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Heavy Ions Collisions and the searchfor the Quark-Gluon Plasma
Carlos A. Salgado
CERN, TH-Division
([email protected], http://home.cern.ch/csalgado)
1. QCD matter. The final state in HIC.
2. The first stages and before. The initial state in HIC.
3. Signals for the QGP formation.
4. Experimental/Theoretical status.
RHIC
LHC
Islamabad, March 2004 HIC and the search for the QGP – p.1
Summary I+II
QCD vacuum:Confinement & chiral symmetry breaking
Theory −→ Different phases exist!
Order of the transition depends on quarks masses. For realisticmasses, most probably crossover at µB = 0.
Initial state effects
Multiple scattering and coherence effects necessary to describeheavy ion collisions
Large multiplicities in HIC
High densities created
Non-linear terms in the evolution equations appear.
Islamabad, March 2004 HIC and the search for the QGP – p.2
3. Signals of QGP formation
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.3
3. Signals of QGP formation
Final state effects
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.3
High-energy heavy ion collisions
Before the collision: Lorentz-contracted nuclei
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.4
High-energy heavy ion collisions
Before the collision: Lorentz-contracted nuclei
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.4
High-energy heavy ion collisions
at t = 0 most of the energy in the central region
Initial stateIslamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.4
High-energy heavy ion collisions
First ∼ 0.1 ÷ 0.3 fm. Quark gluon plasma formation
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.4
High-energy heavy ion collisions
Expansion and hadronization
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.4
"Canonical" space-time picture
production and ther-malization
Transitions: lines of constant proper time τ .
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.5
"Canonical" space-time picture
QGPproduction and ther-malization
Transitions: lines of constant proper time τ .
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.5
"Canonical" space-time picture
mixed phase??
QGPproduction and ther-malization
Transitions: lines of constant proper time τ .
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.5
"Canonical" space-time picture
hadron gas
mixed phase??
QGPproduction and ther-malization
Transitions: lines of constant proper time τ .
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.5
"Canonical" space-time picture
freeze-outhadron gas
mixed phase??
QGPproduction and ther-malization
Transitions: lines of constant proper time τ .
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.5
Characterization of the medium
The medium (or media?!), if formed, has a very short lifetime. In order tostudy its properties some (indirect) signals are proposed
Soft (bulk) signatures:
Strangeness enhancement
Flows
Particle composition
...
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.6
Characterization of the medium
The medium (or media?!), if formed, has a very short lifetime. In order tostudy its properties some (indirect) signals are proposed
Soft (bulk) signatures:
Strangeness enhancement
Flows
Particle composition
...
Hard probes (large Q2)
J/Ψ suppression
Jet quenching
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.6
Characterization of the medium
The medium (or media?!), if formed, has a very short lifetime. In order tostudy its properties some (indirect) signals are proposed
Soft (bulk) signatures:
Strangeness enhancement
Flows
Particle composition
...
Hard probes (large Q2)
J/Ψ suppression
Jet quenchingProduced at the early (τ ∼ 1/Q)stages
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.6
Soft probes
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.7
Strangeness enhancement
In order to produce strangeness,in a medium with broken chiralsymmetry one needs
mK+ +mK− ∼ 1GeV
In a medium in which chiral symmetry is restored, the energy is just thesum of the strange quark mass,
ms +ms ∼ 150÷ 400MeV
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.8
Strangeness enhancement
In order to produce strangeness,in a medium with broken chiralsymmetry one needs
mK+ +mK− ∼ 1GeV
In a medium in which chiral symmetry is restored, the energy is just thesum of the strange quark mass,
ms +ms ∼ 150÷ 400MeV
1
10
1 10 102
103
pT > 0, |y-ycm| < 0.5
< Nwound >
Par
ticle
/ ev
ent /
wou
nd. n
ucl.
rela
tive
to p
Be
Λ
Ξ-
pBe pPb PbPb
1
10
1 10 102
103
pT > 0, |y-ycm| < 0.5
< Nwound >
Par
ticle
/ ev
ent /
wou
nd. n
ucl.
