Thermal Dilepton Radiation at Intermediate Masses at the CERN-SpS
R. Rapp, E. Shuryak

TL;DR
This paper demonstrates that thermal dilepton radiation from hot, deconfined matter significantly contributes to the intermediate-mass region in heavy-ion collisions at CERN-SpS energies, aligning well with experimental data without requiring additional charm enhancement.
Contribution
It introduces a thermal fireball model showing that thermal dilepton radiation dominates over background processes up to 2 GeV, matching experimental observations.
Findings
Thermal radiation accounts for observed dilepton enhancement.
Early-stage hot matter contributes moderately to dilepton yield.
No need for anomalous open charm enhancement to explain data.
Abstract
We investigate the significance of thermal dilepton radiation in the intermediate-mass region in heavy-ion reactions at CERN-SpS energies. Within a thermal fireball model for the space-time evolution, the radiation from hot matter is found to dominate over hard 'background' processes (Drell-Yan and open charm) up to invariant masses of about 2 GeV, with a rather moderate fraction emerging from early stages with temperatures MeV associated with deconfined matter. Further including a schematic acceptance for the NA50 experiment we find good agreement with the observed enhancement in the region 1.5 GeV~~3 GeV. In particular, there is no need to invoke any anomalous open charm enhancement.
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