24.12.2012 Views

References - Bogoliubov Laboratory of Theoretical Physics - JINR

References - Bogoliubov Laboratory of Theoretical Physics - JINR

References - Bogoliubov Laboratory of Theoretical Physics - JINR

SHOW MORE
SHOW LESS

You also want an ePaper? Increase the reach of your titles

YUMPU automatically turns print PDFs into web optimized ePapers that Google loves.

Unpolarized target asymmetries. The azimuthal asymmetry for hadron production<br />

in lepton DIS <strong>of</strong>f unpolarized target was predicted to be non-zero many years ago due to<br />

the fact that the kinematics is noncollinear when the quark intrinsic transverse momentum<br />

is taken into account. Other possible sources <strong>of</strong> the asymmetry are perturbative gluon<br />

radiation and Boer-Mulders mechanism, which is due to the correlation <strong>of</strong> the quark<br />

intrinsic transverse momentum and intrinsic transverse spin. This correlation is described<br />

by the Boer-Mulders distribution function h ⊥ 1 (x, kT ), which represents the transversepolarization<br />

distribution <strong>of</strong> quarks inside an unpolarized nucleon.<br />

The cross-section for hadron production in lepton-nucleon DIS lN −→ l ′ hX for the case<br />

<strong>of</strong> unpolarized target and unpolarized beam can be written in the following form [11]:<br />

d 5 σ<br />

dxdydzdP 2 h⊥ dφh<br />

∝ A(y)FUU,T + B(y)FUU,L +<br />

cos φh<br />

C(y)cosφhFUU cos 2φh<br />

+ B(y)cos2φhFUU Here, φh is the angle between the lepton scattering plane and the hadron production plane,<br />

cos φh<br />

cos 2φh<br />

A(y), B(y), and C(y) are kinematic factors, FUU,T(L), FUU ,andFUU are structure<br />

functions responsible for 1, cos φh, cos2φhazimuthal modulations, respectively.<br />

At HERMES, the extraction <strong>of</strong> the unpolarized modulations was performed using a multidimensional<br />

unfolding procedure to correct for radiative and acceptance effects on hydrogen<br />

and deuterium data, separately for positive and negative hadrons. The cos φh<br />

amplitudes as function <strong>of</strong> x, y, z, andPh⊥for positive and negative hadrons produced <strong>of</strong>f<br />

hydrogen target are presented in top panel <strong>of</strong> Fig. 6. The cos 2φh amplitudes are presented<br />

in bottom panel <strong>of</strong> Fig. 6. An important feature shown by HERMES data is the different<br />

behaviour <strong>of</strong> the amplitudes for positive and negative hadrons. Such difference can be<br />

considered as an evidence <strong>of</strong> a non-zero Boer-Mulders function.<br />

Analogous results were obtained for the hadron asymmetries with deuterium target.<br />

2〈<br />

cos( φ ) 〉<br />

h UU<br />

UU<br />

〉<br />

)<br />

2〈<br />

cos(2φ<br />

h<br />

0.2<br />

0.1<br />

0<br />

-0.1<br />

-0.2<br />

-0.3<br />

0.2<br />

0.1<br />

0<br />

-0.1<br />

-0.2<br />

Hydrogen<br />

-<br />

h<br />

+<br />

h<br />

Hydrogen<br />

-<br />

h<br />

+<br />

h<br />

-1<br />

2<br />

.1<br />

0<br />

.1<br />

2<br />

3<br />

10 1<br />

x<br />

2<br />

.1<br />

0<br />

.1<br />

2<br />

-1<br />

10 1<br />

x<br />

2<br />

.1<br />

0<br />

.1<br />

2<br />

3<br />

0.4 0.6 0.8 0.2 0.4 0.6 0.8 1<br />

y<br />

z<br />

2<br />

.1<br />

0<br />

.1<br />

2<br />

2<br />

0.4 0.6 0.8 0.2 0.4 0.6 0.8 1<br />

y<br />

z<br />

2<br />

.1<br />

0<br />

.1<br />

2<br />

3<br />

2<br />

.1<br />

0<br />

.1<br />

HERMES Preliminary<br />

0.2 0.4 0.6<br />

[GeV]<br />

Ph<br />

HERMES Preliminary<br />

0.2 0.4 0.6<br />

[GeV]<br />

Figure 6: 2 〈cos (φh)〉 UU amplitude (top panel) and 2 〈cos (2φh)〉 UU amplitude (bottom panel) for negative<br />

(circles) and positive (squares) hadrons. Data are from hydrogen target. The error bars represent<br />

the statistical errors while the band represents the systematic errors. The open points at high z are not<br />

included in the projections over the other variables.<br />

226<br />

Ph<br />

(2)

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!