winter workshop in nuclear physics trelawny beach, jamaica march , 2003 steven.manly@rochester
DESCRIPTION
Collective flow with PHOBOS. Steven Manly University of Rochester representing PHOBOS. Why yes, this is a frisbee!. Winter Workshop in Nuclear Physics Trelawny Beach, Jamaica March , 2003 [email protected] http://hertz.pas.rochester.edu/smanly/. - PowerPoint PPT PresentationTRANSCRIPT
March, 2004Winter Workshop - Jamaica - S. Manly 1
Winter Workshop in Nuclear Physics
Trelawny Beach, JamaicaMarch , 2003
[email protected]://hertz.pas.rochester.edu/smanly/
The view from my office webcam: while I’m here working, my group is enjoying spring break in Rochester
Why yes, this is a frisbee!
Collective flow with PHOBOSSteven Manly
University of Rochesterrepresenting
PHOBOS
March, 2004Winter Workshop - Jamaica - S. Manly 2
Collaboration meeting, BNL October 2002
Birger Back, Mark Baker, Maarten Ballintijn, Donald Barton, Russell Betts, Abigail Bickley,
Richard Bindel, Wit Busza (Spokesperson), Alan Carroll, Zhengwei Chai, Patrick Decowski,
Edmundo Garcia, Tomasz Gburek, Nigel George, Kristjan Gulbrandsen, Stephen Gushue,
Clive Halliwell, Joshua Hamblen, Adam Harrington, Conor Henderson, David Hofman, Richard Hollis,
Roman Hołyński, Burt Holzman, Aneta Iordanova, Erik Johnson, Jay Kane, Nazim Khan, Piotr
Kulinich, Chia Ming Kuo, Willis Lin, Steven Manly, Alice Mignerey, Gerrit van Nieuwenhuizen, Rachid
Nouicer, Andrzej Olszewski, Robert Pak, Inkyu Park, Heinz Pernegger, Corey Reed, Michael Ricci,
Christof Roland, Gunther Roland, Joe Sagerer, Iouri Sedykh, Wojtek Skulski, Chadd Smith,
Peter Steinberg, George Stephans, Andrei Sukhanov, Marguerite Belt Tonjes, Adam Trzupek,
Carla Vale, Siarhei Vaurynovich, Robin Verdier, Gábor Veres, Edward Wenger, Frank Wolfs,
Barbara Wosiek, Krzysztof Wožniak, Alan Wuosmaa, Bolek Wysłouch, Jinlong Zhang
ARGONNE NATIONAL LABORATORY BROOKHAVEN NATIONAL LABORATORYINSTITUTE OF NUCLEAR PHYSICS, KRAKOW MASSACHUSETTS INSTITUTE OF TECHNOLOGY
NATIONAL CENTRAL UNIVERSITY, TAIWAN UNIVERSITY OF ILLINOIS AT CHICAGOUNIVERSITY OF MARYLAND UNIVERSITY OF ROCHESTER
March, 2004Winter Workshop - Jamaica - S. Manly 3
Flow in PHOBOSFlow in PHOBOS
March, 2004Winter Workshop - Jamaica - S. Manly 4
coverage
Data at 19.6, 130 and 200 GeV
1m2m
5m
0 1 2 3 4 512345
coverage for vtx at z=0
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Pixelized detector
Hit saturation, grows with occupancy
Sensitivity to flow reduced
Can correct using analogue energy deposition
–or-
measure of occupied and unoccupied pads in local region assuming Poisson statistics
Poisson occupancy Poisson occupancy correctioncorrection
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Acceptance (phase space) weighting
Octagonal detector
Require circular symmetry for equal phase space per pixel
Pixel’s azimuthal phase space coverage depends on location
Relative phase space weight in annular rings = <Nocc>-1
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z
Dilutes the flow signal
Remove Background
Estimate from MC and correct
flow signal
Non-flow background
+
Non-flow Backgrounds
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Background suppression
Works well in Octagon
dE
(keV)
cosh
Background!
