Strangeness production in high-energy collisions and Hawking-Unruh radiation

dc.AffiliationOctober University for modern sciences and Arts (MSA)
dc.contributor.authorTawfik, Abdel Nasser
dc.contributor.authorYassin, Hayam
dc.contributor.authorElyazeed, Eman R. Abo
dc.date.accessioned2019-11-16T08:51:20Z
dc.date.available2019-11-16T08:51:20Z
dc.date.issued2017
dc.descriptionAccession Number: WOS:000396167500003en_US
dc.description.abstractThe assumption that the production of quark-antiquark pairs and their sequential string-breaking takes place, likely as a tunneling process, through the event horizon of the color confinement determines the freezeout temperature and gives a plausible interpretation for the thermal pattern of elementary and nucleus-nucleus collisions. When relating the black-hole electric charges to the baryon-chemical potentials, it was found that the phenomenologically deduced parameters from the ratios of various particle species and the higher-order moments of net-proton multiplicity in the statistical thermal models and Polyakov linear-sigma model agree well with the ones determined from the thermal radiation from charged black hole. Accordingly, the resulting freezeout conditions, such as normalized entropy density s/T-3 = 7 and average energy per particle < E > / < N > similar or equal to 1 GeV, are confirmed at finite chemical potentials as well. Furthermore, the problem 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 (K+/pi(+)), phi-to-kaon (phi/K-) and antilambda-to-pion ((Lambda) over bar/pi(-)) 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) over bar / pi(-), there is an increase with increasing root sNN, i.e., no saturation is to be observed.en_US
dc.description.sponsorshipWORLD SCIENTIFIC PUBL. CO. PTE LTDen_US
dc.identifier.doihttps://doi.org/10.1142/S021830131750001X
dc.identifier.issn1793-6608
dc.identifier.otherhttps://doi.org/10.1142/S021830131750001X
dc.identifier.urihttps://www.worldscientific.com/doi/abs/10.1142/S021830131750001X
dc.language.isoenen_US
dc.publisherWORLD SCIENTIFIC PUBL. CO. PTE LTDen_US
dc.relation.ispartofseriesINTERNATIONAL JOURNAL OF MODERN PHYSICS E-NUCLEAR PHYSICS;Volume: 26 Issue: 3
dc.relation.urihttps://cutt.ly/PeGUZs1
dc.subjectUniversity of Evaporation of black holeen_US
dc.subjectthermodynamics of black holesen_US
dc.subjectstrangeness particleen_US
dc.titleStrangeness production in high-energy collisions and Hawking-Unruh radiationen_US
dc.typeArticleen_US

Files

Original bundle

Now showing 1 - 1 of 1
Loading...
Thumbnail Image
Name:
avatar_scholar_256.png
Size:
6.31 KB
Format:
Portable Network Graphics
Description: