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References - Bogoliubov Laboratory of Theoretical Physics - JINR

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The sensitivity <strong>of</strong> the data to the nucleon parton distribution functions is illustrated by<br />

comparison <strong>of</strong> the results obtained using the parametrizations CTEQ5L [8] (solid line) and<br />

GRV98LO [9] (dashed line). The GRV98 parton distributions have been chosen, because<br />

the strange sea there is purely perturbative, originating only from the production <strong>of</strong> q¯qpairs<br />

by gluons. On the contrary CTEQ allows explicit non-perturbative strangeness in<br />

the nucleon. The amount <strong>of</strong> strangeness was extracted from dimuon experiments CCFR<br />

and NuTeV [10]. This leads to ¯s(x) being nearly two times larger in CTEQ than in GRV98<br />

for COMPASS energies in the x =0.001 − 0.01 range. Therefore the calculation <strong>of</strong> DLL<br />

for ¯ Λ using CTEQ gives twice bigger spin transfer and is closer to the experimental points<br />

in comparison with GRV98.<br />

It should be noted that the polarization <strong>of</strong> Λ and ¯ Λ could be used as a tool to estimate<br />

s(x) and¯s(x) independently <strong>of</strong> each other. More detailed description <strong>of</strong> the analysis could<br />

be found in [12].<br />

<strong>References</strong><br />

[1] COMPASS Collaboration, P. Abbon et al., Nucl. Instrum. Meth. A577 (2007) 455.<br />

[2] NOMAD Collaboration, P. Astier et al., Nucl. Phys., B588 (2000) 3.<br />

[3] NOMAD Collaboration, P. Astier et al., Nucl. Phys., B605 (2001) 3.<br />

[4] E665 Collaboration, M.R. Adams et al., Eur. Phys. J. C17 (2000) 263.<br />

[5] HERMES Collaboration, A. Airapetian et al., Phys. Rev., D74 (2006) 072004.<br />

[6] A.Bravar,D.vonHarrach,A.M.Kotzinian,Eur.Phys.J.,C2 (1998) 329.<br />

[7] J. Ellis, A.M. Kotzinian, D. Naumov, M.G. Sapozhnikov, Eur. Phys. J., C52 (2007)<br />

283.<br />

[8] F. Olness et al., Eur. Phys. J., C40(2005) 145.<br />

[9] M. Glück,E.Reya,A.Vogt,Eur.Phys.J.,C5 (1998) 461.<br />

[10] CCFR and NuTeV Collaborations, M. Goncharov et al., Phys. Rev., D64 (2001)<br />

112006.<br />

[11] M. Burkardt, R.L. Jaffe, Phys. Rev. Lett., 70 (1993) 2537.<br />

[12] COMPASS Collaboration, M. Alekseev et al., Eur. Phys. J. C64 (2009) 171.<br />

322

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