2011
DOI: 10.1103/physrevd.83.026004
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Photoemission rate of strongly interacting quark-gluon plasma at finite density

Abstract: Abstract:We calculate the thermal spectral function of SYM plasma with finite density using holographic technique. The gravity dual of the finite temperature and density is taken as the RN-AdS black hole. In the presence of charge, linearized vector modes of gravitational and electromagnetic perturbation are coupled with each other. By introducing master variables for these modes, we solve the coupled system and calculate spectral function. We also calculate photo-emission rate of our gauge theory plasma from … Show more

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Cited by 13 publications
(14 citation statements)
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“…Our results are quite different from those of Ref. [14] which takes the RN-AdS black hole geometry as the gravity dual of QCD and embeds the baryon charge density in the black hole charge.…”
Section: Soft-wall Ads/qcd Modelcontrasting
confidence: 99%
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“…Our results are quite different from those of Ref. [14] which takes the RN-AdS black hole geometry as the gravity dual of QCD and embeds the baryon charge density in the black hole charge.…”
Section: Soft-wall Ads/qcd Modelcontrasting
confidence: 99%
“…This can also be seen explicitly from plots later in this paper (Figs. 5,8,11,and 14). This proves the claim in Ref.…”
Section: D4/d6 Modelsupporting
confidence: 87%
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