Intermittency in high-energy collisions and a phase transition in the Feynman-Wilson fluid

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dc.contributor.author Antoniou, NG en
dc.contributor.author Contogouris, AP en
dc.contributor.author Papadopoulos, CG en
dc.contributor.author Vlassopulos, SDP en
dc.date.accessioned 2014-03-01T01:08:54Z
dc.date.available 2014-03-01T01:08:54Z
dc.date.issued 1992 en
dc.identifier.issn 0556-2821 en
dc.identifier.uri https://dspace.lib.ntua.gr/xmlui/handle/123456789/10721
dc.subject High Energy en
dc.subject Phase Transition en
dc.subject.classification Astronomy & Astrophysics en
dc.subject.classification Physics, Particles & Fields en
dc.subject.other RAPIDITY DISTRIBUTIONS en
dc.subject.other MULTIHADRON PRODUCTION en
dc.subject.other PARTICLE-PRODUCTION en
dc.subject.other FLUCTUATIONS en
dc.subject.other PATTERNS en
dc.subject.other PHYSICS en
dc.subject.other LATTICE en
dc.subject.other SPACE en
dc.subject.other PI+P en
dc.subject.other K+P en
dc.title Intermittency in high-energy collisions and a phase transition in the Feynman-Wilson fluid en
heal.type journalArticle en
heal.identifier.primary 10.1103/PhysRevD.45.4034 en
heal.identifier.secondary http://dx.doi.org/10.1103/PhysRevD.45.4034 en
heal.language English en
heal.publicationDate 1992 en
heal.abstract We study the intermittency effect in multihadron production processes as a critical phenomenon reflecting a higher-order quark-hadron phase transition in the hadronization process. We show that the production of a critical Feynman-Wilson fluid, representing the hadronized system at the critical temperature, has a fractal structure in a wide range of scales in the rapidity space. The intermittency pattern is specified by the critical exponent alone and, for each factorial moment, a minimal scale in rapidity emerges below which the power-law behavior breaks down. The relevance of the model for quark-gluon-plasma physics in present and future experiments is also discussed. © 1992 The American Physical Society. en
heal.publisher AMERICAN PHYSICAL SOC en
heal.journalName Physical Review D en
dc.identifier.doi 10.1103/PhysRevD.45.4034 en
dc.identifier.isi ISI:A1992HX37900013 en
dc.identifier.volume 45 en
dc.identifier.issue 11 en
dc.identifier.spage 4034 en
dc.identifier.epage 4045 en

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