High Level Trigger of Muon Spectrometer Indranil Das Saha Institute of Nuclear Physics.
Shandong University, Qingdao, China · 3. Analysis details γ rich trigger event Purity of direct...
Transcript of Shandong University, Qingdao, China · 3. Analysis details γ rich trigger event Purity of direct...
3. Analysis detailsγrich trigger event
Purity of direct photon for different trigger ETtrig bins
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Au+Au 200 GeV [year 2014], 0%-15% Uncertaintyσ1±
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-Trigger EventgAu+Au 200 GeV [2014], Event number=37362, Run number=15098037
Measurement of semi-inclusive +jet and π0+jet distributions in central Au+Au collisions at GeV by the STAR experiment
γdirsNN = 200
Nihar Ranjan Sahoo, for the STAR Collaboration Shandong University, Qingdao, China
The STAR Collaboration: https://drupal.star.bnl.gov/STAR/presentations/
JetJet
Abstract
2. STAR detector setup1. Motivation
5. SummaryReferences
4. Results and discussion
γdir+jet vs π0+jet: Recoil jet suppression for two jet radii Rjet = 0.2 Rjet = 0.5
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IAAAI Au+Au 200 GeV, 0-15%
= 0.2jet RTanti-kSTAR Preliminary
< 15 GeV/cconst.T
< 11 GeV, ptrigT9 < E
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• Recoil jet with a jet resolution parameter of Rjet =0.2 shows strong suppression whereas anegligible suppression is observed for Rjet=0.5, within uncertainties.
• IAAPYTHIA values are comparable between the two ETtrig bins.• The same level of suppression is seen between γdir+jet and π0+jet for different ETtrig bins andthe two jet resolution parameters within uncertainties.
γrich trigger events: enriched-γdir trigger events with admixtureof photons from π0.
Caption- IAAPYTHIA as a function ofpT,jetch for γdir- (red band) and π0-trigger (blue band). Top: 9 < ETtrig<11 GeV. Bottom: 11 < ETtrig< 15GeV. Lighter and darker bandsrepresent systematic and statisticaluncertainties, respectively.
• A clear difference between recoil-jetspectra for different trigger ET: 9-11GeV and 11-15 GeV.
• Recoil jet pT is suppressed withrespect to PYTHIA8.
• γdir+jet: downward arrow representsupper limit in the yield at: pT,jetch =11 GeV/c for 9-11 GeV, pT,jetch = 15GeV/c for 11-15 GeV.
• Jet quenching is an important signature of the hot and denseQCD matter produced in heavy-ion collisions [1].
• A direct photon (γdir) produced in coincidence with a recoiljet (γdir+jet) is a good probe to study the parton energy loss inthe QGP [2].
• Comparison between γdir+jet vs π0+jet provides quantitativeunderstanding of parton energy loss in the QCD medium
• Energy loss as a function of path length, colorfactor, parton energy, etc.
• Redistribution of lost energy inside the medium; byvarying jet radius
1. J. Adams et al. (STAR Collaboration), Nucl. Phys. A 757, 102 (2005)2. X.-N. Wang, Z. Huang, and I. Sarcevic, Phys. Rev. Lett. 77, 231 (1996)3. L. Adamczyk et al. (STAR Collaboration), Phys. Lett. B 760 (2016) 689-6964. M. Cacciari, G. P. Salam, and G. Soyez, Eur. Phys. J. C (2012) 72:18965. L. Adamczyk et al. (STAR Collaboration), Phys. Rev. C 96 (2017) no.2,
0249056. PYTHIA8: T. Sjöstrand, S. Askb, J. R. Christiansen, et al.,Comput. Phys.
Commun. 191 (2015) 159-177; arXiv:1410.3012; With default setting for π0+jet and γ+jet
Full analysis chain:1. Discrimination between π0/γrich-triggered events
Transverse Shower Profile method [3]2. Recoil charged jets from high-tower-triggered events
Using FastJet package [4]; Recoil jet region:[π-π/4,π+π/4]; Jet radius = 0.2 and 0.5; |ηjet| < 1-R
3. Subtraction of uncorrelated jet background in recoilregion
Based on the mixed-event technique [5]4. Correction for detector and heavy-ion backgroundfluctuations effects using unfolding technique
Factorizing detector and heavy-ion backgroundfluctuation effects5. Conversion from γrich+jet to γdir+jet [4]; as γrich+jetcontains admixture of π0+jet
Using π0+jet yield and purity of γdir6. Major sources of systematic uncertainty
Unfolding, mixed-event normalization region, detectoreffects, γdir background subtraction [contributes only to
γdir+jet]
• Recoil charged jets dominate (above ~10GeV/c) over the uncorrelated jets for differentETtrig bins and jet radii.
