2007
DOI: 10.1088/0954-3899/34/9/004
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Covariant description of kinetic freeze-out through a finite time-like layer

Abstract: The Freeze Out (FO) problem is addressed for a covariant FO probability and a finite FO layer with a time-like normal vector continuing the line of studies introduced in Ref. [1]. The resulting post FO momentum distribution functions are presented and discussed. We show that in general the post FO distributions are non-thermal and asymmetric distributions even for time-like FO situations.

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Cited by 15 publications
(34 citation statements)
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“…It is interesting that similar type of gradual development from space-like into time-like regime occurs in the hadronization phase of ultra-relativistic heavy ion collisions [15][16][17][18][19][20][21][22] . If we include radiative heat transfer in our model, the transition from space-like to time-like behavior will be gradual.…”
Section: Analytic Modelmentioning
confidence: 91%
“…It is interesting that similar type of gradual development from space-like into time-like regime occurs in the hadronization phase of ultra-relativistic heavy ion collisions [15][16][17][18][19][20][21][22] . If we include radiative heat transfer in our model, the transition from space-like to time-like behavior will be gradual.…”
Section: Analytic Modelmentioning
confidence: 91%
“…Such simplified models were developed and studied in Refs. [5,7,8,9,10], but all these were missing expansion. Thus, the important question to be studied is whether the important freeze out features, pointed out in the earlier works, are not smeared out by the expansion of the system?…”
Section: Introductionmentioning
confidence: 99%
“…In this Section we present a model for a gradual FO through a finite layer, where the thickness L can be varied from zero to infinity, thus making a bridge between the two extreme schemes [25] and time-like [26] layer; see also [27,28].…”
Section: Introductionmentioning
confidence: 99%
“…In order to get an idea about the physical scales of the total FO time L of the FO layer, we recall that the collision time τ coll between the pions, which are the dominant hadrons, depends on temperature τ coll (T ) = 12 f 4 π /T 5 [35,36,37], where f Here, we will not repeat the theoretical developments of [25,26,27,28] in detail, but should consider the essential steps relevant for our investigations.…”
Section: Introductionmentioning
confidence: 99%
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