1976
DOI: 10.1016/0550-3213(76)90116-4
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Radiative corrections to low-energy ππ scattering

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Cited by 11 publications
(16 citation statements)
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“…If one therefore directly compares the processes e + e − → π + π − (γ) and e + e − → µ + µ − (γ), one is only sensitive to the difference (1/M π ± ) log(∆E/M π ± )−(1/M µ ) log(∆E/M µ ) which reduces the dependence on the detector resolution by almost one order of magnitude. Another way of proceeding is to follow the arguments which have been used in the discussion of ππ scattering [32,10]. While the cross section of course depends on the detector resolution and so does the scattering length a, dσ/dΩ = |a| 2 , one can define an electromagnetically corrected scattering length which is independent of ∆E.…”
Section: Vector Form Factor and Pion Charge Radiusmentioning
confidence: 99%
“…If one therefore directly compares the processes e + e − → π + π − (γ) and e + e − → µ + µ − (γ), one is only sensitive to the difference (1/M π ± ) log(∆E/M π ± )−(1/M µ ) log(∆E/M µ ) which reduces the dependence on the detector resolution by almost one order of magnitude. Another way of proceeding is to follow the arguments which have been used in the discussion of ππ scattering [32,10]. While the cross section of course depends on the detector resolution and so does the scattering length a, dσ/dΩ = |a| 2 , one can define an electromagnetically corrected scattering length which is independent of ∆E.…”
Section: Vector Form Factor and Pion Charge Radiusmentioning
confidence: 99%
“…Finally, electromagnetic corrections to low energy π − π scattering within different contexts and/or frameworks have been considered previously in Refs. [27], [28] and [29]. Unless otherwise stated, we shall work within the framework of standard chiral perturbation theory, where (1.1) is assumed to hold.…”
Section: Introductionmentioning
confidence: 99%
“…Once this is done, the corrected scattering length a 0 (+−; 00) might be defined from the threshold expansion of the infrared finite cross-section, eq. (5.9), by subtracting the Coulomb pole term and excluding the corrections due to the mass squared differences in the phase-space in the following way [25] σ(s; ∆E) = 1 32πs…”
Section: Soft Photon Contributionmentioning
confidence: 99%