Abstract
We report the first dijet transverse momentum asymmetry measurements from Au + Au and pp collisions at RHIC. The two highest-energy back-to-back jets reconstructed from fragments with transverse momenta above 2 GeV/c display a significantly higher momentum imbalance in heavy-ion collisions than in the pp reference. When reexamined with correlated soft particles included, we observe that these dijets then exhibit a unique new feature—momentum balance is restored to that observed in pp for a jet resolution parameter of R = 0.4, while rebalancing is not attained with a smaller value of R = 0.2.
Document Type
Article
Publication Date
8-10-2017
Digital Object Identifier (DOI)
https://doi.org/10.1103/PhysRevLett.119.062301
Related Content
See Supplemental Material at http://link.aps.org/supplemental/10.1103/PhysRevLett.119.062301, which includes Refs. [23–29], for an evaluation of instrumental and heavy-ion background effects.
Repository Citation
Adamczyk, L.; Adkins, James K.; Agakishiev, G.; Aggarwal, M. M.; Ahammed, Z.; 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.; 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.; Bunzarov, I.; Butterworth, J.; Fatemi, Renee H.; and Ramachandran, Suvarna, "Dijet Imbalance Measurements in Au + Au and pp Collisions at √sNN = 200 GeV at STAR" (2017). Physics and Astronomy Faculty Publications. 531.
https://uknowledge.uky.edu/physastron_facpub/531
Supplemental Material
Notes/Citation Information
Published in Physical Review Letters, v. 119, issue 6, 062301, p. 1-7.
© 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/PhysRevLett.119.062301
This group of authors is collectively known as the STAR Collaboration.