Cooper–Frye formula and non-extensive coalescence at RHIC energy

Transverse spectra are calculated for various types of hadrons stemming from AuAu collisions at s=200 GeV. We utilize a quark recombination model based on generalized Boltzmann–Gibbs thermodynamics for local hadron production at various break-up scenarios.

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Bibliographic Details
Published inPhysics letters. B Vol. 689; no. 1; pp. 14 - 17
Main Authors ÜRMÖSSY, K, BIRO, T. S
Format Journal Article
LanguageEnglish
Published Kidlington Elsevier B.V 17.05.2010
Elsevier
Subjects
Coalescence
Coalescing
Cooper–Frye
Elementary particles
Energy (nuclear)
Exact sciences and technology
Hadrons
Mathematical models
Non-extensive
Nuclear physics
Physics
Recombination
Spectra
Stemming
The physics of elementary particles and fields
Non-extensive
Recombination
Coalescence
Cooper–Frye
Hadrons
Thermodynamics
Quark model
Hadron production
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Summary:Transverse spectra are calculated for various types of hadrons stemming from AuAu collisions at s=200 GeV. We utilize a quark recombination model based on generalized Boltzmann–Gibbs thermodynamics for local hadron production at various break-up scenarios.
Bibliography:ObjectType-Article-2
SourceType-Scholarly Journals-1
ObjectType-Feature-1
content type line 23
ISSN:0370-2693
1873-2445
DOI:10.1016/j.physletb.2010.04.037