The data were collected in two days with a primary electron beam energy of only 3.3 GeV, limiting the data from this run to smaller values of Q2 and scattering angle. Nonetheless, this measurement yields a data sample for e±p with statistics comparable to those of the best previous measurements. We have shown that we can cleanly identify elastic scattering events and correct for the difference in acceptance for electron and positron scattering. Because we ran with only one polarity for the chicane, we are unable to study the difference between the incoming electron and positron beams. This systematic effect leads to the largest uncertainty in the final ratio of positron to electron scattering: R = 1.027 ± 0.005 ± 0.05 for Q2 = 0.206 GeV2 and 0.830 0.943. Conclusions: We have demonstrated that the tertiary e ± beam generated using this technique provides the opportunity for dramatically improved comparisons of e±p scattering, covering a significant range in both Q2 and scattering angle. Combining data with different chicane polarities will allow for detailed studies of the difference between the incoming e+ and e− beams.

Demonstration of a novel technique to measure two-photon exchange effects in elastic e^{±}p scattering

CONTALBRIGO, Marco;PAPPALARDO, Luciano Libero;
2013

Abstract

The data were collected in two days with a primary electron beam energy of only 3.3 GeV, limiting the data from this run to smaller values of Q2 and scattering angle. Nonetheless, this measurement yields a data sample for e±p with statistics comparable to those of the best previous measurements. We have shown that we can cleanly identify elastic scattering events and correct for the difference in acceptance for electron and positron scattering. Because we ran with only one polarity for the chicane, we are unable to study the difference between the incoming electron and positron beams. This systematic effect leads to the largest uncertainty in the final ratio of positron to electron scattering: R = 1.027 ± 0.005 ± 0.05 for Q2 = 0.206 GeV2 and 0.830 0.943. Conclusions: We have demonstrated that the tertiary e ± beam generated using this technique provides the opportunity for dramatically improved comparisons of e±p scattering, covering a significant range in both Q2 and scattering angle. Combining data with different chicane polarities will allow for detailed studies of the difference between the incoming e+ and e− beams.
2013
M., Moteabbed; M., Niroula; B. A., Raue; L. B., Weinstein; D., Adikaram; J., Arrington; W. K., Brooks; J., Lachniet; Dipak, Rimal; M., Ungaro; A., Afanasev; K. P., Adhikari; M., Aghasyan; M. J., Amaryan; S., Anefalos Pereira; H., Avakian; J., Ball; N. A., Baltzell; M., Battaglieri; V., Batourine; I., Bedlinskiy; R. P., Bennett; A. S., Biselli; J., Bono; S., Boiarinov; W. J., Briscoe; V. D., Burkert; D. S., Carman; A., Celentano; S., Chandavar; P. L., Cole; P., Collins; Contalbrigo, Marco; O., Cortes; V., Crede; A., D’Angelo; N., Dashyan; R., De Vita; E., De Sanctis; A., Deur; C., Djalali; D., Doughty; R., Dupre; H., Egiyan; L., El Fassi; P., Eugenio; G., Fedotov; S., Fegan; R., Fersch; J. A., Fleming; N., Gevorgyan; G. P., Gilfoyle; K. L., Giovanetti; F. X., Girod; J. T., Goetz; W., Gohn; E., Golovatch; R. W., Gothe; K. A., Griffioen; M., Guidal; N., Guler; L., Guo; K., Hafidi; H., Hakobyan; C., Hanretty; N., Harrison; D., Heddle; K., Hicks; D., Ho; M., Holtrop; C. E., Hyde; Y., Ilieva; D. G., Ireland; B. S., Ishkhanov; E. L., Isupov; H. S., Jo; K., Joo; D., Keller; M., Khandaker; A., Kim; F. J., Klein; S., Koirala; A., Kubarovsky; V., Kubarovsky; S. E., Kuhn; S. V., Kuleshov; S., Lewis; H. Y., Lu; M., Maccormick; I. J. D., Macgregor; D., Martinez; M., Mayer; B., Mckinnon; T., Mineeva; M., Mirazita; V., Mokeev; R. A., Montgomery; K., Moriya; H., Moutarde; E., Munevar; C., Munoz Camacho; P., Nadel Turonski; R., Nasseripour; S., Niccolai; G., Niculescu; I., Niculescu; M., Osipenko; A. I., Ostrovidov; Pappalardo, Luciano Libero; R., Paremuzyan; K., Park; S., Park; E., Phelps; J. J., Phillips; S., Pisano; O., Pogorelko; S., Pozdniakov; J. W., Price; S., Procureur; D., Protopopescu; A. J. R., Puckett; M., Ripani; G., Rosner; P., Rossi; F., Sabatié; M. S., Saini; C., Salgado; D., Schott; R. A., Schumacher; E., Seder; H., Seraydaryan; Y. G., Sharabian; E. S., Smith; G. D., Smith; D. I., Sober; D., Sokhan; S., Stepanyan; S., Strauch; W., Tang; C. E., Taylor; Ye, Tian; S., Tkachenko; H., Voskanyan; E., Voutier; N. K., Walford; M. H., Wood; N., Zachariou; L., Zana; J., Zhang; Z. W., Zhao; I., Zonta
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11392/2018015
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