10 - H1 - Desy
10 - H1 - Desy
10 - H1 - Desy
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20 Theoretical framework<br />
than in the inclusive case, suggests that higher order corrections are of less importance<br />
for prompt photons if accompanied by an energetic jet.<br />
Inclusive prompt photon<br />
dσ / dE γ T (pb/GeV)<br />
<strong>10</strong><br />
<strong>H1</strong><br />
ZEUS<br />
PYTHIA<br />
dir<br />
without m.i.<br />
HERWIG<br />
dσ / dη γ (pb)<br />
40<br />
30<br />
20<br />
<strong>10</strong><br />
1<br />
a)<br />
<strong>10</strong> 2 6 8 <strong>10</strong><br />
E γ T (GeV)<br />
0<br />
b)<br />
-1 -0.5 0 0.5<br />
η γ<br />
Figure 1.15: Inclusive prompt photon differential cross sections dσ/dE γ T<br />
(a) and dσ/dηγ<br />
(b) in photoproduction as measured by the <strong>H1</strong> [35] and ZEUS [36] collaborations compared<br />
to predictions by PYTHIA (solid black line) and HERWIG (dashed red line). The<br />
contribution of direct events is presented with a dashed dotted line and a prediction<br />
without multiparton interaction with blue dotted line. Cross sections of the ZEUS were<br />
corrected to the kinematics used by the <strong>H1</strong> analysis.<br />
Prompt photon production with accompanying jet was also studied by the ZEUS collaboration<br />
[38] and some results of this study are presented in figure 1.17. Monte Carlos again<br />
predict cross sections low in the normalisation, while QCD calculations give a reasonable<br />
description of the data. Especially the calculation based on the k T factorisation approach<br />
(see section 2.2.2) performs well, while NLO calculations predict too low cross sections<br />
for low transverse energies of the photon and low pseudorapidities. For an increased minimum<br />
transverse energy of the photons to 7 GeV, the differential cross sections are well<br />
described by all studied calculations.<br />
In deep inelastic scattering, prompt photons were studied by both ZEUS [41, 42] and<br />
<strong>H1</strong> [43]. Figure 1.18 presents the differential cross sections measured by the ZEUS collaboration<br />
[41] compared to MC predictions of PYTHIA and HERWIG. The measurement<br />
has been performed in the phase space 5 < E γ T < <strong>10</strong> GeV, −0.7 < ηγ < 0.9 and<br />
Q 2 > 35 GeV 2 . The transverse energy distribution is reasonably described by PYTHIA<br />
scaled by factor 2.3 and by HERWIG scaled by factor 7.9. PYTHIA fails to predict even<br />
the shape of cross section in bins of η γ , while HERWIG predicts a too steep Q 2 slope.<br />
The contribution of photons radiated from the electron was neglected in this study.