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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Chapter 5<br />
Isosp<strong>in</strong> violation <strong>in</strong> the two-nucleon<br />
system<br />
In this chapter we would like to discuss charge symmetry and charge <strong>in</strong>dependence break<strong>in</strong>g <strong>in</strong><br />
an effective field theory approach for few-nucleon systems. In particular, we will concentrate on<br />
the 1 So channel, <strong>in</strong> which the largest isosp<strong>in</strong> violat<strong>in</strong>g effects are observed. Further , we will use<br />
the formalism proposed by Kaplan, Savage and Wise (KSW) [91] throughout this chapter.<br />
It is weIl established that the nucleon-nucleon <strong>in</strong>teractions are charge dependent (for a review, see<br />
e.g. [216] ). For example, <strong>in</strong> the ISO channel one has for the scatter<strong>in</strong>g lengths a and the effective<br />
ranges r (n and p refers to the neutron and the proton, respectively)<br />
.6.rcIB<br />
1<br />
2" (ann + app) - anp = 5.7 ± 0.3 fm ,<br />
1<br />
2" (rnn + rpp) - rnp = 0.05 ± 0.08 fm . (5.1)<br />
<strong>The</strong>se numbers for charge <strong>in</strong>dependence break<strong>in</strong>g (CIB) are based on the Nijmegen potential<br />
and the Coulomb effect for pp scatter<strong>in</strong>g is subtracted based on standard methods.1 <strong>The</strong><br />
charge <strong>in</strong>dependence break<strong>in</strong>g <strong>in</strong> the scatter<strong>in</strong>g lengths is large, of the order of 25%, s<strong>in</strong>ce<br />
anp = (-23.714 ± 0.013) fm. In addition, there are charge symmetry break<strong>in</strong>g (CSB) effects<br />
lead<strong>in</strong>g to different values for the pp and nn threshold parameters,<br />
.6.acsB<br />
.6.rcsB<br />
app - ann = 1.5 ± 0.5 fm ,<br />
rpp - rnn = 0.10 ± 0.12 fm . (5.2)<br />
Both the CIB and CSB effects have been studied <strong>in</strong>tensively with<strong>in</strong> potential models of the<br />
nucleon-nucleon (NN) <strong>in</strong>teractions. In such approaches, the dom<strong>in</strong>ant CIB comes from the charged<br />
to neutral pion mass difference <strong>in</strong> the one-pion exchange (OPE), rv .6.agrBE 3.6±0.2 fm. Additional<br />
contributions come from 17f and 27f (TPE) exchanges. Note also that the charge dependence <strong>in</strong> the<br />
pion-nucleon coupl<strong>in</strong>g constants <strong>in</strong> OPE and TPE almost entirely cancel. In the meson-exchange<br />
picture, CSB orig<strong>in</strong>ates mostly from p - w mix<strong>in</strong>g, .6.a�s� rv 1.2 ± 0.4 fm. Other contributions due<br />
to 7r - 7], 7f - 7] ' mix<strong>in</strong>g or the proton-neutron mass difference are known to be much smaller.<br />
With<strong>in</strong> QCD, CSB and CIB are of course due to the different masses and charges of the up and<br />
down quarks. Such isosp<strong>in</strong> violat<strong>in</strong>g effects can be systematically analyzed with<strong>in</strong> the framework<br />
of chiral effective field theories. In the two-nucleon sector, a complication arises due to the<br />
1 In particular, the magnetic <strong>in</strong>ter action had also been to be considered.<br />
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