Abstract
We present measurements of elliptic flow (ν2) of electrons from the decays of heavy-flavor hadrons (eHF) by the STAR experiment. For Au+Au collisions at √sNN = 200 GeV we report v2, for transverse momentum (pT) between 0.2 and 7 GeV/c, using three methods: the event plane method (v2{EP}), two-particle correlations (v2{2}), and four-particle correlations (v2{4}). For Au+Au collisions at √sNN = 62.4 and 39 GeV we report v2{2} for pT < 2 GeV/c. v2{2} and v2{4} are nonzero at low and intermediate pT at 200 GeV, and v2{2} is consistent with zero at low pT at other energies. The v2{2} at the two lower beam energies is systematically lower than at √sNN = 200 GeV for pT < 1GeV/c. This difference may suggest that charm quarks interact less strongly with the surrounding nuclear matter at those two lower energies compared to √sNN = 200 GeV.
Document Type
Article
Publication Date
3-13-2017
Digital Object Identifier (DOI)
https://doi.org/10.1103/PhysRevC.95.034907
Repository Citation
Adamczyk, L.; Adkins, J. Kevin; Agakishiev, G.; Aggarwal, M. M.; Ahammed, Z.; Ajitanand, N. N.; Alekseev, I.; Anderson, D. M.; Aoyama, R.; Aparin, A.; Arkhipkin, D.; Aschenauer, E. C.; Ashraf, M. U.; Attri, A.; Averichev, G. S.; Bai, X.; Bairathi, V.; Behera, A.; Bellwied, R.; Bhasin, A.; Bhati, A. K.; Bhattarai, P.; Bielcik, J.; Bielcikova, J.; Bland, L. C.; Bordyuzhin, I. G.; Bouchet, J.; Brandenburg, J. D.; Brandin, A. V.; Brown, D.; Fatemi, Renee H.; and Ramachandran, Suvarna, "Elliptic Flow of Electrons from Heavy-Flavor Hadron Decays in Au + Au Collisions at √sNN = 200, 62.4, and 39 GeV" (2017). Physics and Astronomy Faculty Publications. 534.
https://uknowledge.uky.edu/physastron_facpub/534
Notes/Citation Information
Published in Physical Review C, v. 95, issue 3, 034907, p. 1-12.
©2017 American Physical Society
The copyright holder has granted permission for posting the article here.
Due to the large number of authors, only the first 30 and the authors affiliated with the University of Kentucky are listed in the author section above. For the complete list of authors, please download this article or visit: https://doi.org/10.1103/PhysRevC.95.034907
This group of authors is collectively known as the STAR Collaboration.