introduction to relativistic heavy ion physicsintroduction to relativistic heavy ion physics lecture...
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Introduction to Relativistic Heavy Ion Physics
Lecture 2: Experimental Discoveries
W.A. ZajcColumbia University
01-Jul-09
1
W.A. Zajc
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Reminder- From Lecture 1
• General arguments suggest that for
temperatures T ~ 200 MeV, nuclear matter will
undergo a deconfining phase transition.
• Similar arguments suggest
the required energy density is of order
Note 1: normal nuclear density e0 ~ 0.16 GeV/fm3
Note 2: Also true near T = 0, i.e., cold nuclear
matter
• How to create study experimentally ?01-Jul-09 W.A. Zajc
2
3
3
42
/4.2~)2.0(
3
137~)200(
30~ fmGeV
fm
GeVMeVndf
e
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Exploring the QCD Phase Diagram
• Hot nuclear matter:
Study
experimentally
by colliding
heaviest nuclei
at highest
energies:
• Cold nuclear matter:
Study by
observation of neutron stars and other exotic objects
(Not covered in these lectures)01-Jul-09 W.A. Zajc
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01-Jul-09 W.A. Zajc
Expectations circa 2000
As encoded in the Nuclear Physics Wall Chart,http://www.lbl.gov/abc/wallchart/
RHIC would create a quark-gluon plasma;a “gas” of weakly interacting quarks and gluons
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RHIC and Its Experiments
STAR
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RHIC Specifications 3.83 km circumference
Two independent rings 120 bunches/ring
106 ns crossing time
Capable of colliding ~any nuclear species on ~any other species
Energy:
500 GeV for p-p
200 GeV for Au-Au(per N-N collision)
Luminosity
Au-Au: 2 x 1026 cm-2 s-1
p-p : 2 x 1032 cm-2 s-1
(polarized)
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How is RHIC Different?• Different from p-p, e-p colliders
Atomic weight A introduces new scale Q2 ~ A1/3 Q02
• Different from previous (fixed target) heavy ion facilities
ECM increased by order-of-magnitude
Accessible x (parton momentum fraction)
decreases by ~ same factor
Access to 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
s
p 2~x T
Jargon Alert:s = Center-of-mass energy (per nucleon collision)pT = transverse momentum = |p| sin qQ2 = (momentum transfer)2
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The Plan circa 2000
• Use RHIC‟s unprecedented capabilities
Large √s
♦ Access to reliable pQCD probes
♦ Clear separation of valence baryon number and glue
♦ To provide definitive experimental evidence for/against
Quark Gluon Plasma (QGP)
Polarized p+p collisions
• Two small detectors, two large detectors
Complementary capabilities
Small detectors envisioned to have 3-5 year lifetime
Large detectors ~ facilities
♦ Major capital investments
♦ Longer lifetimes
♦ Potential for upgrades in response to discoveries
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Since 2000…
• Accelerator complex Routine operation at 2-4 x design luminosity (Au+Au)
Extraordinary variety of operational modes
♦ Species: Au+Au, d+Au, Cu+Cu, p+p
♦ Energies: 22 GeV (Au+Au, Cu+Cu, p), 56 GeV (Au+Au), 62 GeV (Au+Au,Cu+Cu, p+p) , 130 GeV (Au+Au),
200 GeV (Au+Au, Cu+Cu, d+Au, p+p), 410 GeV (p), 500 GeV (p)
• Experiments:
Worked !
• Science More than 200 refereed publications, among them 100+ PRL‟s
Major discoveries
• Future Demonstrated ability to upgrade
Key science questions identified
Accelerator and experimental upgrades underway for that science
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Assertion
• In these complicated events, we have
(a posteriori) control over the event geometry:
Degree of overlap
Classify by “centrality”, e.g., 0-10% most central events
Orientation with respect to overlap
“Central” “Peripheral”
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“Central”
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Outline
Will present sample of results from
various points of the collision process:
1. Final State
Yields of produced particles
Thermalization, Hadrochemistry
3. Initial State
Hydrodynamic flow from initial spatial asymmetries
2. Plasma(?)
Probes of dense matter
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Final StateDoes the huge abundance of final
state particles reflect a thermal
distribution?:
1. Final State
Yields of produced particles
Thermalization, Hadrochemistry
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Origin of the (Hadronic) Species, 0, K, K*0(892), Ks
0, h, p, d, r0, f, D,
L, S*(1385), L*(1520), X± , W, D0, D±, J/Y’s,
(+ anti-particles) … T ~ 170 MeV ~ 2 x 1012 K
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• Thermal? Apparently:
Assume all distributions described
by one temperature T and
one ( baryon) chemical potential m :
One ratio (e.g., p / p ) determines
m / T :
A second ratio (e.g., K / )
provides T m
• Then predict all other hadronic
yields and ratios:
• NOTE: Truly thermal implies
No memory (!)
