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dc.contributor.authorBiondini, S.
dc.contributor.authorBrambilla, N.
dc.contributor.authorEscobedo Espinosa, Miguel
dc.contributor.authorVairo, A.
dc.date.accessioned2017-05-24T07:07:36Z
dc.date.available2017-05-24T07:07:36Z
dc.date.issued2017
dc.identifier.citationBiondini, S., Brambilla, N., Escobedo Espinosa, M., & Vairo, A. (2017). Momentum anisotropy effects for quarkonium in a weakly coupled quark-gluon plasma below the melting temperature. <i>Physical Review D</i>, <i>95</i>(7), Article 074016. <a href="https://doi.org/10.1103/PhysRevD.95.074016" target="_blank">https://doi.org/10.1103/PhysRevD.95.074016</a>
dc.identifier.otherCONVID_27012791
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/54086
dc.description.abstractIn the early stages of heavy-ion collisions, the hot QCD matter expands more longitudinally than transversely. This imbalance causes the system to become rapidly colder in the longitudinal direction, and a local momentum anisotropy appears. In this paper, we study the heavy-quarkonium spectrum in the presence of a small plasma anisotropy. We work in the framework of potential nonrelativistic QCD at finite temperature. We inspect arrangements of nonrelativistic and thermal scales complementary to those considered in the literature. In particular, we consider temperatures larger and Debye masses smaller than the binding energy, which is a temperature range relevant for presently running LHC experiments. In this setting, we compute the leading thermal corrections to the binding energy and the thermal width induced by quarkonium gluodissociation.en
dc.language.isoeng
dc.publisherAmerican Physical Society
dc.relation.ispartofseriesPhysical Review D
dc.subject.otherquarkonium
dc.subject.otheranisotropy
dc.titleMomentum anisotropy effects for quarkonium in a weakly coupled quark-gluon plasma below the melting temperature
dc.typeresearch article
dc.identifier.urnURN:NBN:fi:jyu-201705192429
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosDepartment of Physicsen
dc.type.urihttp://purl.org/eprint/type/JournalArticle
dc.date.updated2017-05-19T15:15:03Z
dc.type.coarhttp://purl.org/coar/resource_type/c_2df8fbb1
dc.description.reviewstatuspeerReviewed
dc.relation.issn2470-0010
dc.relation.numberinseries7
dc.relation.volume95
dc.type.versionpublishedVersion
dc.rights.copyright© 2017 American Physical Society. Published in this repository with the kind permission of the publisher.
dc.rights.accesslevelopenAccessfi
dc.type.publicationarticle
dc.relation.grantnumber303756
dc.subject.ysohiukkasfysiikka
jyx.subject.urihttp://www.yso.fi/onto/yso/p15576
dc.relation.doi10.1103/PhysRevD.95.074016
dc.relation.funderSuomen Akatemiafi
dc.relation.funderResearch Council of Finlanden
jyx.fundingprogramAkatemiatutkijan tutkimuskulut, SAfi
jyx.fundingprogramResearch costs of Academy Research Fellow, AoFen
jyx.fundinginformationThe work of S. B. was partly supported by the Swiss National Science Foundation (SNF) under Grant No. 200020-168988. N. B. and A. V. acknowledge support from DFG Grant No. BR 4058/1-2 “Effective field theories for hard probes of hot plasma” and the DFG cluster of excellence “Origin and structure of the universe” (www.universe-cluster.de). The work of M. A. E. was supported by the European Research Council under Advanced Investigator Grant No. ERC-AD-267258 and by the Academy of Finland, Project No. 303756.
dc.type.okmA1


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