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2011 QCD and High Energy Interactions - Rencontres de Moriond ...

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The azimuthal or<strong>de</strong>ring should be<br />

visible as a peak in a suitably <strong>de</strong>fined<br />

power spectrum ( in or<strong>de</strong>r<br />

to obtain a clear signal, the <strong>de</strong>finition<br />

of the power spectrum has<br />

to reflect the parametrization of<br />

the helix string structure, see discussion<br />

in 3 ). A typical size <strong>and</strong><br />

position of the expected signal is<br />

shown in Fig. 3, based on the prediction<br />

of the helix string mo<strong>de</strong>l<br />

tuned at LEP data.<br />

4 Conclusions<br />

Figure 3: Azimuthal or<strong>de</strong>ring of hadrons can be <strong>de</strong>tected as a peak in<br />

the power spectrum <strong>de</strong>fined according to the expected helix structure.<br />

Pythia mo<strong>de</strong>lling of non-diffractive events at √ s=900 GeV.<br />

Generator level study.<br />

The hypothesis of the existence of a helix-like or<strong>de</strong>red gluon field explains some characteristic<br />

discrepancies between mo<strong>de</strong>lling of hadronic processes <strong>and</strong> the data. The interplay between soft<br />

non-perturbative region <strong>and</strong> the parton shower activity is better <strong>de</strong>scribed using the helix string<br />

hypothesis (the comparison is done using a representative set of inclusive charged spectra <strong>and</strong><br />

event shape variables). The helix string scenario predicts azimuthal or<strong>de</strong>ring of direct hadrons,<br />

experimentally observable at LHC. If confirmed, such an effect may be consi<strong>de</strong>red a first direct<br />

evi<strong>de</strong>nce in favour of the helix-like <strong>QCD</strong> string.<br />

References<br />

1. B. An<strong>de</strong>rsson, G. Gustafson, J. Hakkinen, M. Ringner <strong>and</strong> P. Sutton, JHEP 9809 (1998)<br />

014 [arXiv:hep-ph/9807541].<br />

2. DELPHI Coll., DELPHI 98-156 PHYS 799.<br />

3. ˇ S. Todorova,[arXiv:1101.2407]<br />

4. DELPHI Coll., Z. Phys. C73 (1996) 11., CERN-PPE/96-120.<br />

5. New J.Phys.13 (<strong>2011</strong>) 053033.<br />

6. A. Buckley, H. Hoeth, H. Lacker, H. Schulz <strong>and</strong> J. E. von Seggern,<br />

doi:10.1140/epjc/s10052-009-1196-7.<br />

7. T. Sjöstr<strong>and</strong>, S. Mrenna <strong>and</strong> P. Z. Sk<strong>and</strong>s, JHEP 0605 (2006) 026 [arXiv:hep-ph/0603175].<br />

8. L.Lönnblad, Comput.Phys.Commun. 71 (1992) 15.<br />

9. ˇ S. Todorova, https://nova.www.cern.ch/nova/helix.html<br />

10. ˇ S. Todorova,[arXiv:1012.5778]<br />

11. H. Schulz, private communication.

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