2020
DOI: 10.1016/j.nima.2020.163970
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The STAR event plane detector

Abstract: The Event Plane Detector (EPD) is an upgrade detector to the STAR experiment at RHIC, designed to measure the pattern of forward-going charged particles emitted in a high-energy collision between heavy nuclei. It consists of two highly-segmented discs of 1.2-cm-thick scintillator embedded with wavelength-shifting fiber, coupled to silicon photomultipliers and custom electronics. We describe the general design of the device, its construction, and performance on the bench and in the experiment.

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Cited by 45 publications
(27 citation statements)
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“…For RHIC highest energy and using the STAR detector, we propose a similar investigation to be performed using the first-order spectator event plane from spectator neutrons, measured by the zero-degree calorimeters (ZDC) [54] and the second-order event plane using the new installed Event-Plane-Detector (EPD) [55]. Consequently, we think that conducting a similar experimental study will reveal important information about the elliptic flow fluctuations and will shed light on the ICCING scenario suggested in Reference [50].…”
Section: Introductionmentioning
confidence: 99%
“…For RHIC highest energy and using the STAR detector, we propose a similar investigation to be performed using the first-order spectator event plane from spectator neutrons, measured by the zero-degree calorimeters (ZDC) [54] and the second-order event plane using the new installed Event-Plane-Detector (EPD) [55]. Consequently, we think that conducting a similar experimental study will reveal important information about the elliptic flow fluctuations and will shed light on the ICCING scenario suggested in Reference [50].…”
Section: Introductionmentioning
confidence: 99%
“…Here we use the factor (C Res EP ) to account for the high event-plane resolution provided by the STAR Event Plane Detector (EPD) [36] since 2018, relative to the previously used Beam-Beam Counter (BBC) [37]. For Au+Au collisions at √ s N N = 27 GeV and 10-40% centrality, we obtain k = 3.48 with N BES−I evt = 70M [24], N BES−II evt = 400M [35] and C Res EP = 1.45 [36] (for midcentral collisions). Then the uncertainty projections for d∆v 1 /dy in BES-II, estimated by scaling the corresponding numbers for BES-I with the obtained k factor, are shown by solid green bands in Fig.…”
Section: Energy Namelymentioning
confidence: 99%
“…The main STAR detectors that we have used in our analysis is the Time Projection Chamber (TPC), Time Of Flight (TOF) detector and Event Plane Detectors (EPDs) [5,6]. The TPC is a cylindrical detector having a length of 4.2m and a radius of 4m which surrounds the beam pipe.…”
Section: Star Detectorsmentioning
confidence: 99%