2000
DOI: 10.1103/physrevd.62.076004
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Nonlinear evolution of the momentum dependent condensates in strong interaction: The “pseudoscalar laser”

Abstract: We discuss the relaxation of the scalar and pseudoscalar condensates after a rapid quench from an initial state with fluctuations. If we include not only the zero-mode but also higher modes of the condensates in the classical evolution, we observe parametric amplification of those "hard" modes. Thus, they couple nonlinearly to the "soft" modes. As a consequence, domains of coherent π-field emerge long after the initial spinodal decomposition. The momentum-space distribution of pions emerging from the decay of … Show more

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Cited by 9 publications
(7 citation statements)
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“…We employed the same small grid spacing ∆x = 0.3 fm as for the fluid. Although the mean fields vary on a larger scale, it is important to allow for non-linear amplification of harder fluctuations which can couple to the soft modes and affect the dynamical relaxation to the vacuum state with broken symmetry, see for example [36] and [37].…”
Section: Numerics and Technical Detailsmentioning
confidence: 99%
“…We employed the same small grid spacing ∆x = 0.3 fm as for the fluid. Although the mean fields vary on a larger scale, it is important to allow for non-linear amplification of harder fluctuations which can couple to the soft modes and affect the dynamical relaxation to the vacuum state with broken symmetry, see for example [36] and [37].…”
Section: Numerics and Technical Detailsmentioning
confidence: 99%
“…In this sense our study is close to the real world. As a consequence, the pion production in our model is not as pronounced as in other models [6,9,10]. However, the momentum distribution of the produced pions possesses fingerprints of the zone structure of the amplification regions in momentum space: a cluster of pions with low momenta is formed.…”
Section: Discussionmentioning
confidence: 57%
“…These initial conditions differ from the ones assumed for particle production through inflaton decay in cosmology [8], and in some works on QCD [9,10], as in those cases the initial particle number is taken to be zero.…”
Section: Initial Conditionsmentioning
confidence: 99%
“…The study of parametric resonance at finite temperature in chiral phase transition has never been examined, while that at zero temperature [1][2][3][4][5][6][7] has been performed. Parametric resonance may occur even when the temperature is not zero if the condensates moves periodically like a sine function.…”
Section: Introductionmentioning
confidence: 99%