Heavy Ions at the SP[b]S What Is There Left to Do? SPSC Special Workshop Villars s/Ollon • • • • September 22 – 28, 2004 Superdense (and -hot) QCD.

Download Report

Transcript Heavy Ions at the SP[b]S What Is There Left to Do? SPSC Special Workshop Villars s/Ollon • • • • September 22 – 28, 2004 Superdense (and -hot) QCD.

Heavy Ions at the SP[b]S
What Is There Left to Do?
SPSC Special Workshop
Villars s/Ollon
•
•
•
•
September 22 – 28, 2004
Superdense (and -hot) QCD Matter
What We Already Know (SPS & RHIC)
What We Would Like to Know
Possible goals of Future HI Expts at the SPS
QCD Phase Diagram
Early universe
RHIC, LHC
T
QGP
Critical endpoint
Quark-Gluon Plasma (QGP)
Meson
Dominated HG
Hadronic
matter
Chiral symmetry
restored
Baryon
Dominated HG
Chiral symmetry
broken
Nuclei
Color
superconductor
Neutron stars
B
From hadrons to QGP
  30 gDOFT
2
4
QGP = quark-gluon plasma
  0
QCD equation
of state from
lattice QCD
Hadron gas

0
QCD EOS for B  0
S. Ejiri et al. (Bielefeld-Swansea)
Nf=2
Baryon number is
“unthawed” for
T/Tc = 0.9 – 1.1
Evidence that the
carriers of baryon
number (quarks)
become light and
color d.o.f. is freed.
The perturbative QGP
At T > 2Tc the QGP looks perturbative (neglect mq):
 15 s
  1 
4

2
2
 16
 50 s  21
4
4
T

1

N
T
F



30
21

30



 2 s  3 2 2 2 1 2
 1 
 2 q ( T  2 q ) 
 
q 
Expansion in s does not converge, rather one must include
interactions into the particle modes (“quasiparticles”) as
basis for the expansion. All perturbatively calculable terms
(up to s3 ln s) have been calculated, agreeing well with
LGT equation of state down to near Tc.
Quasiparticles in the QGP
Physical excitation modes at high T are not elementary
quarks and gluons, but “dressed” quarks and gluons:
T
Compton scattering
on a thermal gluon!
(k ,  )
Propagator of transversely polarized gluons
1
 1 k   k 
D(k ,  )1   2  k 2  ( gT )2 1     ln

2
2
k



k




 Effective mass of gluon:
1
gT
3
1
k 
mG* 

gT
2
k 0
mG* 

(screening)
(massive mode)
Color Screening in Quenched LGT
O. Kaczmarek et al.
Rapid disappearance of color
screening near Tc suggests
binding of dynamical gluons
into “glueballs”.
Drop in (T) too fast
to be described by
dynamical glue mass
Singlet
potential
T=0 coupling of
static quarks
sQGP = a Plasma of Bound States ?
Lattice simulations (quenched!) of
spectral functions (Asakawa et al.,
Datta et al.) indicate persistence of
(quasi-)bound states above Tc
Very speculative scenario!
(cc )
Shuryak & Zahed
Signatures of the QCD Phase Change
•
•
•
•
•
•
•
•
•
Enhancement of s-quark production
Dissolution of Ψ,  bound states
Disappearance of light hadrons (ρ0)
Effects of “latent heat” in (E,T) relation
Thermal g radiation
Event-by-event fluctuations
Large energy loss of fast partons
Bulk hadronization
Collective vacuum excitations
What We Know Already
Classical QGP Signatures seen at SP[b]S
The SP[b]S “Panorama”
The Novel Discoveries of RHIC
The Three “Classic” Signals
Strangeness Enhancement…
…probes chiral symmetry restoration and deconfinement
Mass (MeV)
NA57 data
1000000
Q CD mass
100000
Higgs mass
(sss)
10000
QCD mass
disappears
(qss)
1000
100
(qqs)
10
1
u
d
s
Flavor
c
b
t
Charmonium Suppression
…probes color deconfinement ?
Y’
NA50
Low-Mass Lepton-Pair Excess
CERES
Collision broadening
of the r resonance in
the baryon-rich
hadronic medium
Three Legs Are a Bit Shaky…
…a 4th Leg Adds Stability !
Thermodynamics near Tc
  30 gDOFT
2
4
T
van Hove
E
Additional energy is
used up to liberate
new degrees of
freedom (color!) in
transition region
Hadrons at the Boiling Point
RHIC
SPS
AGS
Plateau is an indicator of latent heat of phase transformation.
K/ excitation function
Sensitive to B
The “Horn”...
K+
K-
K/ Excitation Function II
K
e( u  s mK ) / T
K
e( s  u mK ) / T
Measures effective K mass
K K

