rhic experimental program - background in preparation for meeting
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Hard Probes 2004 Lisbon, Portugal. RHIC Experimental Program - Background in preparation for meeting. Wit Busza MIT. - PowerPoint PPT PresentationTRANSCRIPT
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RHIC Experimental Program-Background in preparation for meeting
Wit Busza
MIT
Hard Probes 2004
Lisbon, Portugal
Many thanks to Michael Miller for help in preparation of this talk, to Conor Henderson for making some of the transparencies, and to the four RHIC collaborations for most of the material presented in the talk.
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The Relativistic Heavy Ion Collider at BNL
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RHIC First Commissioned, June 2000
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2000-2004 RHIC PERFORMANCE
Phenix 1370 b-1
Star 1270 b-1
Phobos 560 b-1 Brahms 540 b-1
56GeV/u
RHIC Run Colliding System √sNN
1
Au+Au
Au+Au
55.87GeV
130.4GeV
2
Au+Au
Au+Au
Au+Au
p+p
130.4GeV
200.0GeV
19.59GeV
200.0GeV
3
d+Au
p+p
200.7GeV
200.0GeV
4
Au+Au
Au+Au
p+p
200.0GeV
62.40GeV
200.0GeV
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THE DETECTORS
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Coils Magnet
E-M Calorimeter
Time of Flight
Projection Chamber
STAR Solenoidal field, large- tracking
TPC’s, Si-vertex trackingRICH, TOF, large EM Cal
~420 participants
PHENIXAxial field, high resolution & rates
2 central arms, 2 forward muon arms TEC, RICH, EM Cal, Si, TOF, -ID
~450 participants
The Two Large Detectors
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BRAHMS2 “conventional” spectrometers
Multiplicity detector with large phase space coverage
Magnets, TPCs, TOF, RICH~40 participants
PHOBOS“Table-top” 2-arm spectrometer
full phase space multiplicity measurementMagnet, Si pad detectors, TOF+dE/dx
~70 participants
Spectrometer
Paddle Trigger Counter
137000 Silicon Pad ChannelsT0 counter
NIM A 499, 603-623 (2003)
Time of Flight
Calorimeters
Octagon
The Two Small Detectors
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High Multiplicity Au+Au Collision at sNN=130 GeV
colors ~ momentum: low - - - high
STARSTAR
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PHOBOS PID & ACCEPTANCE
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Measured Quantities
Single Particles
Tracking p
time of flight, massdx
dE } P
Event Characteristics
Forward Neutral Energy
d 2nch
dd
dET
dd }
nchtotal
ETtotal}
“spectators”
Centrality or impact parameter, b
[“Npart”, “Ncoll”]
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“Spectators”
Zero-degreeCalorimeter
specpart 2 NAN
Paddle Counter
“Participants”
Experimental Control of Centrality or Impact Parameter
“Spectators”
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Bi-product: Study of Mechanism of Particle Production
See, for example, W. Busza arXiv: nucl-ex/0410035
Aim of Research:
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Too good to be true!
From Harris and MuellerAnn. Rev. Nucl. Sci. 1996
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But RHIC program is an incredible success
RIKEN BNL Workshop May 14-15, 2004
Submitted to NPA 2004
New Discoveries at RHICA RIKEN BNL Research Center Workshop, May 14-15, 2004
Proceedings, Volume 62, BNL-72391-2004
BRAHMS, Phenix, Phobos & STAR “White Papers”:
“Perspectives on Discoveries at RHIC”
To be submitted to NPA November, 2004BRAHMS arXiv: nucl-ex/0410020
Phenix arXiv: nucl-ex/0410003
Phobos arXiv: nucl-ex/0410022
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Where Are We Now?
In Au + Au Collisions at RHIC
1. In 1 fm/c energy density≥3GeV/fm3
2. Description of the created system in terms of simple hadronic degrees of freedom is inappropriate3. Constituents of this novel system are found to interact very strongly
In addition large body of high quality data has been collected on a broad range of topics. Much of it is not well understood. Phenomenology is often simpler than the interpretations.
