2007
DOI: 10.1590/s0103-97332007000500026
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Melting rho meson and thermal dileptons

Abstract: We first give a brief survey of theoretical evaluations of light vector mesons in hadronic matter, focusing on results from hadronic many-body theory. We emphasize the importance of imposing model constraints in obtaining reliable results for the in-medium spectral densities. The latter are subsequently applied to the calculation of dilepton spectra in high-energy heavy-ion collisions, with comparisons to recent NA60 data at the CERN-SPS. We discuss aspects of space-time evolution models and the decomposition … Show more

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Cited by 14 publications
(13 citation statements)
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“…In previous works [15,24,36] this was done by running the fireball an extra ∼1 fm/c using the in-medium ρ spectral function. It turns out [19,20], however, that this description of ρ decays at thermal freezeout carries an extra factor of 1/γ relative to a standard blast-wave spectrum of hadrons at thermal freezeout, where γ = q 0 /M is the usual Lorentz factor. Roughly speaking, the inmedium radiation given by Eq.…”
Section: A ρ Mesons At Thermal Freezeoutmentioning
confidence: 99%
See 1 more Smart Citation
“…In previous works [15,24,36] this was done by running the fireball an extra ∼1 fm/c using the in-medium ρ spectral function. It turns out [19,20], however, that this description of ρ decays at thermal freezeout carries an extra factor of 1/γ relative to a standard blast-wave spectrum of hadrons at thermal freezeout, where γ = q 0 /M is the usual Lorentz factor. Roughly speaking, the inmedium radiation given by Eq.…”
Section: A ρ Mesons At Thermal Freezeoutmentioning
confidence: 99%
“…[95]). Specifically, we evaluate the following scenarios, as sum-marized in the six panels of [15][16][17][18][19][20] MeV in the LMR, approximately reflecting the increase in the hadronic fireball temperatures (e.g., T fo = 136 MeV compared to T fo = 120 MeV at thermal freezeout). Scenario EoS-B (b) additionally improves around the ρ peak due to a larger weight of the relatively hard components from decays of freezeout and primordial ρ, since the overall thermal hadronic emission is smaller than for EoS-A and EoS-C (compare Fig.…”
Section: Slope Analysismentioning
confidence: 99%
“…It was seen that a large excess remained after subtracting contributions from expected hadronic (the cocktail) decays. The remaining excess was examined by a number of groups [5,6,7,8,9] and was interpreted by a combination of thermal partonic and hadronic contributions with modifications to the spectral function due to finite temperature and baryon density.…”
Section: Introductionmentioning
confidence: 99%
“…Quantitative theoretical analyses [106,136] are rather involved, see the center and right panels of Fig. 19, especially for momenta above q t ≃ 1 − 1.5 GeV where nonthermal sources are expected to become significant [137], e.g., Drell-Yan dileptons or primordial ρ decays.…”
Section: Lmr-imr Transition: Chiral Mixingmentioning
confidence: 99%