K

K

 
e
2 mK / T
RHIC
…a Plateau!
SPS
…becomes Part of…
The “Horn”...
AGS
The Villars Panorama
e+e-
Photons
Chemistry
J/Y
HBT
Thorsten Renk
hep-ph/0403239
Spectra
The SP[b]S Panorama
The Model Framework

( x, y, z, t )  r,  ,s  12 ln tt  zz ,  t 2  z 2
R
s
  12 ln
E  pz
E  pz

s  12 ln
tz
tz
s(r,s , )  FR (r, ) FL (s , )
Partial stopping:
 front ( 0 )  0.60 with  0  1fm/c
 front ( f )  1.45 with  f  15fm/c
Compare with Pb = 2.9
at freeze-out
The Cooling Curve
High initial temperature due to
large degree of stopping!
 0  1fm/c
T0  300 MeV
 QGP  6.5fm/c
LGT and
RG EOS
 Had  8.5fm/c
T f  100 MeV
QGP
R rms
 8.55fm
f
Had
 f  0.57
Hadron Spectra
Transverse spectra fix vf┴
Resonance decays
Rapidity distribution
determines ffront
Hadro-Chemistry
Statistical
hadronization
No “free” parameters: Tc from LGT,
B and S from conservation laws.
Lepton pairs
…are sensitive to in-medium modifications of r-meson
and the duration of the hadronic phase, contribution from
QGP visible above 1 GeV invariant mass.
QGP Outshines Hadron Gas!
… because it is so much hotter.
Photon spectrum is sensitive to
the initial temperature T0
Almost all observed direct photons
are emitted by the QGP
Charmonium Suppression
Ionization by thermal gluons
The RHIC Discoveries
Jet Quenching
Baryon Excess  Recombination ?
Large Elliptic Flow
Jet Quenching
High-energy parton loses energy by
rescattering in dense, hot medium.
q
q
Radiative energy loss:
dE / dx
r L kT 2
L
q
q
Scattering centers = color charges
g
Can be described as medium effect on
parton fragmentation:
z


D p h ( z , Q 2 )  D p h ( z , Q 2 )  D p  h 
, Q2 
 1  E / E

Suppression of high-pT hadrons
PHENIX Data: Identified 0
?
Away side jet
Same side jet
STAR
The Baryon “Puzzle”

What makes baryons
different from mesons ?
Hadronization mechanisms
q
q q
q
q
q q q
Recombination
Fragmentation
Baryon
Meson
1
Baryon
1
Meson
pM  2 pQ
pB  3 pQ
Recombination vs. Fragmentation
2
dN M
P u



d

dxw
(
R
,
xP
)
w
(
R
,(1

x
)
P
)

(
x
)



M
d 3P 
(2 )3  ,  
Recombination:
E
Fragmentation:
dN h
P  u dz
1
E 3   d
w
(
r
,


z P )D  h ( z )
3  3
d P
(2 ) 0 z 
Recombination…
w (r , xP  ) w (r , (1  x) P  )  exp   P  u / T 
Meson
w (r , xP  ) w (r , x ' P  ) wg (r , (1  x  x ') P  )  exp   P  u / T 
Baryon
1
…always wins over fragmentation for an exponential spectrum (z<1):
exp( P  u / T )
 exp( P  u / zT )
… but loses at large pT, where the spectrum is a power law ~ (pT) -b
Recombination vs. Fragmentation II
Fries, Bass,
Nonaka, BM
RAA
T = 170 MeV
v┴ = 0.55c
Greco, Ko,
Levai
The Partons Flow!
Recombination model
suggests that hadronic
flow reflects partonic
flow (n = number of
valence quarks):
part
v had

n
v
2
2
pThad  npTpart
Provides measurement
of partonic v2 !?
Was Landau right ?
STAR + PHENIX
Central plateau or peak
of a Gaussian?
BRAHMS
(P. Steinberg- PHOBOS)
 y2 
dN K s1/ 4

