Summary
We found that the Regge-pole parameters obtained through a sum-rule integral over the low-energy πN data (phase shifts up toT π=1.3 GeV) and over the σ-pole contribution in thet-channel, nearu=0, are compatible with the available Regge parameters obtained at high energy. In particular in the interval fromu=0.1 to −0.35 (GeV)2 we predict a zero in the scattering amplitude associated with the nucleon (N α) trajectory exchange and no zero in the scattering amplitude associated with Δ exchange. The coupling of theN γ trajectory is weak throughout this region.
Riassunto
Si trova che i parametri dei poli di Regge ottenuti integrando la regola di somma rispetto ai dati di πN di bassa energia (spostamenti di fase fino aT π=1.3 GeV) e al contributo del polo σ nel canalet, vicino au=0, sono compatibili con i parametri di Regge disponibili ottenuti ad alta energia. In particolare, nell'intervallo dau=0.1 a −0.35 (GeV)2 si predice uno zero nell'ampiezza di scattering associata allo scambio di traiettoria del nucleone (N α) e nessuno zero nell'ampiezza d'urto associata allo scambio di Δ. In tutta questa regione l'accoppiamento della traiettoriaN γ è debole.
Резюме
Мы нашли, что параметры полюсов Редже, полученные с помощью интеграла правила сумм из πN данных при малых энергиях (сдвиги фаз вплоть доT π=1.3 (ГэВ)) и из вклада σ-полюса вt-канале, вблизиu=0, является совместимым с имеющимися параметрами Редже, полученными при высоких энергиях. В частности, в интервале отu=0.1 до −0.35 (ГэВ)2 мы предсказываем нуль в амплитуде рассеяния, связанной с обменом нуклонной (N α) траекторией, и отсутствие нуля в амплитуде рассеяния, связанной с Δ обменом. СвязьN γ траектории является слабой во всей этой области.
Similar content being viewed by others
References
R. Dolen, D. Horn andC. Schmid:Phys. Rev. Lett.,19, 402 (1967). See alsoa)A. A. Logunov, L. D. Soloviev andA. N. Tavkhelidze:Phys. Lett.,24 B, 181 (1967);b) California Institute of Technology Preprint by DHS (CALT-68-143: Prediction of the Regge Parameters of the σ Trajectory From Low-Energy πG Data, to be published inPhys. Rev.).
A. A. Logunov andL. D. Soloviev:Sov. Journ. Nucl. Phys.,10, 60 (1959);V. De Alfaro, S. Fubini, G. Rossetti andG. Furlan:Phys. Lett.,21, 576 (1966).
C. B. Chiu andJ. D. Stack:Phys. Rev.,153 1575 (1967).
We assume the contribution of the third double spectral function to the amplitude at this point can be ignored. For a discussion of the effect of the third double spectral function at nonsense wrong signature points seeS. Mandelstam andL. L. Wang:Phys. Rev.,160, 1490 (1967).
C. Lovelace:Pion-nucleon phase shifts, submitted to theXIII International Conference on High Energy Physics (Berkeley, Cal., 1966).
S. C. Frautschi andJ. D. Walecka:Phys. Rev.,120, 1486 (1960).
V. Singh:Phys. Rev.,129, 1889 (1963).
M. Jacob andG. F. Chew:Strong Interaction Physics (New York, 1963).
The f0 meson has the quantum numbersI=0,J=2,G=+1, mass=1260 MeV, and decays predominantly into two pions.
J. Schwarz:Symmetry subtractions and superconvergence (Princeton University Preprint, 1967, unpublished). The fact that the Schwarz sum rule can be used to show that the contribution of f0 to theB amplitude sum rule is suppressed was recognized byFinkelstein. We are indebted to Dr.Finkelstein for showing us the numerical work in this connection before publication.
This is perhaps the weakest point in the present analysis. It is almost certain that thet-channel spectrum forI t=1 will be more complicated. However, we derive a certain confidence in the pole approximation for thet-channel spectrum based on the discussion in the Appendix. For an indication of some of the problems involved see the following references:C. B. Chiu andM. DerSarkissian:Nuovo Cimento,51 A, 235 (1967) and references given there.
D. Beder andJ. Finkelstein:Phys. Rev.,160, B 1363 (1967).
B. R. Desai:Phys. Rev. Lett.,17, 498 (1966). The convention for defining theW u-plane is as follows: For thel=j+1/2 trajectory, β<0 forW u<−(Mn+mπ) and for thel=j−1/2 trajectory β>0 forW u>(Mn+mπ). So β must change sign in the interval −(M n+mπ)<W u<(M n+mπ). It is therefore plausible that dβ/dW u>0 nearW u=0 provided that the trajectory has not passed through the nonsense wrong signature point.
V. Barger andD. Cline:Phys. Rev.,155, 1792 (1967).
A. Ashmore, C. J. S. Damerell, W. R. Frisken, R. Rubenstein, J. Orear, D. P. Owen, F. C. Peterson, A. L. Read, D. G., Ryan andD. H. White:Phys. Rev. Lett.,19, 460 (1967).
Author information
Authors and Affiliations
Additional information
Part of this work was done under the auspices of the United States Atomic Energy Commission.
Traduzione a cura della Redazione.
Перевебено ребакцией.
Rights and permissions
About this article
Cite this article
Chiu, C.B., DerSarkissian, M. Application of finite energy sum rules to πN scattering near the backward directionscattering near the backward direction. Nuovo Cimento A (1965-1970) 55, 396–411 (1968). https://doi.org/10.1007/BF02857562
Received:
Published:
Issue Date:
DOI: https://doi.org/10.1007/BF02857562