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PHENIX OVERVIEW W.A. Zajc Columbia University for the PHENIX Collaboration Special thanks to J. Mitchell (BNL) for animations

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Page 1: PHENIX OVERVIEW W.A. Zajc Columbia University for the PHENIX Collaboration Special thanks to J. Mitchell (BNL) for animationsanimations

PHENIX OVERVIEW

W.A. Zajc

Columbia University

for the PHENIX Collaboration

Special thanks to J. Mitchell (BNL) for animations

Page 2: PHENIX OVERVIEW W.A. Zajc Columbia University for the PHENIX Collaboration Special thanks to J. Mitchell (BNL) for animationsanimations

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OutlineOutline

Why Nuclear Physics?

Why RHIC?

Why PHENIX?

Where do we go from here?

Page 3: PHENIX OVERVIEW W.A. Zajc Columbia University for the PHENIX Collaboration Special thanks to J. Mitchell (BNL) for animationsanimations

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Central Truths of Nuclear Physics

Central Truths of Nuclear Physics

We are nothing

We are dust

We don’t matter

Page 4: PHENIX OVERVIEW W.A. Zajc Columbia University for the PHENIX Collaboration Special thanks to J. Mitchell (BNL) for animationsanimations

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We are nothing (c. 1900)

We are nothing (c. 1900)

Most of “us” is (nearly) empty space 99.9% of the mass of atoms is

contained in the nucleus The nucleus is about one-trillionth

( 1/1,000,000,000,000 ) the size of the atom

ProtonProtonNeutronNeutronQuarksQuarksHeld togetherHeld togetherby gluonsby gluons(not shown)(not shown)

NucleusNucleus(“ion” when alone)(“ion” when alone)

AtomAtom

KeyKey

Page 5: PHENIX OVERVIEW W.A. Zajc Columbia University for the PHENIX Collaboration Special thanks to J. Mitchell (BNL) for animationsanimations

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We are dust (c. 1950)

We are dust (c. 1950)

Only the lightest elements (Hydrogen and Helium) were created in the Big Bang

The rest of “us” is stardust All heavy elements (like the Carbon and

Nitrogen we’re made of) were “cooked” together inside stars

Explosions of those (early) stars spread the heavier elements throughout the universe.

Page 6: PHENIX OVERVIEW W.A. Zajc Columbia University for the PHENIX Collaboration Special thanks to J. Mitchell (BNL) for animationsanimations

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We don’t matter (c. 2000)

We don’t matter (c. 2000)

More accurately: We’re not matter

Recall nearly all the mass of each atom is concentrated in the nucleus: Each nucleus consists of

neutrons and protons Each neutron and proton consists

of 3 quarks Each quark has the mass of about

1% of a proton or neutron(!) The rest of the mass of protons

and neutrons (and hence our mass) is “frozen energy” from the Big Bang

Page 7: PHENIX OVERVIEW W.A. Zajc Columbia University for the PHENIX Collaboration Special thanks to J. Mitchell (BNL) for animationsanimations

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Phase Transitions

Phase Transitions

The “great freeze” took place about 10 millionths of a second after the Big Bang

General name for such phenomena: Phase transitionExamples:

Steam to water to ice

(Free quarks and gluons) to (protons and neutrons) to (??)

Page 8: PHENIX OVERVIEW W.A. Zajc Columbia University for the PHENIX Collaboration Special thanks to J. Mitchell (BNL) for animationsanimations

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Phase DiagramsPhase Diagrams

Water

Nuclear Matter

Page 9: PHENIX OVERVIEW W.A. Zajc Columbia University for the PHENIX Collaboration Special thanks to J. Mitchell (BNL) for animationsanimations

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A Silly AnalogyA Silly Analogy Suppose…

You lived in a frozen world where water existed only as ice and ice comes in only quantized sizes ~ ice cubes and theoretical friends tell you there should be a liquid phase and your only way to heat the ice is by colliding two ice cubes So you form a “bunch” containing a billion ice cubes which you collide with another such bunch 10 million times per second which produces about 1000 IceCube-IceCube collisions per

second which you observe from the vicinity of Mars

Change the length scale by about 10 trillion You’re doing physics at RHIC!

