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Anisotropic Hydrodynamics for Au-Au Collisions at 200 GeV
Open AccessProceedings

Open Bottom Production in Au Au Collisions at √sNN = 200 GeV with the STAR Experiment

by 1,2,3
1
Department of Modern Physics, University of Science and Technology of China (USTC), Hefei 230026, China
2
Department of Radiology, Lanzhou University Second Hospital, Lanzhou 730030, China
3
Key Laboratory of Medical Imaging of Gansu Province, Lanzhou 730030,China
Presented at Hot Quarks 2018—Workshop for young scientists on the physics of ultrarelativistic nucleus-nucleus collisions, Texel, The Netherlands, 7–14 September 2018.
Proceedings 2019, 10(1), 39; https://doi.org/10.3390/proceedings2019010039
Published: 24 April 2019
In these proceedings, we present measurements of open bottom hadron production through multiple decay channels in Au + Au collisions at s NN = 200 GeV by the STAR experiment. Specifically, measurements of nuclear modification factors for electrons, J / ψ , and D 0 from open bottom hadron decays, enabled by the Heavy Flavor Tracker, are shown. A large suppression for non-prompt J / ψ and non-prompt D 0 are observed at high transverse momenta. On the other hand, there seems to be less suppression for electrons from bottom hadron decays than for those from charm hadron decays at ∼ 2 σ significance level.
Keywords: open bottom production; nuclear modification factors; non-prompt J/ψ; non-prompt D0; electrons from bottom hadron decays; quark-gluon plasma open bottom production; nuclear modification factors; non-prompt J/ψ; non-prompt D0; electrons from bottom hadron decays; quark-gluon plasma
MDPI and ACS Style

Zhang, S. Open Bottom Production in Au Au Collisions at √sNN = 200 GeV with the STAR Experiment. Proceedings 2019, 10, 39. https://doi.org/10.3390/proceedings2019010039

AMA Style

Zhang S. Open Bottom Production in Au Au Collisions at √sNN = 200 GeV with the STAR Experiment. Proceedings. 2019; 10(1):39. https://doi.org/10.3390/proceedings2019010039

Chicago/Turabian Style

Zhang, Shenghui. 2019. "Open Bottom Production in Au Au Collisions at √sNN = 200 GeV with the STAR Experiment" Proceedings 10, no. 1: 39. https://doi.org/10.3390/proceedings2019010039

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