Abstract

We discuss the processes $\pi \pi \to \pi \pi$ and $\pi \pi \to \pi \pi \gamma$ from a general quantum field theory (QFT) point of view. In the soft-photon limit where the photon energy $\omega \to 0$ we study the theorem due to F.E. Low. We confirm his result for the $1/\omega$ term of the $\pi \pi \to \pi \pi \gamma$ amplitude but disagree for the $\omega^{0}$ term. We analyse the origin of this discrepancy. Then we calculate the amplitudes for the above reactions in the tensor-pomeron model. We identify places where ``anomalous'' soft photons could come from. Three soft-photon approximations (SPAs) are introduced. The corresponding SPA results are compared to those obtained from the full tensor-pomeron model for c.m. energies $\sqrt{s} = 10$ GeV and 100 GeV. The kinematic regions where the SPAs are a good representation of the full amplitude are determined. Finally we make some remarks on the type of fundamental information one could obtain from high-energy exclusive hadronic reactions without and with soft photon radiation.

Highlights

  • In this paper we shall be concerned with photon emission in some strong-interaction processes

  • In this paper we have studied elastic pion-pion scattering without and with photon radiation

  • Low in [1] but, to our great surprise, our term of order ω0 disagrees with that given in [1]. We have analyzed this important discrepancy and we have shown that our expansion is for the photonemission amplitude satisfying energy-momentum conservation

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Summary

INTRODUCTION

In this paper we shall be concerned with photon emission in some strong-interaction processes. With the present paper we want to start the theoretical study of soft photon emission in exclusive diffractive highenergy reactions in the TeV energy region in the framework of the tensor-Pomeron model. As we shall see, we can in this example compare our “exact” model results for photon emission to approximations based on Low’s theorem which gives the photon-emission amplitude to order ω−1 and ω0 in the photon energy ω for ω → 0. In QFT we can extend the amplitude (2.5) for off shell pions (Fig. 1) This off shell scattering amplitude will still satisfy the energy-momentum conservation (2.3) and can only depend on the following 6 variables sL 1⁄4 pa · pb þ p1 · p2; t 1⁄4 ðpa − p1Þ2 1⁄4 ðpb − p2Þ2; m2a 1⁄4 p2a; m2b 1⁄4 p2b; m21 1⁄4 p21; m22 1⁄4 p22: ð2:6Þ. From (2.11), (2.12), (2.16), (2.19), and (2.20), we obtain kλMðλaÞ 1⁄4 eMð0;aÞ; kλMðλbÞ 1⁄4 −eMð0;bÞ; ð2:21Þ kλMðλcÞ 1⁄4 −eMð0;aÞ þ eMð0;bÞ; ð2:22Þ where Mð0;aÞ and Mð0;bÞ are given explicitly in (2.11) and (2.12), respectively

THE EXPANSION OF THE PHOTON-EMISSION AMPLITUDE
Charged-pion scattering without and with photon radiation
Comparison with the total and elastic ππ cross sections
CONCLUSIONS
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