Strangeness production in high-energy collisions and Hawking-Unruh radiation
Abdel Nasser Tawfik; Hayam Yassin; Eman R. Abo Elyazeed;
Abstract
The assumption that the production of quark-antiquark pairs and their
sequential string-breaking taking place through the event horizon of the color
confinement determines freezeout temperature and gives a plausible
interpretation of the thermal pattern of pp and AA collisions. When relating
the black-hole electric charges to the baryon-chemical potentials it was found
that the phenomenologically-deduced parameters from various particle ratios in
the statistical thermal models agree well with the ones determined from the
thermal radiation from charged black-hole. Accordingly, the resulting freezeout
conditions, such as $s/T^3=7$ and $/=1~$GeV, are confirmed at finite
chemical potentials, as well. Furthermore, the problematic of strangeness
production in elementary collisions can be interpreted by thermal particle
production from the Hawking-Unruh radiation. Consequently, the freezeout
temperature depends on the quark masses. This leads to a deviation from full
equilibrium and thus a suppression of the strangeness production in the
elementary collisions. But in nucleus-nucleus collisions, an average
temperature should be introduced in order to dilute the quark masses. This
nearly removes the strangeness suppression. An extension to finite chemical
potentials is introduced. The particle ratios of kaon-to-pion, phi-to-kaon and
antilambda-to-pion are determined from Hawking-Unruh radiation and compared
with the thermal calculations and the measurements in different experiments. We
conclude that these particle ratios can be reproduced, at least qualitatively,
as Hawking-Unruh radiation at finite chemical potential. With increasing
energy, both K+/pi+ and phi/K^- keep their maximum values at low SPS energies.
But the further energy decrease rapidly reduces both ratios. For Lambda/pi-,
there is an increase with increasing collision energy, i.e. no saturation is to
be observed.
sequential string-breaking taking place through the event horizon of the color
confinement determines freezeout temperature and gives a plausible
interpretation of the thermal pattern of pp and AA collisions. When relating
the black-hole electric charges to the baryon-chemical potentials it was found
that the phenomenologically-deduced parameters from various particle ratios in
the statistical thermal models agree well with the ones determined from the
thermal radiation from charged black-hole. Accordingly, the resulting freezeout
conditions, such as $s/T^3=7$ and $
chemical potentials, as well. Furthermore, the problematic of strangeness
production in elementary collisions can be interpreted by thermal particle
production from the Hawking-Unruh radiation. Consequently, the freezeout
temperature depends on the quark masses. This leads to a deviation from full
equilibrium and thus a suppression of the strangeness production in the
elementary collisions. But in nucleus-nucleus collisions, an average
temperature should be introduced in order to dilute the quark masses. This
nearly removes the strangeness suppression. An extension to finite chemical
potentials is introduced. The particle ratios of kaon-to-pion, phi-to-kaon and
antilambda-to-pion are determined from Hawking-Unruh radiation and compared
with the thermal calculations and the measurements in different experiments. We
conclude that these particle ratios can be reproduced, at least qualitatively,
as Hawking-Unruh radiation at finite chemical potential. With increasing
energy, both K+/pi+ and phi/K^- keep their maximum values at low SPS energies.
But the further energy decrease rapidly reduces both ratios. For Lambda/pi-,
there is an increase with increasing collision energy, i.e. no saturation is to
be observed.
Other data
Title | Strangeness production in high-energy collisions and Hawking-Unruh radiation | Authors | Abdel Nasser Tawfik ; Hayam Yassin ; Eman R. Abo Elyazeed | Keywords | Physics - General Physics;Physics - General Physics;High Energy Physics - Phenomenology | Issue Date | 8-Dec-2016 | Journal | Int. J. Mod. Phys. E 26, (2017) 1750001 | DOI | 03 1750001 http://arxiv.org/abs/1612.05105v1 26 10.1142/S021830131750001X |
Scopus ID | 2-s2.0-85009948872 |
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