Page 10: PHENIX OVERVIEW W.A. Zajc Columbia University for the PHENIX Collaboration Special thanks to J. Mitchell (BNL) for animationsanimations

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Boiling Neutrons and Protons

Boiling Neutrons and Protons

Fundamental Method:Collide heavy nuclei at the highest

possible energies:

Fundamental Goals: Create (new) dense forms of matter Re-create the quark-gluon phase transition

Page 11: PHENIX OVERVIEW W.A. Zajc Columbia University for the PHENIX Collaboration Special thanks to J. Mitchell (BNL) for animationsanimations

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In PicturesIn Pictures

Page 12: PHENIX OVERVIEW W.A. Zajc Columbia University for the PHENIX Collaboration Special thanks to J. Mitchell (BNL) for animationsanimations

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RHIC = Relativistic Heavy Ion Collider Located at Brookhaven National Laboratory

RHICRHIC

Page 13: PHENIX OVERVIEW W.A. Zajc Columbia University for the PHENIX Collaboration Special thanks to J. Mitchell (BNL) for animationsanimations

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RHIC’s Experiments

RHIC’s Experiments

STAR

Page 14: PHENIX OVERVIEW W.A. Zajc Columbia University for the PHENIX Collaboration Special thanks to J. Mitchell (BNL) for animationsanimations

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How is RHIC Different?

How is RHIC Different?

It’s a collider Detector systematics independent of ECM (No thick targets!)

It’s dedicated Heavy ions will run 20-30 weeks/year

It’s high energy Access to non-perturbative phenomena

Jets Non-linear dE/dx

Its detectors are comprehensive ~All final state species measured with a

suite of detectors that nonetheless have significant overlap for comparisons

Page 15: PHENIX OVERVIEW W.A. Zajc Columbia University for the PHENIX Collaboration Special thanks to J. Mitchell (BNL) for animationsanimations

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What is PHENIX?What is PHENIX? Pioneering High Energy Nuclear Interaction

eXperiment Goals:

Broadest possible study of A-A, p-A, p-p collisions to Study nuclear matter under extreme conditions Using a wide variety of probes sensitive to all

timescales Study systematic variations with species and

energy Measure spin structure of the nucleon

These two programs have produced a detector with unparalleled capabilities

Page 16: PHENIX OVERVIEW W.A. Zajc Columbia University for the PHENIX Collaboration Special thanks to J. Mitchell (BNL) for animationsanimations

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The CollaborationThe CollaborationA strongly international venture:

11 nationsBrazil, China, France, Germany, India,

Israel, Japan, South Korea, Russia, Sweden, United States

51 institutions

Page 17: PHENIX OVERVIEW W.A. Zajc Columbia University for the PHENIX Collaboration Special thanks to J. Mitchell (BNL) for animationsanimations

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PHENIX at RHICPHENIX at RHIC

2 central spectrometers

2 forward spectrometers

3 global detectors

West

EastSouth

North

Page 18: PHENIX OVERVIEW W.A. Zajc Columbia University for the PHENIX Collaboration Special thanks to J. Mitchell (BNL) for animationsanimations

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ScheduleSchedule

2 central spectrometers

2 forward spectrometers

3 global detectors

1999

20002001

2002

Page 19: PHENIX OVERVIEW W.A. Zajc Columbia University for the PHENIX Collaboration Special thanks to J. Mitchell (BNL) for animationsanimations

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24-Jul-9724-Jul-97

Page 20: PHENIX OVERVIEW W.A. Zajc Columbia University for the PHENIX Collaboration Special thanks to J. Mitchell (BNL) for animationsanimations

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10-Jan-9810-Jan-98

Page 21: PHENIX OVERVIEW W.A. Zajc Columbia University for the PHENIX Collaboration Special thanks to J. Mitchell (BNL) for animationsanimations

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12-Jan-9912-Jan-99

Page 22: PHENIX OVERVIEW W.A. Zajc Columbia University for the PHENIX Collaboration Special thanks to J. Mitchell (BNL) for animationsanimations

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23-Dec-9923-Dec-99

Page 23: PHENIX OVERVIEW W.A. Zajc Columbia University for the PHENIX Collaboration Special thanks to J. Mitchell (BNL) for animationsanimations

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Run-1 Configuration

Run-1 Configuration

Two central arms Mechanically

~complete Roughly half of

aperture instrumented Global detectors

Zero-degree Calorimeters (ZDCs)

Beam-Beam Counters (BBCs)

Multiplicity and Vertex Detector (MVD, engineering run)

Page 24: PHENIX OVERVIEW W.A. Zajc Columbia University for the PHENIX Collaboration Special thanks to J. Mitchell (BNL) for animationsanimations

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TourTour

Page 25: PHENIX OVERVIEW W.A. Zajc Columbia University for the PHENIX Collaboration Special thanks to J. Mitchell (BNL) for animationsanimations

