Analysis of the Direct Photon Data of the Experiment WA98 B,W
K. Gallmeister, B. Kämpfer, O.P. Pavlenko1

Recently the WA98 collaboration published data concerning the direct photon production in the reaction Pb(158 AGeV)+Pb [1]. Analog to our studies [2] of the dilepton spectra in similar reactions, we use a superposition of hard photon production processes and of the yields from thermalized matter in order to describe these data.
The contributions of the hard annihilation and Compton like diagrams within the framework of perturbative QCD are calculated using the event generator PYTHIA. The comparison of PYTHIA results and various direct photon data in proton induced collisions indicates that the shapes of the data are well described. Fig. 1 displays two examples of the comparison of our calculations and data.
The hard perturbative QCD contribution, calculated for pp collisions, is up-scaled such that the large-p^ tail of the WA98 data is reproduced (cf. fig. 2). The thermal source is described by


dN
d3p/E
= Neff  5aasTeff2
12p2
ó
õ
1

0 
ds s2 ó
õ
+1

-1 
dx e-A log é
ê
ë
1+ 2.912
4pas
A ù
ú
û
(1)
with A = [(p^coshy (1-sv0x))/(TeffÖ[(1-(sv0)2)])], an effective temperature of Teff = 170 MeV and a space-time normalization factor Neff = 3×104 fm4. These parameters are taken from our analysis [2] of dilepton data. Contrary to the SPS dilepton data, flow effects are visible in the photon p^ spectra at values around 2 GeV. With a maximal radial expansion of v0 = 0.3c of the radiating fireball a good description of the data is achieved (see fig. 2).

kaempfer51.gif kaempfer52.gif

Fig. 1 A comparison of calculations of the hard photon production in proton-proton collisions with data from E704 [3] at Ös = 19.4 GeV (small p^ values) and from UA6 [4] at Ös = 24.3 GeV (large p^ values). For more details cf. [5].

Fig. 2 The data of the WA98 collaboration [1] compared with the hard direct photons (dashed curve) and the thermal contribution (thin curve). The sum of these contributions is depicted by the solid curve. A radial flow of v0 = 0.3c is assumed.

1Institute for Theoretical Physics, 252143 Kiev - 143, Ukraine

References

[1] M. M. Aggarwal et al. (WA98), Phys. Rev. Lett 85 (2000) 3595

[2] K. Gallmeister, B. Kämpfer, O.P. Pavlenko, Phys. Lett. 473 (2000) 20

[3] D.L. Adams et al. (E704), Phys. Lett. B 345 (1995) 569

[4] G. Ballocchi et al. (UA6), Phys. Lett. B 317 (1993) 250

[5] K. Gallmeister, B. Kämpfer, O.P. Pavlenko, Phys. Rev. C 62 (2000) 057901


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