With logarithmic (due to running of the coupling) accuracy the energy density of the resulting medium would scale with the. The energy content is dE = á m t ñ dn, where á m t ñ is the average transverse mass at y = 0, so similarly to Bjorken, the initial energy density is Using the Bjorken hydrodynamical model one obtains an estimate of about 3 GeV pre cubic fermi for the energy density in the early phase of central Pb+Pb collisions. A local maximum is seen at N_part ~ 90, with corresponding energy density based on the Bjorken picture of \epsilon_Bj \tau ~ 2.4 GeV/(fm^2 c) with a transverse area size of 60 fm^2. When viscous corrections are added to Bjorken hydrodynamics, the energy. The energy content is dE = á m t ñ dn, where á m t ñ is the average transverse mass at y = 0, so similarly to Bjorken, the initial energy density is. Ç«Bj, the Bjorken energy density) up to lower SPSenergy. A further increasein collisionen ergy leads to an increase of early temperature andpressureofthesystem.



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