Exercise 1: Find T and m from data at right
pdednTE 3/)(~ m
T
TE
TE
ee
e
p
p /2
/)(
/)(m
m
m
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130 GeV RHIC : STAR / PHENIX /
PHOBOS / BRAHMS
17.4 GeV SPS : NA44, WA97
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Locating RHIC on Phase Diagram
• Previous figure RHIC has net baryon density ~ 0:
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Locating RHIC on Phase Diagram
RHIC is as close as we’ll get to the early universe for some time (until nextyear )
• Previous figure RHIC has net baryon density ~ 0:
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Probes of the Plasma(?) State
Q. How dense is the matter?
A. Do Rutherford scattering on deep interior
using “auto-generated” probes:
2. Plasma(?)
Probes of dense matter
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Transverse Dynamics
q
p
pT
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3
3
dp
dE
s
Exercise 2: Remind yourself why this is invariant
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Kinematics 101
Fundamental single-particle observable:
Momentum Spectrum
dypd
d
pE
pEy
Tz
z
2
3
ln2
1 s
dy
dn
pd
d
T
2
2
~s
-1 -0.5 0 0.5
cosq
)(cosqd
dn
-6 -4 -2 0 2 4 6
y
dy
dn
-6 -4 -2 0 2 4 6
y
dy
dn
Kinematics
DynamicsExercise 3: Show that y is additive under Lorentz transformations. Use this to show dy = d .
Observation: Roughly the same pT spectra here and here
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Aside- Estimating Energy Density
• This will be an incredibly crude
(wrong) estimate:
Take all ~10,000 particles produced in Au+Au
collision at RHIC
Assume the ~constant <pT> ~ 0.4 GeV
represents “thermalized” energy
Initial volume
♦ RAu ~ 6.5 fm
♦ Dz ~ 1/T ~ 1 fm
Energy density
e ~ (104 x 0.4 GeV) / (RAu2 x 1 fm) ~ 30 GeV/fm3
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dydz t
-6 -4 -2 0 2 4 6
y
dy
dn
Dynamics 101
t
dy
dE
RdzR
dE
V
E T
TT
T
te
22
1~
Q. How to really (?) estimate initial energy density?
A. From rapidity density of transverse energy ET Si Ei sin qi
“Highly relativistic nucleus-nucleus collisions: The central rapidity region”, J.D. Bjorken,Phys. Rev. D27, 140 (1983).
Assumes
♦ ~ 1-d hydrodynamic expansion
♦ Invariance in y along “central rapidity plateau”(I.e., flat rapidity distribution)
♦ Then
since boost-invariance of matter
where t ~ 1 fm/c
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For the most central events:
PHENIX
R2
Determining Energy Density
eBjorken ~ 4.6 GeV/fm3
~30 times normal nuclear density~1.5 to 2 times higher than any previous experiments
Bjorken formula for thermalized energy density
time to thermalize the system (t0 ~ 1 fm/c)~6.5 fm
What is the energy density achieved?
How does it compare to the expected phase transition value ?
dy
dE
R
TBj
0
2
11
te
dydz 0t
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-6 -4 -2 0 2 4 6
y
The Danger in Cartoons
• What is this thing ??
• Surely not the space-time development:
W.A. Zajc
-6 -4 -2 0 2 4 6
y
?
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Using “Hard Probes”
time
p+p
d+Au
Au+Au
Systematic approach essential:
p+p: BASELINE
d+Au: CONTROL
Au+Au: NEW EFFECT
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Baseline p+p Measurements with pQCD• Consider measurement of 0‟s
in p+p collisions at RHIC.
• Compare to pQCD calculation
• Phys. Rev. Lett. 91, 241803 (2003)
•parton distribution functions, for partons a and b•measured in DIS, universality
•perturbative cross-section (NLO)•requires hard scale•factorization between pdf and cross section
•fragmentation function•measured in e+e-
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),(
)(ˆ
),(),(
2
/
2
/
2
/
m
s
mms
hch
bBbaAa
zD
dcbad
xfxfd
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Systematic Measurement in Au+Au
constancy for pT > 4 GeV/c for all centralities?
