Freeze out of the expanding system
arXiv:nucl-th/0702069 · doi:10.1140/epja/i2006-10280-8
Abstract
The freeze out (FO) of the expanding systems, created in relativistic heavy ion collisions, is discussed. We start with kinetic FO model, which realizes complete physical FO in a layer of given thickness, and then combine our gradual FO equations with Bjorken type system expansion into a unified model. We shall see that the basic FO features, pointed out in the earlier works, are not smeared out by the expansion.
3 pages, 2 figures
References in corpus (6)
- An unusual space-time evolution for heavy ion collisions at high energies due to the QCD phase transition
- Freeze out in hydrodynamical models
- Non-ideal Particle Distributions from Kinetic Freeze Out Models
- Covariant description of kinetic freeze out through a finite space-like layer
- Non-equilibrated post freeze out distributions
- Modified Boltzmann Transport Equation
Cited by in corpus (7)
- Viscous evolution of the rapidity distribution of matter created in relativistic heavy-ion collisions
- Matching Stages of Heavy Ion Collision Models
- Observables from a solution of 1+3 dimensional relativistic hydrodynamics
- Covariant description of kinetic freeze out through a finite time-like layer
- Anti-Proton Evolution in Little Bangs and Big Bang
- Kinetic description of particle emission from expanding source
- Pion Mass Shift and the Kinetic Freeze Out Process