dc.contributor.author | Biondini, S. | |
dc.contributor.author | Brambilla, N. | |
dc.contributor.author | Escobedo Espinosa, Miguel | |
dc.contributor.author | Vairo, A. | |
dc.date.accessioned | 2017-05-24T07:07:36Z | |
dc.date.available | 2017-05-24T07:07:36Z | |
dc.date.issued | 2017 | |
dc.identifier.citation | Biondini, 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.other | CONVID_27012791 | |
dc.identifier.uri | https://jyx.jyu.fi/handle/123456789/54086 | |
dc.description.abstract | In 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.iso | eng | |
dc.publisher | American Physical Society | |
dc.relation.ispartofseries | Physical Review D | |
dc.subject.other | quarkonium | |
dc.subject.other | anisotropy | |
dc.title | Momentum anisotropy effects for quarkonium in a weakly coupled quark-gluon plasma below the melting temperature | |
dc.type | research article | |
dc.identifier.urn | URN:NBN:fi:jyu-201705192429 | |
dc.contributor.laitos | Fysiikan laitos | fi |
dc.contributor.laitos | Department of Physics | en |
dc.type.uri | http://purl.org/eprint/type/JournalArticle | |
dc.date.updated | 2017-05-19T15:15:03Z | |
dc.type.coar | http://purl.org/coar/resource_type/c_2df8fbb1 | |
dc.description.reviewstatus | peerReviewed | |
dc.relation.issn | 2470-0010 | |
dc.relation.numberinseries | 7 | |
dc.relation.volume | 95 | |
dc.type.version | publishedVersion | |
dc.rights.copyright | © 2017 American Physical Society. Published in this repository with the kind permission of the publisher. | |
dc.rights.accesslevel | openAccess | fi |
dc.type.publication | article | |
dc.relation.grantnumber | 303756 | |
dc.subject.yso | hiukkasfysiikka | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p15576 | |
dc.relation.doi | 10.1103/PhysRevD.95.074016 | |
dc.relation.funder | Suomen Akatemia | fi |
dc.relation.funder | Research Council of Finland | en |
jyx.fundingprogram | Akatemiatutkijan tutkimuskulut, SA | fi |
jyx.fundingprogram | Research costs of Academy Research Fellow, AoF | en |
jyx.fundinginformation | The 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.okm | A1 | |