Show simple item record

dc.contributor.authorAndres, C.
dc.contributor.authorArmesto, N.
dc.contributor.authorNiemi, H.
dc.contributor.authorPaatelainen, R.
dc.contributor.authorSalgado, C.
dc.contributor.editord'Enterria, David
dc.contributor.editorMorsch, Andreas
dc.contributor.editorCrochet, Philippe
dc.date.accessioned2019-10-17T08:39:20Z
dc.date.available2019-10-17T08:39:20Z
dc.date.issued2019
dc.identifier.citationAndres, C., Armesto, N., Niemi, H., Paatelainen, R., & Salgado, C. (2019). Constraining energy loss from high-pt azimuthal asymmetries. In D. d'Enterria, A. Morsch, & P. Crochet (Eds.), <i>Hard Probes 2018 : International Conference on Hard and Electromagnetic Probes of High-Energy Nuclear Collisions</i> (Article 070). Sissa Medialab srl. POS Proceedings of Science, 345. <a href="https://doi.org/10.22323/1.345.0070" target="_blank">https://doi.org/10.22323/1.345.0070</a>
dc.identifier.otherCONVID_33248741
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/65927
dc.description.abstractThe nuclear modification factor RAA has been satisfactorily described by various jet quenching models. Nonetheless, all these formalisms, until very recently, underpredicted the high-pT (> 10 GeV) elliptic flow v2. We find that the simultaneous description of these observables requires to strongly suppress the quenching for the first ~ 0.6 fm after the collision. This shows the potential of jet quenching observables to constrain the dynamics of the initial stages of the evolution.en
dc.format.mimetypeapplication/pdf
dc.languageeng
dc.language.isoeng
dc.publisherSissa Medialab srl
dc.relation.ispartofHard Probes 2018 : International Conference on Hard and Electromagnetic Probes of High-Energy Nuclear Collisions
dc.relation.ispartofseriesPOS Proceedings of Science
dc.rightsCC BY-NC-ND 4.0
dc.titleConstraining energy loss from high-pt azimuthal asymmetries
dc.typeconferenceObject
dc.identifier.urnURN:NBN:fi:jyu-201910174499
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosDepartment of Physicsen
dc.type.urihttp://purl.org/eprint/type/ConferencePaper
dc.description.reviewstatuspeerReviewed
dc.relation.issn1824-8039
dc.type.versionpublishedVersion
dc.rights.copyright© Authors, 2019
dc.rights.accesslevelopenAccessfi
dc.relation.conferenceInternational Conference on Hard and Electromagnetic Probes of High-Energy Nuclear Collisions
dc.relation.grantnumber297058
dc.subject.ysoydinfysiikka
dc.subject.ysohiukkasfysiikka
dc.format.contentfulltext
jyx.subject.urihttp://www.yso.fi/onto/yso/p14759
jyx.subject.urihttp://www.yso.fi/onto/yso/p15576
dc.rights.urlhttps://creativecommons.org/licenses/by-nc-nd/4.0/
dc.relation.doi10.22323/1.345.0070
dc.relation.funderSuomen Akatemiafi
dc.relation.funderAcademy of Finlanden
jyx.fundingprogramAkatemiahanke, SAfi
jyx.fundingprogramAcademy Project, AoFen
jyx.fundinginformationWe acknowledge the CSC – IT Center for Science in Espoo, Finland, for the allocation of the computational resources. HN is supported by the Academy of Finland, project 297058. RP is supported by the European Research Council, grant no. 725369. NA and CAS are supported by Ministerio de Ciencia e Innovación of Spain under project FPA2017-83814-P and Unidad de Excelencia María de Maetzu under project MDM-2016-0692, by Xunta de Galicia (Consellería de Educación) and FEDER. This work has been performed in the framework of COST Action CA15213 ‘Theory of hot matter and relativistic heavy-ion collisions’ (THOR).


Files in this item

Thumbnail

This item appears in the following Collection(s)

Show simple item record

CC BY-NC-ND 4.0
Except where otherwise noted, this item's license is described as CC BY-NC-ND 4.0