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PHOBOS
PHOBOS
Global Properties
PHOBOS
Data smooth as a function of energy
Pseudorapidity plotted in rest frame of one of the nuclei
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TOTAL CHARGED MULTIPLICITY
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Elliptic Flow
PHOBOS nucl-ex/0406021 Au+Au 0-40%
Elli
pti
c F
low
Pseudorapidity plotted in rest frame of one of the nuclei
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Data smooth as a function of centrality or impact parameter
Total number of particles PHOBOS
Mid rapidity density
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NA49 (from Agnes Richard)
NA50 Experiment
SOME EXCEPTIONS:
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Although in the RHIC Energy Range (20-200 GeV) there are no obvious discontinuities, with very
reasonable assumptions we can conclude
Time of equilibration is short
Energy Density is very high,
cfm133 fmGeV
Note: Cold Nuclear Matter Density ~
Energy Density Inside Hadrons ~
150 MeV fm3
500 MeV fm3
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Not only is the energy density very high, the matter is strongly interacting at early times
Evidence:
Strong Flow Signal
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Analogy: Elliptic Flow of Ultracold Li6 Atoms
K.M.O’Hara et al, Science, 298 (2179) 2002
T~ 50 10-9 K
Elliptic Flow a very real phenomenon!Elliptic Flow a very real phenomenon!
x
y
x
y
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Elliptic Flow at RHIC
Geometry: asymmetric initial state
Fourier analysis 1+2v2cos2(lab-plane)
Asymmetry + interactions creates final state azimuthal correlations:
elliptic flowlab-plane
PHOBOS
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Bulk PQCD Hydro qqq Coalescence
Large v2 - strongly interacting matter at early time
pQCD Jets
From Gyulassy DNP 2004
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To answer these questions one needs localized penetrating probes
Such probes do exist main topic of this meeting
What is the novel medium?What is the origin of its strong interactions?
parton (quark or gluon)
parton (quark or gluon)
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HARD PROBES
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q+g q+g
For parton-parton scattering with high Pt
The basic interaction is understood pQCD
(Nobel Prize 2004)
pQCD
If parton beams of known momentum where available and scattered partons could be directly detected, life would be
beautiful!
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q+g jet+ X
jet
hadron
p
pz
ionFragmentat
:Rcone=0.7 rad
The best we can hope to do is to look at jets or jet fragments. This is reasonably well understood (combination of calculation and phenomenology, eg e+e- annihilation)
pQCD
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p+p π0+ X
“leading” π0
Xpp 0
More phenomenology needed but under control:
pQCD
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Au+Au π0+ X“leading” π0
More complications:
Multiple interactions and radiation before high Pt scattering (e.g.Cronin effect),
Shadowing
Saturation (e.g. Color Glass Condensate)
Appropriate normalization?
Effect of medium on fragmentation?
pA &dA helps to sort out initial state and final state effects
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Correct Normalization, i.e. What is the Number of Relevant Collisions for Colliding Nuclei?
Numbers obtained from Glauber model:Straight trajectoriesConstant cross-sectionNuclear density profile
Issues:Appropriate cross-sectionShadowingSaturationAll of above are Pt dependent
Npart = 4 + 2 = 6Ncoll = 4 2 = 8
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Nuclear Modification Factors
Some vocabulary:
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• Peripheral Au+Au = superposition of p+p reactions.
• Central Au+Au reveals a significant suppression !
EXAMPLES OF DATA
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CentralPeripheral
“Jet quenching” or Suppression of High PT Particles
Phenix Phenix
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STAR
PHENIX
PHOBOS
BRAHMS
AuAu and dAu comparison (Ncoll normalization):
BRAHMS
Phys Rev Lett 91, 072302/3/5 (2003)
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STAR: Phys.Rev.Lett.91:072304, 2003
Back-to-back jets:
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Out-plane
In-plane
K. Filimonov: DNP 10.31.03; nucl-ex/0410009
Correlation of suppression with reaction plane:
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• Different particles may behave differently. Looking at the behavior of all charged particles together may be misleading.
• Theorists may be pushing their luck using a high Pt approximation to a regime where it is clearly not applicable.