• A clear trigger dependence can been seen.
pchT,jet<latexit sha1_base64="eA/vN+HGIBEOXPe77PzZ7X5UhCY=">AAAB+3icbVDLSsNAFJ3UV62vWJduBovgQkqigi6LblxW6AvaGCbTm3bsTBJmJmIJ+RU3LhRx64+482+cPhbaeuDC4Zx7ufeeIOFMacf5tgorq2vrG8XN0tb2zu6evV9uqTiVFJo05rHsBEQBZxE0NdMcOokEIgIO7WB0M/HbjyAVi6OGHifgCTKIWMgo0Uby7XJPCpz4WeP0AXR+n9Fh7tsVp+pMgZeJOycVNEfdt796/ZimAiJNOVGq6zqJ9jIiNaMc8lIvVZAQOiID6BoaEQHKy6a35/jYKH0cxtJUpPFU/T2REaHUWASmUxA9VIveRPzP66Y6vPIyFiWphojOFoUpxzrGkyBwn0mgmo8NIVQycyumQyIJ1SaukgnBXXx5mbTOqu559ezuolK7nsdRRIfoCJ0gF12iGrpFddREFD2hZ/SK3qzcerHerY9Za8GazxygP7A+fwD8u5Rp</latexit>
Y (pchT,jet)p+p
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Y (pchT,jet)Au+Au
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Recoil jet yield suppression withrespect to p+p:
andrepresent recoil jet yield pertrigger as a function of inAu+Au and p+p collisions,respectively, For p+p baseline,PYTHIA8 result is used.
IAA(pchT,jet) =
Y (pchT,jet)Au+Au
Y (pchT,jet)p+p
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We present the semi-inclusive measurement of charged jets recoiling from direct-photon and π0 triggers in central Au+Au collisions at 200 GeV center of mass energy per neucleon, using a datasetwith integrated luminosity 13 nb−1 recorded by the STAR experiment in 2014. The photon and π0 triggers have 9 < ETtrig < 15 GeV. Charged jets are reconstructed with the anti-kT algorithm withresolution parameters R=0.2 and 0.5. A mixed-event technique developed previously by STAR is used to correct the recoil jet yield for uncorrelated background, enabling recoil jet measurementsover a broad pT,jet range with large jet radius. We report the corrected semi-inclusive recoil jet yields for both triggers and compare them to those in p+p collisions. Such measurements have differenttrigger bias, in terms of both the path-length distribution and quark/gluon contributions to the recoil jet population.
MTD TOF Magnet VPD BBC EEMCBEMC TPC
§ Special High Tower trigger for π0/γ event [BEMC] § Discrimination between π0 γγ and γdir
§ By Transverse Shower Profile (TSP) method [3] § Using Barrel Shower Maximum Detector [BSMD]
p+p baseline: PYTHIA8 [6] is used for both triggers
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richg
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< 15 GeV [SE]Ttrig11 < E
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γrich+jet: SE and MEπ0+jet: SE and ME
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preco,chT,jet (= praw,chT,jet � ⇢.A) [GeV/c]
<latexit sha1_base64="3o5THPyQge35D2UbUG4c86OfncQ=">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</latexit>
STAR Preliminary STAR PreliminarySTAR Preliminary
STAR Preliminary
Caption- The reconstructed jet pT,jetreco distributions forthe same event (SE) and mixed event (ME) for twotriggers (ETtrig) bins: 9-11 GeV and 11-15 GeV. Left andright panels are for Rjet =0.2 and 0.5, respectively.Lower panels shows the ratio between SE andnormalized ME.
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γdir+jet: Recoil jet pT spectra
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π0+jet: Recoil jet pT spectra
Rjet = 0.2 Rjet = 0.5 Rjet = 0.2 Rjet = 0.5
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Au+Au 200 GeV, 0-15% Au+Au 200 GeV, 0-15% Au+Au 200 GeV, 0-15% Au+Au 200 GeV, 0-15%
• First γdir+jet and π0+jet measurement at RHIC within 9 < ETtrig < 15 GeV is presented in central Au+Au collisions atcenter of mass energy 200 GeV
• Recoil jet with jet radius 0.2 is strongly suppressed at high jet pT whereas a noticeable recovery of jet energy loss isobserved at jet radius 0.5 for both the γdir and π
0 trigger cases; consistent with the previous h+jet analysis [5]
• Recoil jet suppression is seen to be independent of ETtrig; whereas γdir+jet and π0+jet show similar level of
suppression
Caption- Fully corrected semi-inclusive recoilcharged jet pT,jetch spectra for the above twoETtrig bins. Dashed lines are PYTHIA8expectation. Left panel (Rjet=0.2) and Rightpanel (Rjet=0.5). Lighter (darker) bandsrepresent systematic (statistical) uncertainties.