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Luminosity
• Consider collision of „A‟ ions per bunch
with „B‟ ions per bunch:
• LuminosityA
B
Cross-sectional
area ‘S’
S
BAL
~
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Change scale by ~ 109
• Consider collision of „A‟ nucleons per nucleus
with „B‟ nucleons per nucleus:
• „Luminosity‟
A
B
Cross-sectional
area ‘S’
BANS
BAL Coll
~~
Provided:No shadowingSmall
cross-sectionsBANnot Part
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Binary Collisions
Participants
b (fm)
Systematizing our Knowledge• All four RHIC experiments have
carefully developed techniques for
determining
the number of participating nucleons
NPART in each collision
(and thus the impact parameter)
The number of binary nucleon-
nucleon collisions NCOLL as a function
of impact parameter
• This effort has been essential in
making the QCD connection
Soft physics ~ NPART
Hard physics ~ NCOLL
• Often express impact parameter b
in terms of “centrality”, e.g.,
10-20% most central collisions
Participants
Spectators
Spectators
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Rare Processes• Particle production via rare processes should scale with Ncoll , the number of
underlying binary nucleon-nucleon collisions
• Roughly: Small s no shadowing
per nucleon luminosity is relevant quantity
• Take scaling with Ncoll as our null hypothesis
for hard processes
FunctionThickness
),()( dzzddTA r
dz
d
FunctionOverlap
)2
()2
()( sdb
sTb
sTbT BAAB
b
INTINT
)(2
AB
AB
INT
small""for
1
then is section cross TOTAL the
section cross withinteract which
tsconstituen B has B"" Nucleus and
tsconstituen Ahas A"" Nucleus If
ss
s
s
s
s
BA
ebdbTABINT
Exercise 4: Make a plausibility argument for sAB formula, and verify approximation.
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no effect
Systematizing Our Expectations
Describe in terms of scaled ratio RAA
= 1 for “baseline expectations”
> 1 “Cronin” enhancements (as in proton-nucleus)
< 1 (at high pT) “anomalous” suppression
Events) ppin B)(Yield(A
EventsAu Auin Yield
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no effect
Systematizing Our Expectations
Describe in terms of scaled ratio RAA
= 1 for “baseline expectations”
> 1 “Cronin” enhancements (as in proton-nucleus)
< 1 (at high pT) “anomalous” suppression
Events) ppin B)(Yield(A
EventsAu Auin Yield
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Systematic Suppression PatternSu
pp
ressed
Enh
ance
d
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Unique to Heavy Ion Collisions?• YES! : Run-3: a crucial control measurement via d+Au collisions
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Unique to Heavy Ion Collisions?• YES! : Run-3: a crucial control measurement via d+Au collisions
d+Au results from
presented at a press conference at BNL on June, 18th, 2003
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Energy Loss of Fast Partons• Many approaches
1983: Bjorken
1991: Thoma and Gyulassy (1991)
1993: Brodsky and Hoyer (1993)
1997: BDMPS- depends on path length(!)
1998: BDMS
• Numerical values range from ~ 0.1 GeV / fm (Bj, elastic scattering of partons)
~several GeV / fm (BDMPS, non-linear interactions of gluons)
2
22
2
2 4ln~
4ln
4
303
M
ETT
M
ET
dx
dESS e
D
SF
ETC
dx
dE
m
ln
3
4 22
2
2
Tk
dx
dE D
gg
DRS
LL
C
dx
dE
m ln
8
2
24
2
TC
s
kN
dx
dE D
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The One That Started It All…
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Pedestal&flow subtracted
01-Jul-09 W.A. Zajc
The Matter is Opaque
C2(Au Au) C2(p p) A*(1 2v22 cos(2Df))
STAR azimuthal correlation function shows ~ complete absence of “away-side” jet
Surface emission only (?)
That is, “partner” in hard scatter is absorbed in the dense medium
Density ~ 50 x normal nuclear e0
Df
GONE
GONE
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Schematically (Partons)
Scattered partons on the “near side” lose energy, but emerge;
those on the “far side” are totally absorbed
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Photons shine, Pions don’t
• Direct photons are not inhibited by hot/dense medium
• Rather: shine through consistent with pQCD
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Precision Probes
• This one figure encodes
rigorous control of systematics
• in four different measurements
over many orders of
magnitude
centralN
coll= 975 94
= =
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Schematically (Photons)Scattered partons on the “near side”
lose energy, but emerge;
the direct photon always emerges
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RHIC and the Phase “Transition”42
• Suppression of high momentum probes
requires densities > 50 x e0
• High Tinit
~ 300 MeV
to
• Low Tfinal
~ 100 MeV
Exercise 5: Use the statement about energy density to verify upper edge of band for RHIC
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Summary- Lecture 2
• Au+Au collisions at top RHIC energy produces thermal matter with energy density
e >> e0 and e >> eQGP
From simple estimates
From detailed pQCD probes
• Suppression not seen in
d+Au control
Photons
• Results consistent with the formation of QGP with a temperature T ~ 2TC
• Next time: How fluid is the densest matter ever studied ?
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