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IHEP 2001 - 18 | |
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| S.I.Alekhin, V.B.Anykeyev, A.A.Borisov, N.I.Bozhko, S.K.Chernichenko, R.M.Fachrutdinov, V.N.Goryachev, S.V.Goryachev, M.M.Kirsanov, A.I.Kononov, A.S.Kozhin, V.V.Lipajev, A.I.Mukhin, Y.I.Salomatin, Y.M.Sviridov, V.L.Tumakov, A.S.Vovenko (Institute for High Energy Physics, Protvino, Russia) Y.A.Batusov, S.A.Bunyatov, O.Y.Denisov, M.Y.Kazarinov, O.L.Klimov, A.V.Krasnoperov, Y.A.Nefedov, B.A.Popov, S.N.Prakhov, V.I.Snyatkov, V.V.Tereshchenko (Joint Institute for Nuclear Research, Dubna, Russia) | ||
| Determination of the High-Twist Contribution to the Structure Function $xF^{\nu N}_3 | ||
| Protvino, 2001.- p.6, figs. 1, tables 1, refs.:21. | ||
We extract the high-twist contribution to the neutrino-nucleon structure function $xF_3^{(\nu+\overline{\nu})N}$ from the analysis of the data collected by the IHEP-JINR Neutrino Detector in the runs with the focused neutrino beams at the IHEP 70 GeV proton synchrotron. The analysis is performed within the infrared renormalon (IRR) model of high twists in order to extract the normalization parameter of the model. From the NLO QCD fit to our data we obtained the value of the IRR model normalization parameter $\Lambda^2_{3}=0.69\pm0.37~({\rm exp})\pm0.16~({\rm theor})~{\rm GeV}^2$. We also obtained $\Lambda^2_{3}=0.36\pm0.22~({\rm exp})\pm0.12~({\rm theor})~{\rm GeV}^2$ from a similar fit to the CCFR data. The average of both results is $\Lambda^2_{3}=0.44\pm0.19~({\rm exp})~{\rm GeV}^2$.
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