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Tour (Particle View)

Tour (Particle View)

Page 26: PHENIX OVERVIEW W.A. Zajc Columbia University for the PHENIX Collaboration Special thanks to J. Mitchell (BNL) for animationsanimations

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Run-1 Accomplishments

Run-1 Accomplishments

First collisions:15-Jun-00 Last collisions: 04-Sep-00 During this period:

Commissioned Zero-Degree Calorimeters Beam-Beam Counters Multiplicity and Vertex Counter Drift Chambers Pad Chambers Ring Imaging Cerenkov Counter Time Expansion Chamber Time-of-Flight Counters Electromagnetic Calorimeter Muon Identifier Minimum Bias Triggers Data Acquisition System

Recorded ~5M minimum bias events

Page 27: PHENIX OVERVIEW W.A. Zajc Columbia University for the PHENIX Collaboration Special thanks to J. Mitchell (BNL) for animationsanimations

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Run-1 ResultsRun-1 Results

This is a partial compilation

Page 28: PHENIX OVERVIEW W.A. Zajc Columbia University for the PHENIX Collaboration Special thanks to J. Mitchell (BNL) for animationsanimations

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Measuring InitialCollision GeometryMeasuring Initial

Collision Geometry

Zero Degree Calorimeters (ZDC) Sensitive to spectator

neutrons common to all four RHIC

experiments Using a combination of

the ZDC’s and BBC’s we can define Centrality Classes

Zero Degree Calorimeter

5-10%10-15%

15-20%

0-5 %

“Spectators”

“Spectators”

“Participants”. n

nnp

pp

Beam-Beam Counter (BBC)Impact Parameter

ZD

CBBC

Page 29: PHENIX OVERVIEW W.A. Zajc Columbia University for the PHENIX Collaboration Special thanks to J. Mitchell (BNL) for animationsanimations

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R2

Determining Energy DensityDetermining

Energy Density

Bjorken~ 5.0 GeV/fm3

Roughly 1.5 to 2 times higher than any previous experiments

Bjorken formula for thermalized energy density

time to thermalize the system (0 ~ 1 fm/c)~6.5 fm

For the most central events:

PHENIX preliminary

EMCAL

What is the energy density achieved? How does it compare to the expect

phase transition value ? Is this energy density thermalized?

dy

dE

RT

Bj0

2

11

dydz 0

Page 30: PHENIX OVERVIEW W.A. Zajc Columbia University for the PHENIX Collaboration Special thanks to J. Mitchell (BNL) for animationsanimations

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Have studied growth of Number of particles Energy

versus “centrality” Excellent consistency between two analyses First evidence for new term in growth ~ number

of collisions

PHENIX preliminaryPHENIX preliminary

collpart NBNAddX 0

28.088.0 A

12.034.0 B

First PublicationsFirst Publications

)(24.080.0 GeVA )(09.023.0 GeVB

19.038.0/ AB 18.029.0/ AB

Page 31: PHENIX OVERVIEW W.A. Zajc Columbia University for the PHENIX Collaboration Special thanks to J. Mitchell (BNL) for animationsanimations

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Fingerprinting Particles

Fingerprinting Particles

Combined Tracking Beam-Beam Counter Time-of-Flight array

provides excellent hadron identification over broad momentum band:

Page 32: PHENIX OVERVIEW W.A. Zajc Columbia University for the PHENIX Collaboration Special thanks to J. Mitchell (BNL) for animationsanimations

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Anti-proton/proton ratio

Anti-proton/proton ratio

Page 33: PHENIX OVERVIEW W.A. Zajc Columbia University for the PHENIX Collaboration Special thanks to J. Mitchell (BNL) for animationsanimations

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Approaching the Early Universe

Approaching the Early Universe

Early Universe: Anti-proton/proton = 0.999999999

√s [GeV]

PHENIX preliminary

E866Au+Au

NA44Pb+Pb

pba

r/p

We’ve created “pure” matterapproaching this value

Page 34: PHENIX OVERVIEW W.A. Zajc Columbia University for the PHENIX Collaboration Special thanks to J. Mitchell (BNL) for animationsanimations

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0 0 spectraspectra0 0 spectraspectra