• Most data are for single particles and yet one speaks of them as if they are scattered partons or jets
• Inappropriate or unknown normalization can enhance or suppress an effect
• Important to ask if a “high Pt effect” is not there at low Pt
•Is there evidence that jet quenching goes approximately like density times the square of path length?
THERE ARE ISSUES ONE SHOULD BE AWARE OF WHILE LISTENING TO THE TALKS
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Suppression depends on produced particle type:
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• Different particles may behave differently. Looking at the behavior of all charged particles together may be misleading
• Theorists may be pushing their luck using a high Pt approximation to a regime where it is clearly not applicable
• Most data are for single particles and yet one speaks of them as if they are scattered partons or jets
• Inappropriate or unknown normalization can enhance or suppress an effect
• Important to ask if a “high Pt effect” is not there at low Pt
•Is there evidence that jet quenching goes approximately like density times the square of path length?
THERE ARE ISSUES ONE SHOULD BE AWARE OF WHILE LISTENING TO THE TALKS
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• Different particles may behave differently. Looking at the behavior of all charged particles together may be misleading
• Theorists may be pushing their luck using a high Pt approximation to a regime where it is clearly not applicable
• Most data are for single particles and yet one speaks of them as if they are scattered partons or jets
• Inappropriate or unknown normalization can enhance or suppress an effect
• Important to ask if a “high Pt effect” is not there at low Pt
•Is there evidence that jet quenching goes approximately like density times the square of path length?
THERE ARE ISSUES ONE SHOULD BE AWARE OF WHILE LISTENING TO THE TALKS
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• Different particles may behave differently. Looking at the behavior of all charged particles together may be misleading
• Theorists may be pushing their luck using a high Pt approximation to a regime where it is clearly not applicable
• Most data are for single particles and yet one speaks of them as if they are scattered partons or jets
• Inappropriate or unknown normalization can enhance or suppress an effect
• Important to ask if a “high Pt effect” is not there at low Pt
•Is there evidence that jet quenching goes approximately like density times the square of path length?
THERE ARE ISSUES ONE SHOULD BE AWARE OF WHILE LISTENING TO THE TALKS
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0-10% Central 200 GeV AuAu
PHENIX Preliminary
1 + ( pQCD x Ncoll) / phenix
backgrd Vogelsang NLO
AuAu→Direct photons consistent with Ncoll scaling
A inelastic cross-section consistent with Ncoll scaling
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Trends seen in “suppression” or “nuclear modification” depend on normalization
62.4 GeV200 GeV
PHOBOSAu+AuCharged particles
Most Central
Npart scaling
Ncoll scaling
Most peripheral
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Factorization of Energy/Centrality Dependence
62.4 GeV200 GeV
Mid rapidity density PHOBOS
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• Different particles may behave differently. Looking at the behavior of all charged particles together may be misleading
• Theorists may be pushing their luck using a high Pt approximation to a regime where it is clearly not applicable
• Most data are for single particles and yet one speaks of them as if they are scattered partons or jets
• Inappropriate or unknown normalization can enhance or suppress an effect
• Important to ask if a “high Pt effect” is not there at low Pt
•Is there evidence that jet quenching goes approximately like density times the square of path length?
THERE ARE ISSUES ONE SHOULD BE AWARE OF WHILE LISTENING TO THE TALKS
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A of pA hX
Barton et al Skupic et al -2 -1 0 y
From E451:Barton et al Phys Rev 27 (1983) 2580
Particle ratios in forward production of particles are independent of A
“Quenching” is seen in production of all particles in the very forward region of rapidity ( 2 units)
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• Different particles may behave differently. Looking at the behavior of all charged particles together may be misleading
• Theorists may be pushing their luck using a high Pt approximation to a regime where it is clearly not applicable
• Most data are for single particles and yet one speaks of them as if they are scattered partons or jets
• Inappropriate or unknown normalization can enhance or suppress an effect
• Important to ask if a “high Pt effect” is not there at low Pt
•Is there evidence that jet quenching goes approximately like density times the square of path length?
THERE ARE ISSUES ONE SHOULD BE AWARE OF WHILE LISTENING TO THE TALKS
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LISTEN WITH SOME SKEPTICISM
ENJOY THE MEETING
IT IS AN EXCITING ERA FOR THE FIELD
Last Words