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Joint Institute for Nuclear Research Relativistic ... - Index of - JINR

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and<br />

< ν p >= 1− 3 2 w D +∆ rel , (15)<br />

w D is the probability <strong>of</strong> the D state in the deuteron.<br />

The experimental values <strong>of</strong> the first moments <strong>of</strong> the spin structure functions <strong>of</strong> the<br />

protonΓ p 1 andneutronΓn 1 atQ2 = 5GeV 2 obtainedbytheE155collaborationbyanalyzing<br />

all available data are as follows [3]:<br />

The experimental value <strong>for</strong> Γ d 1 is<br />

Γ p 1 = 0,118±0,004(stat.)±0,007(sist.), (16)<br />

Γ n 1 = −0,058±0,005(stat.)±0,008(sist.). (17)<br />

Γ d 1<br />

= 0,028±0,004(stat.)±0,005(sist.). (18)<br />

The Bjorken and Ellis-Jaffe sum rules are theoretical relations <strong>of</strong> the first moments <strong>for</strong><br />

the proton and neutron to the fundamental weak coupling constants. The test <strong>of</strong> the<br />

Bjorken sum rule <strong>for</strong> Q 2 = 5GeV 2 with the experimental data [3] give Γ p 1−Γ n 1 = 0,176±<br />

0,003(stat.)±0,007(sist.). The first moment <strong>of</strong>the spin structure function <strong>of</strong>the neutron<br />

extracted from the measured first moments <strong>of</strong> the spin structure functions <strong>of</strong> the deuteron<br />

Γ D 1 | exp and proton Γ p 1| exp including the relativistic correction is represented in the <strong>for</strong>m<br />

Γ n 1 (Q2 ) = 2Γd 1 (Q2 )| exp<br />

< ν p > −Γp 1 (Q2 )| exp . (19)<br />

At Q 2 = 5GeV 2 , Γ n 1 (Q2 ) = −0.05621. The Bjorken sum at Q 2 = 5GeV 2 gives Γ p 1 −Γ n 1 =<br />

0.17421. There are several different parameterizations <strong>for</strong> the spin structure function<br />

<strong>of</strong> the nucleon g N 1 (x,Q 2 ) . In this work, the parameterization <strong>of</strong> parton distributions<br />

LSS2006 [4] is used. The results were obtained with the Bonn wave function <strong>of</strong> the<br />

deuteron (w D =0,0425) [5].<br />

References<br />

[1] F.F.Pavlov, Zh. Eksp. Teor. Fiz. 141, 1084(2012)[Sov. Phys. JETP 114, 946(2012)];<br />

arXiv:hep-ph/1206.0676v2.<br />

[2] P.L. Anthony, R.G. Arnold, T. Averett et al., arXiv:hep-ph/0007248v1.<br />

[3] P.L. Anthony et al., Phys. Lett. B 493, 19 (2000).<br />

[4] E. Leader, A.V. Sidorov, and D.B. Stamenov, Phys. Rev. D 75, 074027 (2007).<br />

[5] R. Machleidt, K. Holinde, Ch. Elster, Phys. Rep. 149, 1 (1987).<br />

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