0

pT >2 GeV,asym<0.8

Systematic errors includedMain sources:

peak extraction PID loss efficiency calculations non-vertex pions pT scale

Centrality ~Nbin ~Npart

10% 800 300 M.B. 125 75 75-92% 10 10 ~1M Min Bias AuAU events

s = 130 GeV

Peripheral

Min bias

Central

Page 35: PHENIX OVERVIEW W.A. Zajc Columbia University for the PHENIX Collaboration Special thanks to J. Mitchell (BNL) for animationsanimations

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Charged pT SpectraCharged pT Spectra Systematic

trends in high momentum production also studied with charged particles Much greater

statistics Different

systematics

Page 36: PHENIX OVERVIEW W.A. Zajc Columbia University for the PHENIX Collaboration Special thanks to J. Mitchell (BNL) for animationsanimations

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Comparison to charged spectraComparison to

charged spectra

0 spectra matches identified charged pion spectra –

A very good internal test of our results

(+ +-)/2

0

All charged

Page 37: PHENIX OVERVIEW W.A. Zajc Columbia University for the PHENIX Collaboration Special thanks to J. Mitchell (BNL) for animationsanimations

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Comparison to Theory

Comparison to Theory

Good agreement with “grazing” collisions

For head-on collisions, clear deficit with respect to “no new physics” calculations

Page 38: PHENIX OVERVIEW W.A. Zajc Columbia University for the PHENIX Collaboration Special thanks to J. Mitchell (BNL) for animationsanimations

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Central Events – What’s Going On?Central Events – What’s Going On?

“Standard” predictions overestimate the cross-sectionfor 0 by at least 5

dE/dx=0.25 GeV/fm

dE/dx = 0 (pQCD)

Predictions including (plasma-like!)energy loss consistent with 0

Page 39: PHENIX OVERVIEW W.A. Zajc Columbia University for the PHENIX Collaboration Special thanks to J. Mitchell (BNL) for animationsanimations

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Physics Implications (??)

Physics Implications (??)

Slide fromseminar given lastmonth by M. Gyulassy

Page 40: PHENIX OVERVIEW W.A. Zajc Columbia University for the PHENIX Collaboration Special thanks to J. Mitchell (BNL) for animationsanimations

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Physics ImpactPhysics Impact

Page 41: PHENIX OVERVIEW W.A. Zajc Columbia University for the PHENIX Collaboration Special thanks to J. Mitchell (BNL) for animationsanimations

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Composition at high pT

Composition at high pT

Possible complication in comparisons of charged yields to theory:

Particle composition is observed to be a strong function of pT

Page 42: PHENIX OVERVIEW W.A. Zajc Columbia University for the PHENIX Collaboration Special thanks to J. Mitchell (BNL) for animationsanimations

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Time to PhysicsTime to PhysicsAgain, learn from the past:

First CDF publication:Transverse-Momentum

Distributions of Charged Particles Produced in p-pbar Interactions at 630 and 1800 GeV, F. Abe et al., Phys. Rev. Lett. 61, 1819 (1988).

~One year from data-taking.

Much simpler final state!

We will be hard-pressed to reach this goal

And much harder-pressed to maintain “CDF-like” rate WRONG!(?)

Page 43: PHENIX OVERVIEW W.A. Zajc Columbia University for the PHENIX Collaboration Special thanks to J. Mitchell (BNL) for animationsanimations

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One Year AgoOne Year AgoFor years we’d been showing pictures of one “central” arm:

21-Jan-00: The real thing moves into place

Page 44: PHENIX OVERVIEW W.A. Zajc Columbia University for the PHENIX Collaboration Special thanks to J. Mitchell (BNL) for animationsanimations

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Shape of Things to Come

Shape of Things to Come

Completion of Central Arms Significantly

increased aperture Addition of new capabilities

South Muon Arm Di-muon physics

Upgraded Triggers Data Acquisition

The ~5M events recorded in Run-1 represent ~1 day of data-taking for RHIC+PHENIX in Run-2

Insert here

Page 45: PHENIX OVERVIEW W.A. Zajc Columbia University for the PHENIX Collaboration Special thanks to J. Mitchell (BNL) for animationsanimations

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Shape of Things NowShape of Things Now

Page 46: PHENIX OVERVIEW W.A. Zajc Columbia University for the PHENIX Collaboration Special thanks to J. Mitchell (BNL) for animationsanimations

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SummarySummary PHENIX detector has provided outstanding data in

first year of RHIC operations Measured

Charged multiplicity Transverse energy Elliptic flow Identified particle spectra HBT parameters High pT spectra Inclusive electron spectrum (much more)

Observed New trends in particle production New behavior in particle yields at high momentum

Ideally positioned to dramatically extend these results in second year of RHIC running