rela
tive
to p
Be
Λ
Ξ +
Ω-+Ω +
pBe pPb PbPb
Strange baryons enhancement by NA57 (√s=17.3 GeV)
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.8
Statistical description of particle yields
Assuming an ideal gas of particles, the number densities are
ni = −TV
∂ lnZ
∂µi
gi
2π2
∫
∞
0
p2dp
exp[(Ei − µi)/T ]± 1
Only two independent parameters, µB and T (+some assumptions)
Rat
ios
10-2
10-1
1
=130 GeVNNs =200 GeVNNs
Braun-Munzinger et al., PLB 518 (2001) 41 D. Magestro (updated July 22, 2002)
STARPHENIXPHOBOSBRAHMS
Model prediction for = 29 MeVbµT = 177 MeV,
Model re-fit with all data = 41 MeVbµT = 176 MeV,
/pp Λ/Λ Ξ/Ξ Ω/Ω +π/-π +/K-K -π/-K -π/p -/h*0K-
/hφ -/hΛ -/hΞ *10-π/Ω /pp +/K-K -π/-K -π/p *50-/hΩ
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.9
Statistical description of particle yields
Assuming an ideal gas of particles, the number densities are
ni = −TV
∂ lnZ
∂µi
gi
2π2
∫
∞
0
p2dp
exp[(Ei − µi)/T ]± 1
However, it also works for e+e−...
Hadron mass (GeV)
nh
πππ
K
η
ρ0ω
K*
p
η, Φ
Λ
ΣΞ-
∆++
Σ*
Ξ*0 Ω
LEP
T=162.9±2.1 MeV
V=21.4±1.9 Fm3
γs=0.70±0.027
π0 π+ K+ K0 η ρ0 ω K*+K*0p η, Φ Λ Σ0 Σ+ ∆++Ξ- Σ* Ξ*0Ω
Num
ber
of s
t. de
v.
10-3
10-2
10-1
1
10
0 0.2 0.4 0.6 0.8 1 1.2 1.4 1.6 1.8
-4-2024
[Becattini 1995]
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.9
Collective flow
In a non-relativistic fluid, the fluid acceleration is given by Euler’s eq.
dβ
dt= −1
ρ∇P
[
dβ
dt= − c2
ε+ P∇P → relativistic
]
where, β is the fluid velocity, ρ the mass density and P the pressure.Pressure gradients produce collective flow.
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.10
Collective flow
In a non-relativistic fluid, the fluid acceleration is given by Euler’s eq.
dβ
dt= −1
ρ∇P
[
dβ
dt= − c2
ε+ P∇P → relativistic
]
where, β is the fluid velocity, ρ the mass density and P the pressure.Pressure gradients produce collective flow.
Hydrodynamical models are fixed by
An equation of state −→ relation between P and ε.
Initial condition: fluid velocity and energy density.
freeze-out temperature.
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.10
Collective flow
In a non-relativistic fluid, the fluid acceleration is given by Euler’s eq.
dβ
dt= −1
ρ∇P
[
dβ
dt= − c2
ε+ P∇P → relativistic
]
where, β is the fluid velocity, ρ the mass density and P the pressure.Pressure gradients produce collective flow.
Hydrodynamical models are fixed by
An equation of state −→ relation between P and ε.
Initial condition: fluid velocity and energy density.
freeze-out temperature.
Initial condition in a HIC has gradients of energy density. Thistranslates into gradients of the pressure and, by evolution, flow.
Relation between the initial distribution of energy and flow(s).
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.10
Elliptic flow
Gradients are more easily produced in asymmetric media: Changing thecentrality of the collision.
Reaction plane defined by theimpact parameter and thecollision axis.
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.11
Elliptic flow
Gradients are more easily produced in asymmetric media: Changing thecentrality of the collision.
Reaction plane defined by theimpact parameter and thecollision axis.
Doing the Fourier expansion ofthe number of particles in thereaction plane
dN
dφ∝ 1 + 2
∞∑
n=1
vn cos(nφ)
vn characterize the strength ofthe anisotropic flow.
v2 elliptic flow.
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.11
Elliptic flow
Elliptic flow has measured at RHIC (one of the main signals)
0
0.1
0.2
0.3
0 1 2 3 4
pbarK−π−
v 2
pT (GeV/c)0 1 2 3 4
pK+π+
pT (GeV/c)
0
0.1
0.2
0.3
0 1 2 3 4
p pbarK+ K−π+ π−
hydro πhydro Khydro p
v 2
pT (GeV/c)
0
0.05
0.1
0 0.5 1 1.5
p pbarK+ K−π+ π−
v 2/n
qu
ark
pT/nquark (GeV/c)
[STAR data]
Comparison with hydrodynamical calculations
The main interest of elliptic flow is that it is very difficult to generatewithout strong final state interactions/thermalization.
