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Numerical Approach to the Low-Energy ππ Bootstrap

Farzam Arbab* and J. T. Donohue

  • Brookhaven National Laboratory, Upton, New York 11973

  • *Present address: Physics Department, University of the Valley, Cali, Colombia.

Phys. Rev. D 1, 217 – Published 1 January, 1970

DOI: https://doi.org/10.1103/PhysRevD.1.217

Abstract

The ππ amplitude in the low-energy region is parametrized in a crossing-symmetric way as the sum of the ρ and f0 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 I=1, 2 amplitudes. With the mass and width of the f0, the mass of the ρ, and the slope of the ρ trajectory fixed, an approximate solution satisfying the constraints is found, yielding a ρ width of 80± 30 MeV. The solution displays the usual characteristics of the low-energy ππ amplitudes suggested by other analyses, namely, small scattering lengths and a large I=0 S-wave phase shift near the mass of the ρ. This resonantlike behavior is found without introducing an S-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 π0π0 scattering amplitude.

References (16)

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  10. Weinberg, [1] Proceedings of the Fourteenth International Conference on High-Energy Physics, Vienna 1968, edited by J. Prentki and J. Steinberger (CERN, Geneva, 1968), p. 253
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  16. Omitted endnote

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