dc.contributor.author | Andres, C. | |
dc.contributor.author | Armesto, N. | |
dc.contributor.author | Niemi, H. | |
dc.contributor.author | Paatelainen, R. | |
dc.contributor.author | Salgado, C. | |
dc.contributor.editor | d'Enterria, David | |
dc.contributor.editor | Morsch, Andreas | |
dc.contributor.editor | Crochet, Philippe | |
dc.date.accessioned | 2019-10-17T08:39:20Z | |
dc.date.available | 2019-10-17T08:39:20Z | |
dc.date.issued | 2019 | |
dc.identifier.citation | Andres, 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.other | CONVID_33248741 | |
dc.identifier.uri | https://jyx.jyu.fi/handle/123456789/65927 | |
dc.description.abstract | The 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.mimetype | application/pdf | |
dc.language | eng | |
dc.language.iso | eng | |
dc.publisher | Sissa Medialab srl | |
dc.relation.ispartof | Hard Probes 2018 : International Conference on Hard and Electromagnetic Probes of High-Energy Nuclear Collisions | |
dc.relation.ispartofseries | POS Proceedings of Science | |
dc.rights | CC BY-NC-ND 4.0 | |
dc.title | Constraining energy loss from high-pt azimuthal asymmetries | |
dc.type | conferenceObject | |
dc.identifier.urn | URN:NBN:fi:jyu-201910174499 | |
dc.contributor.laitos | Fysiikan laitos | fi |
dc.contributor.laitos | Department of Physics | en |
dc.type.uri | http://purl.org/eprint/type/ConferencePaper | |
dc.type.coar | http://purl.org/coar/resource_type/c_5794 | |
dc.description.reviewstatus | peerReviewed | |
dc.relation.issn | 1824-8039 | |
dc.type.version | publishedVersion | |
dc.rights.copyright | © Authors, 2019 | |
dc.rights.accesslevel | openAccess | fi |
dc.relation.conference | International Conference on Hard and Electromagnetic Probes of High-Energy Nuclear Collisions | |
dc.relation.grantnumber | 297058 | |
dc.subject.yso | ydinfysiikka | |
dc.subject.yso | hiukkasfysiikka | |
dc.format.content | fulltext | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p14759 | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p15576 | |
dc.rights.url | https://creativecommons.org/licenses/by-nc-nd/4.0/ | |
dc.relation.doi | 10.22323/1.345.0070 | |
dc.relation.funder | Research Council of Finland | en |
dc.relation.funder | Suomen Akatemia | fi |
jyx.fundingprogram | Academy Project, AoF | en |
jyx.fundingprogram | Akatemiahanke, SA | fi |
jyx.fundinginformation | We 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). | |
dc.type.okm | A4 | |