Basit öğe kaydını göster

dc.contributor.authorArnold, Peter
dc.contributor.authorDogan, Caglar
dc.contributor.authorMoore, Guy D.
dc.date.accessioned2021-03-04T18:36:44Z
dc.date.available2021-03-04T18:36:44Z
dc.date.issued2006
dc.identifier.citationArnold P., Dogan C., Moore G. D. , "Bulk viscosity of high-temperature QCD", PHYSICAL REVIEW D, cilt.74, no.85021, 2006
dc.identifier.issn1550-7998
dc.identifier.othervv_1032021
dc.identifier.otherav_8ba46bb3-7b9f-4037-ae39-a2e50508200e
dc.identifier.urihttp://hdl.handle.net/20.500.12627/94517
dc.identifier.urihttp://prd.aps.org/abstract/PRD/v74/i8/e085021
dc.identifier.urihttps://doi.org/10.1103/physrevd.74.085021
dc.description.abstractWe compute the bulk viscosity zeta of high-temperature QCD to leading order in powers of the running coupling alpha(s)(T). We find that it is negligible compared to shear viscosity eta for any alpha(s) that might reasonably be considered small. The physics of bulk viscosity in QCD is a bit different than in scalar phi(4) theory. In particular, unlike in scalar theory, we find that an old, crude estimate of zeta similar or equal to 15(1/3-v(s)(2))(2)eta gives the correct order of magnitude, where v(s) is the speed of sound. We also find that leading-log expansions of our result for zeta are not accurate except at very small coupling.
dc.language.isoeng
dc.subjectAstronomi ve Astrofizik
dc.subjectTemel Parçacıklar ve Alanlar
dc.subjectTemel Bilimler
dc.subjectFizik
dc.subjectFİZİK, PARTİKLER VE ALANLAR
dc.subjectTemel Bilimler (SCI)
dc.subjectUzay bilimi
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.titleBulk viscosity of high-temperature QCD
dc.typeMakale
dc.relation.journalPHYSICAL REVIEW D
dc.contributor.department, ,
dc.identifier.volume74
dc.identifier.issue8
dc.contributor.firstauthorID1465866


Bu öğenin dosyaları:

DosyalarBoyutBiçimGöster

Bu öğe ile ilişkili dosya yok.

Bu öğe aşağıdaki koleksiyon(lar)da görünmektedir.

Basit öğe kaydını göster