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
You also want an ePaper? Increase the reach of your titles
YUMPU automatically turns print PDFs into web optimized ePapers that Google loves.
2.3. Go<strong>in</strong>g to higher energies: a toy model 45<br />
exactly reproduced.21 For example, at NLO one can fix the constants Co and C 2 to reproduce<br />
the scatter<strong>in</strong>g length and the effective range correspond<strong>in</strong>g to the orig<strong>in</strong>al potential (2.112). As<br />
shown <strong>in</strong> table 2.4, both methods give similar results for the coupl<strong>in</strong>g constants.<br />
Let us now make two observations concern<strong>in</strong>g the obta<strong>in</strong>ed results. First, one observes a much<br />
better convergence for the low-energy phase shift with the coupl<strong>in</strong>gs from table 2.4 than with the<br />
true values of Ci ' So This has to be expected, s<strong>in</strong>ce now their values are optimized to obta<strong>in</strong> a good<br />
description for the phase shifts at low-energies or for the effective range parameters and not to<br />
precisely reproduce the true potential for low momenta, which is, <strong>in</strong> pr<strong>in</strong>ciple, not an observable.<br />
<strong>The</strong> same holds also for the two-body b<strong>in</strong>d<strong>in</strong>g energy given <strong>in</strong> table 2.5, which now shows a<br />
much better convergence than with the true values of coupl<strong>in</strong>gs. This <strong>in</strong>dicates that the "f<strong>in</strong>e<br />
tun<strong>in</strong>g" of the coupl<strong>in</strong>g constants may significantly improve the convergence for such "unnatural"<br />
quantities22 like the small b<strong>in</strong>d<strong>in</strong>g energy (or, equivalently, large scatter<strong>in</strong>g length). Indeed, small<br />
changes <strong>in</strong> the values of the Ci's lead to large variations of the b<strong>in</strong>d<strong>in</strong>g energy E, as follows from<br />
the estimation (2.123), and may allow for E to take its correct value already at 'lead<strong>in</strong>g orders.<br />
Secondly, one observes that all Ci'S (with the exception of C�) are with<strong>in</strong> 25% of their exact values.<br />
<strong>The</strong> deviation of the fitted value for C� from the exact one rem<strong>in</strong>ds us of the fact that such f<strong>in</strong>e<br />
tun<strong>in</strong>g can produce sizeable uncerta<strong>in</strong>ties <strong>in</strong> higher orders <strong>in</strong> such type of cut-off schemes and thus<br />
the <strong>in</strong>terpretation of such values has to be taken with so me caution. This is, <strong>in</strong> fact, even a more<br />
deep problem s<strong>in</strong>ce the potential itself is not an observable. Unitary transformations pro duces<br />
phase equivalent potentials without chang<strong>in</strong>g the observables. Although we have found only one<br />
solution for the Ci 's shown <strong>in</strong> table 2.4, fix<strong>in</strong>g the coupl<strong>in</strong>g constants from a fit to phase shifts or,<br />
equivalently, to the first terms <strong>in</strong> the effective range expansion may, <strong>in</strong> general, produce multiple<br />
solutions. An example of such multiple solutions was given <strong>in</strong> section 2.2. <strong>The</strong> precise connection<br />
between the unitarily transformed and effective Hamiltonian is still to be clarified. This might<br />
be quite important for the comparison between various transformed realistic N N <strong>in</strong>teractions<br />
act<strong>in</strong>g only below a certa<strong>in</strong> moment um cut-off and the effective potential derived us<strong>in</strong>g chiral<br />
perturbation theory.<br />
One can also perform a similar analysis for the two-nucleon 1 So channel, which is expected to<br />
be even more troublesome than the 3 SI channel for the effective field theory approach s<strong>in</strong>ce, as<br />
already stated before, the scatter<strong>in</strong>g length takes an unnatural large value. We will not consider<br />
here this case but note that all conclusions drawn above hold also <strong>in</strong> this particular channel. For<br />
more details the <strong>in</strong>terest<strong>in</strong>g reader is referred to reference [124].<br />
To end this section we would like to discuss one furt her issue. In section 2.2 we have considered an<br />
effective theory for two nucleons at very low energies. In such a case even the longest range part<br />
of the nuclear force can be considered as a short range effect. Thus, the effective potential entirely<br />
consists of the contact <strong>in</strong>teractions with <strong>in</strong>creas<strong>in</strong>g number of derivatives. It was demonstrated<br />
that such an effective theory reproduces the effective range expansion but cannot go beyond it.<br />
More precisely, only those first coefficients <strong>in</strong> the effective range expansion are reproduced which<br />
have been used to fix the free parameters of the potential. No predictions for furt her coefficients<br />
could be made. In our current model we have explicitly <strong>in</strong>corporated the long range part of the<br />
underly<strong>in</strong>g <strong>in</strong>teraction <strong>in</strong> the effective Hamiltonian. As a consequence, the predictive power of the<br />
effective theory <strong>in</strong>creases. In table 2.5 we show the values of the b<strong>in</strong>d<strong>in</strong>g energy and effective range<br />
21 At NNLO we obta<strong>in</strong> elose but not exact values of the first four coefficients <strong>in</strong> the effective range expansion.<br />
22 "Unnatural" means <strong>in</strong> this context that the correspond<strong>in</strong>g observable takes a very small or very large value as<br />
the result of a cancelation between some large numbers. For <strong>in</strong>stance, the scatter<strong>in</strong>g length given <strong>in</strong> eq. (2.55) is<br />
natural for all values of the coupl<strong>in</strong>g constant 9 not very elose to one and takes an unnaturally large value if 9 is<br />
accidentally elose to one.