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FIAS Scientific Report 2011 - Frankfurt Institute for Advanced Studies ...

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Dileptons from the strongly interacting quark-gluon plasma (sQGP)<br />

Collaborators: O. Linnyk 1,3 , E. L. Bratkovskaya 1,2 , V. Ozvenchuk 2 , J. Manninen 1,3 , W. Cassing 3 , C.M. Ko 4<br />

1 Institut für Theoretische Physik, Goethe Universität <strong>Frankfurt</strong> am Main, Germany, 2 <strong>Frankfurt</strong> <strong>Institute</strong> <strong>for</strong> <strong>Advanced</strong><br />

<strong>Studies</strong>, Germany, 3 Institut für Theoretische Physik, Justus Liebig Universität Gießen, Germany 4 Cyclotron <strong>Institute</strong><br />

and Department of Physics and Astronomy, Texas A&M University, College Station, Texas, USA<br />

We address dilepton production in Au+Au collisions at √ sNN = 200 GeV by employing the parton-hadronstring<br />

dynamics (PHSD) off-shell transport approach [3,4,6]. Within the PHSD one solves generalized transport<br />

equations and consistently describes the full evolution of a relativistic heavy-ion collision [2]. We calculated the<br />

dilepton radiation from partonic interactions through the reactions q ¯q → γ∗ , q ¯q → γ∗ + g and qg → γ∗q ( ¯qg →<br />

γ∗ ¯q) in the early stage of relativistic heavy-ion collisions with the differential cross sections <strong>for</strong> electromagnetic<br />

radiation calculated with the same propagators as those incorporated in the PHSD transport approach [1]. By<br />

comparing our calculated results [3,4] to the data, we have studied the relative importance of different dilepton<br />

production mechanisms and addressed in particular the ’PHENIX puzzle’ of a large enhancement of dileptons<br />

in the mass range from 0.15 to 0.6 GeV as compared to the emission of hadronic states. Similar to our findings<br />

at SPS energies [5], we find that the partonic dilepton production channels are visible in the intermediate-mass<br />

region between the φ and J/Ψ peaks [3,4,6,9]. Our studies have demonstrated that the observed excess in the<br />

low mass dilepton regime cannot be attributed to partonic productions as expected earlier. Thus the ’PHENIX<br />

puzzle’ still has no explanation from the theoretical approaches so far. The solution has to be relegated to<br />

the experimental side. In fact, the STAR collaboration has taken independent dilepton data <strong>for</strong> centralities<br />

different from the PHENIX measurements and also with different detector acceptances. Our calculations allow<br />

to match with the different experimental conditions and thus to provide a ’theoretical link’ between the different<br />

measurements. To this extent, we have provided our predictions <strong>for</strong> the conditions of the STAR experiment,<br />

which happen to be in a rough agreement with the preliminary data [4].<br />

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Figure 1: The PHSD results <strong>for</strong> the mass differential dilepton spectra in case of inclusive Au+Au collisions at<br />

√ s = 200 GeV in comparison to the data from PHENIX (left pannel) and STAR (right pannel) Collaborations.<br />

Related publications in <strong>2011</strong>:<br />

1) O. Linnyk, J. Phys. G38 (<strong>2011</strong>) 025105.<br />

2) E.L. Bratkovskaya, W. Cassing, V.P. Konchakovski, O. Linnyk, Nucl. Phys. A856 (<strong>2011</strong>) 162.<br />

3) O. Linnyk, W. Cassing, E.L. Bratkovskaya, J. Manninen, Nucl. Phys. A855 (<strong>2011</strong>) 273.<br />

4) O. Linnyk, W. Cassing, J. Manninen, E.L. Bratkovskaya, C.M. Ko, arXiv:1111.2975, Phys. Rev. C (in print).<br />

5) O. Linnyk, E.L. Bratkovskaya, V. Ozvenchuk, W. Cassing, C.M. Ko, Phys. Rev. C84 (<strong>2011</strong>) 054917.<br />

6) J. Manninen, E.L. Bratkovskaya, W. Cassing, O. Linnyk, Eur. Phys. J. C71 (<strong>2011</strong>) 1615.<br />

7) O. Linnyk, E.L. Bratkovskaya, W. Cassing, J. Phys. Conf. Ser. 316 (<strong>2011</strong>) 012028.<br />

8) O. Linnyk, E.L. Bratkovskaya, J. Manninen, W. Cassing, J. Phys. Conf. Ser. 312 (<strong>2011</strong>) 012010.<br />

9) J. Manninen, E.L. Bratkovskaya, W. Cassing, O.Linnyk, J. Phys. Conf. Ser. 270 (<strong>2011</strong>) 012039.<br />

10) O. Linnyk, E.L. Bratkovskaya, W. Cassing, PoS BORMIO<strong>2011</strong> (<strong>2011</strong>) 029.<br />

47

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