exp   
dy
2 L
 2L 
with L = ln(g)
PHOBOS
Implications of RHIC Results
• Early equilibration & development of pressure
• Highly dissipative medium
• Very high density of (colored) scattering centers at
early times (dNG/dy  dNh/dy).
• Collectivity at the parton level
• Hadrons at RHIC are not “hotter” than at SPS
• Physics at RHIC is not boost invariant
What We Would Like to Know
Focus on 3 issues:
What are the initial conditions ?
What kind of material is the “QGP” ?
Where is the QCD critical point ?
GSI/FAIR ???
e+e-
Photons
Chemistry
DONE
J/Y
HBT
Mostly
Done
Spectra
The SP[b]S Panorama
High pT
Photons - From the “depth of time”
Initial stopping
Coherent
bremsstrahlung
2-photon HBT interferometry
Discriminates against 0
decays and makes it possible
to identify “direct” photons at
lower pT. Goal for RHIC II,
but physics case at SPS may
be stronger!
Proposed, but dropped, at RHIC
What kind of Stuff are the Comovers ?
… and how do they disrupt J/Y production ?
• Absorption by hadrons
via charm exchange
• Momentum broadening
• Color screening
• Ionization by (thermal)
gluons
The J/Y Story - Continued
Color screening may not suffice to
dissolve J/Y at SPS. Dissociation
by mesons in HG or gluons in QGP.
Much theoretical progress
(Rapp et al., Duraes et al.,
Maiani et al.,…):
dis(QGP) ~ 1-1.5 mb
dis(HG)  0.5 mb
(T<Tc)
Rapp et al.
T=160 MeV is
not enough !
Maiani et al.
Charm Enhancement…
…could upset the picture
Needed Charm Measurements
•
•
•
•
•
Open charm yield needs to be measured in Pb+Pb
Does charm quarks thermalize and flow?
What is the contribution from recombination?
Are baryons with charm enhanced?
What is the contribution from c to J/Y ?
• Ancillary result: Low-mass l+l- spectrum.
Quark recombination ?
Strong evidence at RHIC
for formation of energetic
(few GeV) hadrons by
quark recombination:
Suggests valence quarks
remain independent until
hadronization, but there is
no evidence for presence
of dynamical gluons.
Is a similar picture valid
at SPS energies? L, X, W
enhancement suggests it.
q q
Recombination
Baryon
1
Meson
q q q
q
q
Fragmentation
Baryon
Meson
1
q
Elliptic Flow at SPS – Pions vs. Protons
Is there a similar scaling law at SPS energies?
NA49
Requires particle ID with good statistics to higher pT
The QCD Critical End Point
If it’s there, we need to find it…
The QCD Critical End Point
Philipsen & Forcrand
Fodor & Katz
Crossover
[Tc(m),c(m)]
First order P.T.
Smaller quark mass
Critical quark masses
mic(B=0)
B=360 MeV
decr.
m
QCD Critical End Point II
Fodor & Katz:
Tc  160 MeV,
Bc  360 MeV;
Ejiri et al.:
Bc  420 MeV
Quark number susceptibility
 E/A ~ 30-40 GeV
Philipsen & Forcrand:
Bc very sensitive to mq
Ejiri et al.
Equation of State Near the CEP
C. Nonaka (Duke) & M. Asakawa
s(T ,  B )  12 [1  tanh Sc (T ,  B )]sH (T ,  B )
Using 3-dim Ising model critical
exponents and scaling hydro.
 12 [1  tanh Sc (T , B )]sQ (T , B )
Hydrodynamics Near the CEP
Focusing effect of critical end
point makes it “easy to find” !
(Tc,c) = (155, 368) MeV
Standard EOS with 1st order phase
transition gives completely different
evolution at phase boundary!
Isentropic trajectories
Dynamical Critical Fluctuations
Dynamical critical enhancement is
almost gone at kinetic freezeout !
• Fluctuations coupled to
critical modes diverge in
equilibrium at CEP,
Critical enhancement survives
if probe decouples early.
• but remain finite in
dynamical scenarios.
Proposed observables:
pT, N Np
Strangeness !!!
Nonaka & Asakawa
L/Ltotal
T [MeV]
Why Look at Strangeness fluctuations?
Because mseff is very sensitive to light quark condensate!
‘t Hooft interaction:
LI  [det f (qR qL )  det f (qLqR )]
qq
sR/L
sL/R
qq
Dynamical strange quark mass
fluctuates with light quark condensate,
but strange hadron abundances freeze
out close to Tc. Strange baryons would
also be sensitive to critical baryon
number fluctuations, but E-by-E
fluctuations may be hard to measure.
Hadron Abundance Fluctuations
(K+K-)/+-
would be better!
Hatta & Stephanov suggest
d(p+-p-)2/(p++p-).
Conclusions
• SPS-HI panorama is coming into focus.
• SPS is unique facility to explore critical end point
of QCD phase diagram.
• Critical measurements:
– Open (and hidden) charm hadrons
– Good statistics for ID’d hadrons at pT  4-5 GeV/c
– E-by-E fluctuations for observables with sensitivity to
critical fluctuations and early freeze-out in dependence
of system size
– Coherent bremsstrahlung, gg HBT
Time for Questions