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Azimuthal di-hadron correlations in d+ Au and Au + Au collisions at √sNN=200 GeV measured at the STAR detector

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Title: Azimuthal di-hadron correlations in d+ Au and Au + Au collisions at √sNN=200 GeV measured at the STAR detector
Author: Aggarwal, M.; Ahammed, Z.; Alakhverdyants, A.; Alekseev, I.; Alford, J.; Anderson, B.; Arkhipkin, D.; Averichev, G.; Balewski, J.; Barnby, L.; Baumgart, S.; Beavis, D.; Bellwied, R.; Betancourt, M.; Betts, R.; Bhasin, A.; Bhati, A.; Bichsel, H.; Bielcik, J.; Bielcikova, J.; Biritz, B.; Bland, L.; Bonner, B.; Bouchet, J.; Braidot, E.; Brandin, A.; Bridgeman, A.; Bruna, E.; Bueltmann, S.; Bunzarov, I. ... [more in full view]
Department: Massachusetts Institute of Technology. Laboratory for Nuclear Science; Massachusetts Institute of Technology. Dept. of Physics; Bates Linear Accelerator Center
Publisher: American Physical Society
Issue Date: 2010-08
Abstract: Yields, correlation shapes, and mean transverse momenta pT [rho tau] of charged particles associated with intermediate- to high-pT [rho tau] trigger particles (2.5<pT[rho tau]<10 GeV/c) in d+ Au and Au + Au collisions at √[square root]sNN=200 GeV are presented. For associated particles at higher pT [rho tau] ≳2.5 GeV/c, narrow correlation peaks are seen in d+ Au and Au + Au, indicating that the main production mechanism is jet fragmentation. At lower associated particle pT [rho tau] <2 GeV/c, a large enhancement of the near- (Δϕ~0[delta phi~0]) and away-side (Δϕ~π [delta phi~pi]) associated yields is found, together with a strong broadening of the away-side azimuthal distributions in Au + Au collisions compared to d+ Au measurements, suggesting that other particle production mechanisms play a role. This is further supported by the observed significant softening of the away-side associated particle yield distribution at Δϕ~π [delta phi~pi] in central Au + Au collisions.
URI: http://hdl.handle.net/1721.1/60884
ISSN: 0556-2813
Citation: Aggarwal, M. et al. “Azimuthal di-hadron correlations in d+ Au and Au + Au collisions at sqrt[s_{NN}]=200 GeV measured at the STAR detector.” Physical Review C 82.2 (2010): n. pag. © 2010 The American Physical Society
Version: Final published version
Terms of Use: Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.
Published as: http://dx.doi.org/10.1103/PhysRevC.82.024912
Journal: Physical review C

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