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.12
Hard Probes
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.13
J/Ψ suppression
A J/Ψ is a bound cc state.
We have seen that the potential between two quarks is screened inthe medium.
In this case, the cc pair is diluted in the medium and the production ofbound states is suppressed.
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.14
J/Ψ suppression
A J/Ψ is a bound cc state.
We have seen that the potential between two quarks is screened inthe medium.
In this case, the cc pair is diluted in the medium and the production ofbound states is suppressed.
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.14
J/Ψ suppression II
*p(450 GeV/c)-p,d (NA51)
208
16
p(200 GeV/c)-A (A=Cu,W,U) (NA38)
O(16x200 GeV/c)-Cu,U (NA38)
*
S(32x200 GeV/c)-U (NA38)
*Pb(208x158 GeV/c)-Pb (NA50)
32
p(450 GeV/c)-A (A=C,Al,Cu,W) (NA38)
10101 10101010652 3 4
B target
σ
projectile
µµB
(
J/
)/(
AB
) (n
b)
ψ
5
4
3
2
10.9
0.8
0.7
0.4
0.5
0.6
A
0.06 = 0.74K
R
0.01 = 0.92
* rescaled to 200 GeV/c
α
J/Ψ suppression measured atCERN (NA50).
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.15
J/Ψ suppression II
*p(450 GeV/c)-p,d (NA51)
208
16
p(200 GeV/c)-A (A=Cu,W,U) (NA38)
O(16x200 GeV/c)-Cu,U (NA38)
*
S(32x200 GeV/c)-U (NA38)
*Pb(208x158 GeV/c)-Pb (NA50)
32
p(450 GeV/c)-A (A=C,Al,Cu,W) (NA38)
10101 10101010652 3 4
B target
σ
projectile
µµB
(
J/
)/(
AB
) (n
b)
ψ
5
4
3
2
10.9
0.8
0.7
0.4
0.5
0.6
A
0.06 = 0.74K
R
0.01 = 0.92
* rescaled to 200 GeV/c
α
J/Ψ suppression measured atCERN (NA50).
pA collisions→ nuclear absopt.(multiple scattering cc-A)
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.15
J/Ψ suppression II
*p(450 GeV/c)-p,d (NA51)
208
16
p(200 GeV/c)-A (A=Cu,W,U) (NA38)
O(16x200 GeV/c)-Cu,U (NA38)
*
S(32x200 GeV/c)-U (NA38)
*Pb(208x158 GeV/c)-Pb (NA50)
32
p(450 GeV/c)-A (A=C,Al,Cu,W) (NA38)
10101 10101010652 3 4
B target
σ
projectile
µµB
(
J/
)/(
AB
) (n
b)
ψ
5
4
3
2
10.9
0.8
0.7
0.4
0.5
0.6
A
0.06 = 0.74K
R
0.01 = 0.92
* rescaled to 200 GeV/c
α
J/Ψ suppression measured atCERN (NA50).
pA collisions→ nuclear absopt.(multiple scattering cc-A)
OCu, OU, SU→ nuclearabsoption.
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.15
J/Ψ suppression II
*p(450 GeV/c)-p,d (NA51)
208
16
p(200 GeV/c)-A (A=Cu,W,U) (NA38)
O(16x200 GeV/c)-Cu,U (NA38)
*
S(32x200 GeV/c)-U (NA38)
*Pb(208x158 GeV/c)-Pb (NA50)
32
p(450 GeV/c)-A (A=C,Al,Cu,W) (NA38)
10101 10101010652 3 4
B target
σ
projectile
µµB
(
J/
)/(
AB
) (n
b)
ψ
5
4
3
2
10.9
0.8
0.7
0.4
0.5
0.6
A
0.06 = 0.74K
R
0.01 = 0.92
* rescaled to 200 GeV/c
α
J/Ψ suppression measured atCERN (NA50).
pA collisions→ nuclear absopt.(multiple scattering cc-A)
OCu, OU, SU→ nuclearabsoption.
PbPb ”anomalous suppression”
hadronic or partonic origin?
