Prospects for detecting an η′c in two-photon processes

Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics

Volumn 385, Issue 1-4, 1996, Pages 391-394

  Barnes, T ^a,b   Browder, T E ^c   Tuan, S F ^c  

^a OAK RIDGE NATIONAL LABORATORY   (United States)

^b UNIVERSITY OF TENNESSEE   (United States)

^c UNIVERSITY OF HAWAII   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0041593424     PISSN: 03702693     EISSN: None     Source Type: Journal    
DOI: 10.1016/0370-2693(96)00878-7     Document Type: Article

References (23)

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3. K.T. Chao (Zhao), Y.F. Gu and S.F. Tuan, On Trigluonia in Charmonium Physics, BIHEP-TH-93-45, PUTP-93-24, and UH-511-790-94; Commun. Theor. Phys. (in press); S.J. Brodsky, G. Peter Lepage and S.F. Tuan, Phys. Rev. Lett. 59 (1987) 621; S.F. Tuan, Aspects of Charmonium, UH-511-832-95, hep-ph/9509388; Proceedings of the HADRON'95 conference (in press).
4. K.T. Chao (Zhao), Y.F. Gu and S.F. Tuan, On Trigluonia in Charmonium Physics, BIHEP-TH-93-45, PUTP-93-24, and UH-511-790-94; Commun. Theor. Phys. (in press); S.J. Brodsky, G. Peter Lepage and S.F. Tuan, Phys. Rev. Lett. 59 (1987) 621; S.F. Tuan, Aspects of Charmonium, UH-511-832-95, hep-ph/9509388; Proceedings of the HADRON'95 conference (in press).
5. K.T. Chao (Zhao), Y.F. Gu and S.F. Tuan, On Trigluonia in Charmonium Physics, BIHEP-TH-93-45, PUTP-93-24, and UH-511-790-94; Commun. Theor. Phys. (in press); S.J. Brodsky, G. Peter Lepage and S.F. Tuan, Phys. Rev. Lett. 59 (1987) 621; S.F. Tuan, Aspects of Charmonium, UH-511-832-95, hep-ph/9509388; Proceedings of the HADRON'95 conference (in press).
6. K.T. Chao (Zhao), Y.F. Gu and S.F. Tuan, On Trigluonia in Charmonium Physics, BIHEP-TH-93-45, PUTP-93-24, and UH-511-790-94; Commun. Theor. Phys. (in press); S.J. Brodsky, G. Peter Lepage and S.F. Tuan, Phys. Rev. Lett. 59 (1987) 621; S.F. Tuan, Aspects of Charmonium, UH-511-832-95, hep-ph/9509388; Proceedings of the HADRON'95 conference (in press).
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15. c2), where the photon flux factor is given for instance in Ref. [15] below.
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18. O. Adriani et al., Phys. Lett. B 318 (1993) 575.
19. c(3590)) = 1.38(30) keV. This references summarizes other predictions, which lie in the range ≈ 1.0-1.7 keV, somewhat smaller than the result of Ackleh and Barnes.
20. c(3590)) = 1.38(30) keV. This references summarizes other predictions, which lie in the range ≈ 1.0-1.7 keV, somewhat smaller than the result of Ackleh and Barnes.
21. R.N. Cahn, Proceedings of the XIVth International Symposium on Lepton and Photon Interactions, Stanford (1989) p. 60; particularly Eq. (12.1).
22. Monte Carlo integration of the exact differential cross section without assuming the equivalent photon approximation gives 2.32 rather than 2.02 for the ratio of photon flux factors. This would reduce the event yield by about 15%. Private communication, Vladimir Savinov.
23. K. Berkelman, Cornell preprint CLNS 96/1396.