Constraining the initial conditions and temperature dependent viscosity with three-particle correlations in Au+Au collisions

STAR Collaboration

Research output: Contribution to journalArticlepeer-review

2 Scopus citations

Abstract

We present three-particle mixed-harmonic correlations 〈cos⁡(mϕa+nϕb−(m+n)ϕc)〉 for harmonics m,n=1−3 for charged particles in sNN=200 GeV Au+Au collisions at RHIC. These measurements provide information on the three-dimensional structure of the initial collision zone and are important for constraining models of a subsequent low-viscosity quark–gluon plasma expansion phase. We investigate correlations between the first, second and third harmonics predicted as a consequence of fluctuations in the initial state. The dependence of the correlations on the pseudorapidity separation between particles show hints of a breaking of longitudinal invariance. We compare our results to a number of state-of-the art hydrodynamic calculations with different initial states and temperature dependent viscosities. These measurements provide important steps towards constraining the temperature dependent viscosity and longitudinal structure of the initial state at RHIC.

Original languageEnglish
Pages (from-to)81-88
Number of pages8
JournalPhysics Letters B
Volume790
DOIs
StatePublished - Mar 10 2019
Externally publishedYes

Funding

We thank Gabriel Denicol, Jean-Yves Ollitrault, Jacquelyn Noronha-Hostler, Harri Niemi, Risto Paatelainen, Björn Schenke, Chun Shen, Yifeng Sun, Derek Teaney and Li Yan for providing their model predictions and helpful discussions. We thank the RHIC Operations Group and RCF at BNL, the NERSC Center at LBNL, and the Open Science Grid consortium for providing resources and support. This work was supported in part by the Office of Nuclear Physics within the U.S. DOE Office of Science, the U.S. National Science Foundation, the Ministry of Education and Science of the Russian Federation, National Natural Science Foundation of China, Chinese Academy of Sciences, the Ministry of Science and Technology of the People's Republic of China and Ministry of Education of the People's Republic of China, the National Research Foundation of Korea, Czech Science Foundation and Ministry of Education, Youth and Sports of the Czech Republic, Department of Atomic Energy and Department of Science and Technology of the Government of India, the National Science Centre of Poland, the Ministry of Science, Education and Sports of the Republic of Croatia, ROSATOM of Russia and German Bundesministerium für Bildung, Wissenschaft, Forschung und Technologie (BMBF) and the Helmholtz Association. We thank Gabriel Denicol, Jean-Yves Ollitrault, Jacquelyn Noronha-Hostler, Harri Niemi, Risto Paatelainen, Björn Schenke, Chun Shen, Yifeng Sun, Derek Teaney and Li Yan for providing their model predictions and helpful discussions. We thank the RHIC Operations Group and RCF at BNL, the NERSC Center at LBNL, and the Open Science Grid consortium for providing resources and support. This work was supported in part by the Office of Nuclear Physics within the U.S. DOE Office of Science , the U.S. National Science Foundation , the Ministry of Education and Science of the Russian Federation , National Natural Science Foundation of China , Chinese Academy of Sciences , the Ministry of Science and Technology of the People's Republic of China and Ministry of Education of the People's Republic of China , the National Research Foundation of Korea , Czech Science Foundation and Ministry of Education, Youth and Sports of the Czech Republic, Department of Atomic Energy and Department of Science and Technology of the Government of India , the National Science Centre of Poland , the Ministry of Science, Education and Sports of the Republic of Croatia, ROSATOM of Russia and German Bundesministerium für Bildung, Wissenschaft, Forschung und Technologie (BMBF) and the Helmholtz Association .

FundersFunder number
National Science Foundation1614545
National Science Foundation
Office of Science
Nuclear Physics
Department of Science and Technology, Ministry of Science and Technology, India
Department of Atomic Energy, Government of India
National Natural Science Foundation of China
Ministerstvo Školství, Mládeže a Tělovýchovy
Grantová Agentura České Republiky
Ministry of Education of the People's Republic of China
Bundesministerium für Bildung und Forschung
Chinese Academy of Sciences
Ministry of Science and Technology of the People's Republic of China
Ministarstvo Obrazovanja, Znanosti i Sporta
Ministry of Education and Science of the Russian Federation
National Research Foundation of Korea
Narodowe Centrum Nauki
Ministarstvo Znanosti, Obrazovanja i Sporta
State Atomic Energy Corporation ROSATOM
Helmholtz Association
Bundesministerium für Bildung, Wissenschaft, Forschung und Technologie

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