Lattice results not yet determinant on whether J/Ψ dissociates at Tc orabove. Other cc states, as ψ′ or χc, could dissociate bellow Tc.
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.15
Jet quenching
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.16
Jet quenching
Suppose a particle entering amedium or created inside themedium
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.17
Jet quenching
Suppose a particle entering amedium or created inside themedium
The particle looses energy whiletraveling through the medium
by scattering with the medium
by radiation
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.17
Jet quenching
Suppose a particle entering amedium or created inside themedium
The particle looses energy whiletraveling through the medium
by scattering with the medium
by radiation
At high energy, gluon radiationdominates: medium-induced gluonemission
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.17
Jet quenching
Suppose a particle entering amedium or created inside themedium
The particle looses energy whiletraveling through the medium
by scattering with the medium
by radiation
At high energy, gluon radiationdominates: medium-induced gluonemission
A high-pt particle produced insidea medium will lose energy while es-caping it −→ spectrum suppressedat large pt.
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.17
High-pt production in pp: pQCD
QCD factorization formula:
dσhpp
dp2tdy∼∑
i,j
x1fpi (x1, Q
2)⊗ x2fpj (x2, Q
2)⊗ dσij→k
dt⊗Dk→h(z, µ2
F )
(Eskola and Honkanen: Nucl.Phys. A713 (2003) 167)
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.18
Space-time picture
Before the collision, initial state: nuclear PDF’s.
QCD factorization formula:
dσhAB
dp2tdy∼∑
i,j
x1fpi (x1, Q
2)⊗ x2fpj (x2, Q
2)⊗ dσij→k
dt⊗Dmed
k→h(z, µ2F )
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.19
Space-time picture
At t ∼ 0
QCD factorization formula:
dσhAB
dp2tdy∼∑
i,j
x1fpi (x1, Q
2)⊗ x2fpj (x2, Q
2)⊗ dσij→k
dt⊗Dmed
k→h(z, µ2F )
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.19
Space-time picture
Evolution.
QCD factorization formula:
dσhAB
dp2tdy∼∑
i,j
x1fpi (x1, Q
2)⊗ x2fpj (x2, Q
2)⊗ dσij→k
dt⊗Dmed
k→h(z, µ2F )
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.19
Effects of nuclear PDF.
Nuclear effects in PDF produce small changes in high–pt particleproduction at RHIC and LHC, at most 25 % .
0 5 10 15 200.7
0.8
0.9
1.0
1.1
1.2
1.3
AuAu/AuAu(ns)AuAu/pppAu/pAu(ns)pAu/ppRHIC, sqrt(s)=130 GeV
0 5 10 15 20 25qT (GeV)
AuAu/AuAu(ns)AuAu/pppAu/pAu(ns)pAu/ppRHIC, sqrt(s)=200 GeV
0 50 100 150 2000.7
0.8
0.9
1.0
1.1
1.2
1.3
PbPb/PbPb(ns), 5.5 TeVPbPb/pp, 5.5 TeVpPb/pPb(ns), 8.8 TeVpPb/pp, 8.8 TeVLHC
[Eskola and Honkanen]
Computed using EKS98 nPDF’s.
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.20
Matter affects evolution.
A quark or gluon (traveling in vacuum) with virtuality Q2 will radiategluons to become on-shell: DGLAP-like evolution.
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.21
Matter affects evolution.
A quark or gluon (traveling in vacuum) with virtuality Q2 will radiategluons to become on-shell: DGLAP-like evolution.
Gluon radiation modified when the particle traverses a medium:medium-induced gluon radiation.
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.21
Matter affects evolution.
A quark or gluon (traveling in vacuum) with virtuality Q2 will radiategluons to become on-shell: DGLAP-like evolution.
Gluon radiation modified when the particle traverses a medium:medium-induced gluon radiation.
Where to look?
Inclusive particle (suppression).
Jets: Jetshapes... −→ LHC
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.21
Medium–induced gluon radiation.
u,k)ω(
lyly
)1(E,p
. . .
. . .
. . .. . .. . .
,k)ω(
)1(E,p)2((1-x)E,p)2((1-x)E,p
For media of finite length
ωdItot
dωdk2⊥
=
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.22
Medium–induced gluon radiation.
u,k)ω(
lyly
)1(E,p
. . .
. . .
. . .. . .. . .
