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Numerical Approach to the Low-Energy Bootstrap
Phys. Rev. D 1, 217 – Published 1 January, 1970
DOI: https://doi.org/10.1103/PhysRevD.1.217
Abstract
The amplitude in the low-energy region is parametrized in a crossing-symmetric way as the sum of the and resonance poles plus a polynomial background. The parametrization is flexible and capable of producing amplitudes having quite different features in the energy region below 1 GeV. The parameters are then varied so as to minimize the deviation from elastic unitarity on a set of closely spaced points. In addition, negative-moment finite-energy sum rules are used to connect the low-energy region with assumed Regge asymptotic behavior in the amplitudes. With the mass and width of the , the mass of the , and the slope of the trajectory fixed, an approximate solution satisfying the constraints is found, yielding a width of 80± 30 MeV. The solution displays the usual characteristics of the low-energy amplitudes suggested by other analyses, namely, small scattering lengths and a large -wave phase shift near the mass of the . This resonantlike behavior is found without introducing an -wave pole in the parametrization, while the small scattering lengths are obtained as results of the numerical bootstrap, although no current-algebra constraints are included. Our proposed solution is also found to satisfy various inequalities proposed by Martin for the scattering amplitude.
References (16)
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