Technique does not work in rings because angle of incidence is ~90
Beampipe
Detector
Demand energy deposition be consistent with angle
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RingsN Octagon RingsP
Spec holes
Vtx holes
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Determining the collision point
High Resolution
extrapolate spectrometer tracks
Low Resolution
octagon hit density peaks at vertex z
position
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RingsN Octagon RingsP
Spec holes
Vtx holes
Detector symmetry issues where SPEC vertex efficiency highest
Most data taken with trigger in place to enhance tracking efficiency
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RingsN Octagon RingsP
Offset vtx method
Limited vertex range along z
Subevents for reaction plane evaluation
Good azimuthal symmetry
Fewer events, no 19.6 GeV data
Gap between subevents relatively small
Technique used for published elliptic flow signal at 130 GeV
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RingsN Octagon RingsP
Full acceptance method
Vertex range -10<z<10
Subevents for reaction plane evaluation vary with analysis
Good statistics, 19.6 GeV data available
Gap between subevents large
Requires “hole filling”
Technique used for elliptic and directed flow signal at all energies (only directed flow released to date, elliptic flow coming soon)
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Dealing with the holes
RingsN Octagon RingsP
Inner layer of vertex detector fills holes in top and bottom. Must map hits from Si with different pad pattern and radius onto a “virtual” octagon Si layer
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Dealing with the holes
RingsN Octagon RingsP
Fill spectrometer holes by extrapolating hit density from adjoining detectors onto a virtual Si layer. (Actual spec layer 1 is much smaller than the hole in the octagon.)
March, 2004Winter Workshop - Jamaica - S. Manly 16
RingsN Octagon RingsP
Track-based method
Vertex range -8<z<10
Subevents for reaction plane
Momentum analysis
200 GeV data
Gap between tracks and subevents large
Little/no background
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Directed flow
Charged hadrons
6-55% central AuAu
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v 1
PHOBOS Preliminary
PHOBOS AuAu √sNN=19.6 GeV
NA49 PbPb √sNN=17.2 GeV
Phys.Rev.C68, 034903, 2003
6-55%
MinimumBias
h±
±
19.6 GeV AuAu & 17.2 GeV PbPb
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STAR AuAu 200 GeV 10-70% central
v1 at 200 GeV AuAu:PHOBOS & STARv 1
STAR, PRL 92 (2004) 062301
PHOBOS Preliminary
PHOBOS 6-55% centralh±
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In target frame of reference, directed flow exhibits signal consistent
with limiting fragmentation
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() PHOBOS Preliminary v2200
() PHOBOS v2130
Minimum Bias
h±
v2 vs. at 130 and 200 GeV AuAu
() PRL 89, 222301 (2002)
Hit-based method
() Nucl.Phys. A715 (2003) 611-614
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width of bin
v2 vs. 200 GeV centrality dependence
PHOBOSPreliminary
central 3-15%midcentral 15-25%peripheral 25-50%
Hit-based method
h±
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Track-basedHit-based
peripheral25-50%h±
v 2
PHOBOS Preliminary
Track-basedHit-based
midcentral15-25%h±
v 2
PHOBOS Preliminary
central3-15%h±
Track-basedHit-based
v 2
PHOBOS Preliminary
v2 vs. 200 GeV method comparison
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Combined hit (offset vertex) and track based
results for v2 vs. || at 200 GeV (Au-Au)
March, 2004Winter Workshop - Jamaica - S. Manly 25
Preliminary
PHOBOS 200 GeV0-55% central
track-based methodv 2
pt (GeV/c)• Nucl.Phys. A715 (2003) 611-614
h± STAR 130 GeV 4-cumulant
STAR 130 GeV 2-cumulant
STAR 130 GeV Reaction Plane5-53% central
Preliminary
PHOBOS 200 GeV0-55% central
pt (GeV/c)
v 2v2 vs. pt AuAu
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STAR 130 GeV 4-cumulant
STAR 130 GeV 2-cumulant
STAR 130 GeV Reaction Plane5-53% central
Preliminary
PHOBOS 200 GeV0-55% central
pt (GeV/c)
v 2PHOBOS signal not pt weighted, thus dominated by low pt
hits where STAR 2- and 4-particle cumulants have small absolute difference
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y vs.
Get a suppression in the spectra which is largest at low pt and small ||. It vanishes at large || and high pt.
Gives the famous dip in multiplicity distribution.
If integrating v2 over pt, get suppression of the lower pt part (where v2 is small) and the signal should rise.
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Transformation of spectra from to y leads to
suppression of multiplicity at low pt and low ||
This leads to an enhancement of inclusive v2
at mid-
P. Kolb, Proc. of 17th Winter Workshop on Nuclear Dynamics (2001)
T. Hirano, BNL-Riken Workshop on Collective Flow and the QGP (Nov. 2003)
~10%
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Limiting fragmentation of elliptic flow
PHOBOS Preliminary v2200
PHOBOS v2130
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Scaled by “Kolb factor”
Limiting fragmentation of elliptic flow
PHOBOS Preliminary v2200
PHOBOS v2130
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Conclusions Directed flow measured at 19.6, 130 and 200 GeV
Mild disagreement with STAR about || where v1 kicks in, but both see flat slope at mid-
v1 shows a limiting fragmentation behavior similar to the multiplicity
v2() hit and track results agree. Likely there is very little non-flow correlations. Expect only small difference between v2() and v2(y).
Hint of limiting fragmentation behavior in v2. Expect better results on this soon