,k)ω(
)1(E,p)2((1-x)E,p)2((1-x)E,p
For media of finite length
ωdItot
dωdk2⊥
=
The medium induced gluon radiation
ωdI
dωdk2⊥
= ωdItot
dωdk2⊥
− ω dIvac
dωdk2⊥
Medium: L (length) and q (transport coefficient).
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.22
Double differential spectrum
High energy approximation −→ multiple scattering. The final result is
ωdI
dωdk⊥
=αs CR
(2π)2 ω22Re
∫
∞
ξ0
dyl
∫
∞
yl
dyl
∫
du e−ik⊥·u e−
12
∫
∞
yldξ n(ξ) σ(u)
× ∂
∂y· ∂∂u
∫ u=r(yl)
y=0=r(yl)
Dr exp
[
i
∫ yl
yl
dξω
2
(
r2 − n(ξ)σ (r)
i ω
)]
.
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.23
Double differential spectrum
High energy approximation −→ multiple scattering. The final result is
ωdI
dωdk⊥
=αs CR
(2π)2 ω22Re
∫
∞
ξ0
dyl
∫
∞
yl
dyl
∫
du e−ik⊥·u e−
12
∫
∞
yldξ n(ξ) σ(u)
× ∂
∂y· ∂∂u
∫ u=r(yl)
y=0=r(yl)
Dr exp
[
i
∫ yl
yl
dξω
2
(
r2 − n(ξ)σ (r)
i ω
)]
.
Two approximations
Multiple soft scattering n(ξ)σ(r) = q(ξ)2 r2. The path integral reduces
to a harmonic oscillator of imaginary frequency.
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.23
Double differential spectrum
High energy approximation −→ multiple scattering. The final result is
ωdI
dωdk⊥
=αs CR
(2π)2 ω22Re
∫
∞
ξ0
dyl
∫
∞
yl
dyl
∫
du e−ik⊥·u e−
12
∫
∞
yldξ n(ξ) σ(u)
× ∂
∂y· ∂∂u
∫ u=r(yl)
y=0=r(yl)
Dr exp
[
i
∫ yl
yl
dξω
2
(
r2 − n(ξ)σ (r)
i ω
)]
.
Two approximations
Multiple soft scattering n(ξ)σ(r) = q(ξ)2 r2. The path integral reduces
to a harmonic oscillator of imaginary frequency.
Single hard scattering First order in the opacity expansion parametern(ξ)σ(r).A Yukawa cross section is usually taken for the cross sectionσ(r)
Expansion in the number of scatterings
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.23
Coherent radiation
Two phases appear: quark and emitted gluon
ϕE =
⟨
k2⊥
2E∆z
⟩
ϕ =
⟨
k2⊥
2ω∆z
⟩
=⇒ lcoh ∼ω
k2⊥
High energy limit E →∞ so, the first one is neglected.
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.24
Coherent radiation
Two phases appear: quark and emitted gluon
ϕE =
⟨
k2⊥
2E∆z
⟩
ϕ =
⟨
k2⊥
2ω∆z
⟩
=⇒ lcoh ∼ω
k2⊥
High energy limit E →∞ so, the first one is neglected.Medium −→ transport coefficient q ' µ2
λ , transverse momentum µ2 permean free path λ. So,
k2⊥∼ lcoh
λµ2 =⇒ k2
⊥∼ qL (for lcoh = L)
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.24
Coherent radiation
Two phases appear: quark and emitted gluon
ϕE =
⟨
k2⊥
2E∆z
⟩
ϕ =
⟨
k2⊥
2ω∆z
⟩
=⇒ lcoh ∼ω
k2⊥
High energy limit E →∞ so, the first one is neglected.Medium −→ transport coefficient q ' µ2
λ , transverse momentum µ2 permean free path λ. So,
k2⊥∼ lcoh
λµ2 =⇒ k2
⊥∼ qL (for lcoh = L)
Let us define κ2 ≡ k2⊥
qL, ωc =
1
2qL2
So, the phase for ∆z = L −→ ϕ ∼ κ2 ωc
ω
gluon emitted when ϕ & 1⇐⇒ radiation suppressed for κ2 . ω/ωc
In cold nuclear matter: Q2sat = qL =⇒ κ2 =
k2⊥
Q2sat
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.24
Gluon energy distributions for quark jets
κ2 =k2⊥
qL, ωc =
1
2qL2
Plateau at small κ←→ coherencegluons =⇒ factor Nc/CF larger
ωdI
dω=
∫ ω
0
dk⊥ωdI
dωdk⊥
kinematical limitk⊥ ≤ ω =⇒ R = ωcL finite
Infrared safe.
