br />

which is believed to be dom<strong>in</strong>ated by long range pion effects. That is done here.3 First, we write<br />

down the lead<strong>in</strong>g strong and electromagnetic four-nucleon contact terms. It is important to note<br />

that <strong>in</strong> contrast to the pion or pion-nucleon sector, one can not easily lump the expansion <strong>in</strong><br />

small momenta and the electromagnetic coupl<strong>in</strong>g <strong>in</strong>to one expansion but rat her has to treat them<br />

separately.4 <strong>The</strong>n we consider <strong>in</strong> detail CIB. <strong>The</strong> lead<strong>in</strong>g effect starts out at order aQ-2, where Q<br />

is the generic expansion parameter <strong>in</strong> the KSW approach. It sterns from OPE plus a contact term<br />

of order a with a coefficient aE� l ) of natural size that scales as Q-2. Similarly, the lead<strong>in</strong>g CSB<br />

effect results from contact terms with four nucleon legs of order a and order E == mu - md, which<br />

also scale as Q-2. While <strong>in</strong> the case of E�l) this scal<strong>in</strong>g property is enforced by a cancellation<br />

of a divergence, the situation is a priori different for CSB. However, for a consistent count<strong>in</strong>g of<br />

all isosp<strong>in</strong> break<strong>in</strong>g effects related to strong or electromagnetic (ern) <strong>in</strong>sertions, one should count<br />

the quark mass difference and virtual photon effects similarly. Note, however, that these CIB and<br />

eSB terms are numerically much smaller than the lead<strong>in</strong>g strong contributions which scale as<br />

Q-l because a« 1 and (mu - md)/Ax «1. <strong>The</strong> correspond<strong>in</strong>g constants, which we call E�1,2),<br />

together with the strong parameters (as given <strong>in</strong> the work of KSW) can be determ<strong>in</strong>ed by fitt<strong>in</strong>g<br />

the three scatter<strong>in</strong>g lengths a pp , ann, an p and the np effective range.5 That allows to predict the<br />

moment um dependence of the np and the nn 1 So phase shifts. Based on these observations, we<br />

can <strong>in</strong> addition give a general classification for the relevant operators contribut<strong>in</strong>g to eIB and<br />

eSB <strong>in</strong> this scheme. Additional work related to long-range Coulomb photon exchange is necessary<br />

<strong>in</strong> the proton-proton system. We do not deal with this issue here but refer to recent work us<strong>in</strong>g<br />

EFT approaches <strong>in</strong> refs. [219] , [220], [221].<br />

5.1 Isosp<strong>in</strong> violat<strong>in</strong>g effective Lagrangian<br />

Let us first discuss the various parts of the effective Lagrangian underly<strong>in</strong>g the analysis of isosp<strong>in</strong><br />

violation <strong>in</strong> the two-nucleon system. To <strong>in</strong>clude virtual photons <strong>in</strong> the pion and the pion-nucleon<br />

2 <strong>The</strong>re exist by now modifications of this approach and it has been argued that it is equivalent to cut-off schemes.<br />

We do not want to enter this discussion here but rather stick to its orig<strong>in</strong>al version.<br />

3For a first look at these effects <strong>in</strong> an EFT framework (based on the We<strong>in</strong>berg power count<strong>in</strong>g) , see the work of<br />

van Kolck [75]. Electromagnetic corrections to the one-pion exchange potential have been considered <strong>in</strong> [218].<br />

4 This is because of the different power count<strong>in</strong>g schemes <strong>in</strong> these cases.<br />

5Whenever we talk of the pp system, we assume that the Coulomb effects have been subtracted.

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