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References - Bogoliubov Laboratory of Theoretical Physics - JINR

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polarization as well as a construction <strong>of</strong> the statistical weight used in the analysis requires<br />

the knowledge <strong>of</strong> the so-called analyzing power, aLL, ( the ratio <strong>of</strong> polarized over unpolarized<br />

partonic cross sections) and the signal strength event-by-event basis. The analyzing<br />

power is calculated in the LO QCD approximation and as a signal identified D 0 meson<br />

(reconstructed from its decay) is used. In contrast to the resolved photon contribution<br />

NLO QCD corrections to unpolarized and polarized cross sections are supposed to be<br />

large in the COMPASS kinematical domain. To allow to use the COMPASS data in the<br />

independent analysis the open-charm asymmetries in bins in pT and energy <strong>of</strong> D 0 meson<br />

was also published [2]. In this paper I would like to present the method <strong>of</strong> computing analyzing<br />

power event-by-event basis in the NLO QCD approximation. The method is based<br />

on LO MC with Parton Shower (PS) and can be easily allied in the COMPASS analysis<br />

scheme, also in the weighting method. The calculations are done for NLO QCD corrected<br />

PGF process and the new gluon polarization result based on published asymmetries are<br />

also presented. There is another part <strong>of</strong> NLO QCD corrections to muoproduction <strong>of</strong> opencharm:<br />

light quark originated processes where emitted gluon produces charm-anticharm<br />

quark pair. These processes contribute to the background because they don’t probe gluons<br />

inside the nucleon. It introduces the complication into the analysis because signal<br />

defined as an observed D 0 meson is polluted by these higher order processes 1 .Theyare<br />

not considered in this paper but the extension <strong>of</strong> the proposed method is rather straightforward<br />

however technically more complicated. It requires modification <strong>of</strong> the asymmetry<br />

decomposition equation which is a basis <strong>of</strong> the COMPASS analysis (see. eqs 5 and 6<br />

in [2]). The paper is organized as follows: in the next section the NLO QCD corrections<br />

to the PGF process are discussed. The Monte-Carlo method and the Parton Shower concept<br />

is presented in section 3. The new results for the gluon polarization obtained using<br />

published asymmetries are presented in section 4. The discussion <strong>of</strong> the approximation<br />

used in the computation <strong>of</strong> the analyzing power is presented in section 4. Conclusions are<br />

presented in section 5.<br />

2 NLO QCD corrections to the open-charm cross<br />

sections<br />

In the LO QCD approximation PGF is the only process which contributes to the opencharm<br />

production. Moreover for the energy range covered by the COMPASS experiment<br />

the QCD evolution is not able to produce significant fraction <strong>of</strong> charm sea inside nucleon<br />

and only hard part <strong>of</strong> the cross section is responsible for open-charm production. As it<br />

was mentioned above the resolved photon contribution is also small and so-called intrinsic<br />

charm content inside nucleon is in the considered kinematics suppressed. Therefore<br />

observation <strong>of</strong> the charm signal seems to be an ideal to probe gluons inside nucleon for<br />

the COMPASS experiment. It is however known that the unpolarized cross section (averaged<br />

over spin states) is not precisely described by the LO QCD approximation and<br />

the NLO QCD corrections are important for the photoproduction <strong>of</strong> the open-charm, [4].<br />

Also spin-dependent (polarized) cross section, calculated recently shows the important<br />

dependence <strong>of</strong> the approximation used [5]. It was also argued that the naive expectation<br />

1Notice that background taken into account in the COMPASS analysis is a combinatorial background;<br />

see also [3]<br />

230

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