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.25
Properties of the spectrum
For gluon emission, we have the restriction k⊥ ≤ ω.
Coherence, k2⊥
. qL. =⇒ spectrum suppressed for
ω2 . k2⊥∼ qL ⇐⇒
(
ω
ωc
)2
.2
R, R =
1
2qL3 .
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.26
Properties of the spectrum
For gluon emission, we have the restriction k⊥ ≤ ω.
Coherence, k2⊥
. qL. =⇒ spectrum suppressed for
ω2 . k2⊥∼ qL ⇐⇒
(
ω
ωc
)2
.2
R, R =
1
2qL3 .
−→ Formation time effects suppress IR region.
Removing this limit (R→∞)
limR→∞
ωdI(ω)
dω=αsCR
πln
[
cosh2
√
ωc
2ω− sin2
√
ωc
2ω
]
.
[Baier, Dokshitzer, Mueller, Peigné, Schiff]
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.26
Properties of the spectrum
For gluon emission, we have the restriction k⊥ ≤ ω.
Coherence, k2⊥
. qL. =⇒ spectrum suppressed for
ω2 . k2⊥∼ qL ⇐⇒
(
ω
ωc
)2
.2
R, R =
1
2qL3 .
−→ Formation time effects suppress IR region.
Removing this limit (R→∞)
limR→∞
ωdI(ω)
dω=αsCR
πln
[
cosh2
√
ωc
2ω− sin2
√
ωc
2ω
]
.
[Baier, Dokshitzer, Mueller, Peigné, Schiff]
The total energy loss:
limR→∞
ωdI(ω)
dω−−−→ω<ωc
√
ωc
ω⇐⇒ ∆E =
∫
dωωdI(ω)
dω∼ ωc ∼ qL2
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.26
Medium-modified fragmentation functions I
For large-pt the hadronization takes place outside the medium
Model: (Wang, Huang, Sarcevic, PRL 77 2537)
D(med)h/q (z,Q2) =
∫ 1
0
dε PE(ε)1
1− ε Dh/q(z
1− ε ,Q2) .
P (ε) probability that the hard parton loses a fraction of energy ε.
Independent gluon emission approx.: (BDMS, JHEP 0109:033)
PE(ε) =∞∑
n=0
1
n!
[
n∏
i=1
∫
dωidI(ωi)
dω
]
δ
(
ε−n∑
i=1
ωi
E
)
exp
[
−∫
dωdI
dω
]
.
P (ε) = p0δ(ε) + p(ε)
p0 ⇒ no E.loss
p(ε)⇒ sum for n ≥ 1.
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.27
Medium-modified FF II
Quenching weights for quarks.
Tabulated: http://home.cern.ch/csalgado
R =q
2L3 =
L2
R2A
dNg
dy
Suppression of ∼ 5 for pt ∼ 5÷7GeV =⇒ R∼ 2000.
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.28
Comparison with PHENIX data.
At RHIC, particles with pt . 10 GeV have been measured.
Ratio with proton-proton:
RAA =dNAA/dpt
NcolldNpp/dpt
RAA = 1⇒ no effect.
A factor of 5 suppression forcentral AuAu collisions.
Smallest values of pt are in thelimit of applicability of the calcu-lations.
Can be described with dNg/dy ∼ 1000÷ 2000.
Some estimates [X-N Wang]
ε|τ∼0.2fm/c ∼ 15GeV/fm3
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.29
Summary III
In order to characterize the created medium (indirect) signals arenecessary.
Soft: strangeness enhancement, particle ratios, flows
Hard: J/Ψ suppression, jet quenching
Hard probes specially interesting as
they are created at very short times ∼ 1/Q
can be described by perturbative QCD
All these effects have been measured in nucleus-nucleus collisions,however, they can also be produced by
Nuclear effects in the initial state (shadowing...)
Interaction with a confined medium (pion gas...)
Study proton-nucleus collisions as a control experiment.
Islamabad, March 2004 HIC and the search for the QGP - 3. Signals. – p.30