Dilepton production in statistical models
J. Manninen 1
1
Frankfurt Institute for Advanced Studies
May 3, 2013
Outline
1 Introduction
2 Statistical hadronization model Freeze-out decay cocktail
3 Di-electron radiation
Introduction
Introduction
Invariant mass spectrum of di-lepton pairs carry plenty of information
p+p well understood in terms of CFO cocktail
Deviations from cocktail in A+A: dynamics, energy loss, quarkonia melting, in-medium modication, QGP
Electromagnetic signals survive the evolution and are separable
→ oers windows to look into all stages of evolution
Statistical hadronization model
Statistical hadronization: counting the number of hadrons
Statistical Hadronization Model:
Statistical equilibrium:
a priori equal probabilities Boltzmann energy spectrum Resonant interactions
Include all resonances ≈ interactions
arXiv:0901.2909v2
All light (uds) hadron yields can be described in all collision systems Also the yields that are dicult to measure (η, ω, ρ ...)
Free parameters of the model:
T , γ and normalisation
Statistical hadronization model
Statistical model as an event generator
h N j i = (2J j + 1)V ( 2π) 3
Z Z
γ S − n
se qp
2+ m
2j/ T −µ·q
j/ T
− 1
× SF (m)d 3 pdm
Choose thermal parameters, calculate (once) hN j i as usual Sample for each event N i :s from Poisson with hN j i
Sample N i hadrons (+momenta & masses) for each event Easy to implement geometrical / kinematic cuts
Easy to emulate clusters' dynamics
Statistical hadronization model Freeze-out decay cocktail
Cocktail at RHIC and LHC
Above SPS energies, mesons completely dominate the decay cocktail but baryons aect indirectly the cocktail composition (relative yields) + potentially strong in-medium modication of vector mesons
Hadron direct Dalitz other
π 0 - π 0 → γ e + e − -
η 0 - η 0 → γ e + e − η 0 → π + π − e + e − η 0 - η 0 → γ e + e − η 0 → π + π − e + e −
ρ 0 ρ 0 → e + e − - -
ω 0 ω 0 → e + e − - ω 0 → π 0 e + e − φ 0 φ 0 → e + e − - φ 0 → η e + e − J/ψ J/ψ → e + e − J/ψ → γ e + e −
ψ 0 ψ 0 → e + e − ψ 0 → γ e + e − -
D mesons - - D ± → e ± ν e + X
B mesons - - B → e ± ν e + X
Statistical hadronization model Freeze-out decay cocktail
Mass dependent widths for the di-lepton sources
Example ρ 0 direct decay
Partial width : Γ V →l
+l
−(m) = m 3 0
m 3 Γ V →l
+l
−(m 0 ) Total width : Γ tot (m) ≈ Γ ρ→ππ (m) = Γ 0 m 0 2
m 2
p
m 2 − 4m 2 π
q m 0 2 − 4m 2 π
3
Branching fraction(ρ 0 → e + e − ) = Γ V →l
+l
−( m)
Γ tot ( m)
Statistical hadronization model Freeze-out decay cocktail
But the clusters are moving
SHM does not tell anything about the clusters' distributions
Assumption: Clusters have Gaussian rapidity and p T distributions Every p+p interaction produces always 2 equal mass clusters RHIC: t σ y and σ p
T(means are set to zero)
LHC: σ y and σ p
Tcalculated from models
Statistical hadronization model Freeze-out decay cocktail
SHM transverse momentum spectra at 2.76 TeV
SHM: T=170MeV ; γ S = 0.6 (p+p) γ S = 0.95 (Pb+Pb) ; V 0 =70fm 3
In thermal equilibrium, energy is shared equally among available forms
⇒ In each event in the rest frame of the cluster M clust = P
i E i
Transverse momentum of the cluster in LAB frame is normally
distributed with h|~p clust |i == M clust and σ p
T= M clust / 2
Statistical hadronization model Freeze-out decay cocktail
Landau scaling in longitudinal direction
Projectile/Target dynamics spread the thermal distribution Random (Gaussian) boosts along z-axis σ y clust ( √
s) = ln( √ s/2m p )
Boosts do not change the inv. mass of a correlated dilepton pair
Statistical hadronization model Freeze-out decay cocktail
Transverse momentum boosts and p T cuts
Light hadrons→ e + e −
ALICE acceptance
Di-electron radiation
From p+p to A+A with Glauber model
Light (uds) hadron yields are scaled with N P
Heavy (cb) hadron yields are scaled with N bin
Scaling works well at RHIC
May not be a good approximation at LHC
Model dependent extrapolation to A+A (especially semi-central)
Di-electron radiation
Low invariant mass region at 2.76 TeV
Low invariant mass region is dominated by the freeze-out decay cocktail
T=170MeV ; γ S = 0.6 ; V=2V 0 γ S = 0.95 ; V=380V 0
Di-electron radiation
SHM vs. PHSD at LHC 2.76 TeV
Cocktails agree well in p+p
ρ 0 enhanced due to nite length hadronic phase in PHSD
η 's involve dierent di-lepton channels
Di-electron radiation
Statistical model vs. HSD transport calculations at RHIC
SHM agree very well with the hadronic transport model HSD at RHIC Au+Au
No evidence for prolonged hadronic radiation
Di-electron radiation
Di-electron radiation from QGP in Pb+Pb 2.76 TeV
QGP dominates the M ∈ [M φ : M J/ψ ]
over heavy avor radiation at LHC SHM insucient for A+A Di-electrons provide a unique window to
detect and study properties of QGP at LHC
Di-electron radiation
Invariant mass spectrum in LMR in p+p √
s NN =200 GeV
LMR can be understood well within the simple model
Di-electron radiation
The PHENIX excess
Di-electron radiation
Beyond standard cocktail contributions
X → K ¯ K → e + e − ν e ν ¯ e Hadron
f 0 ( 980) K + K − K 0 K ¯ 0 -
f 1 ( 1285) - - K ¯ Kπ
f 2 ( 1270) K + K − K 0 K ¯ 0 - f 0 0 ( 1350) K + K − K 0 K ¯ 0 - f 1 0 ( 1420) K ∗+ K − + c.c K ∗ 0 K 0 + c.c - f 2 0 ( 1525) K + K − K 0 K ¯ 0 - f 0 ( 1500) K + K − K 0 K ¯ 0 - f 1 (1510) K ∗+ K − + c.c K ∗ 0 K 0 + c.c - f 2 ( 1430) K + K − K 0 K ¯ 0 -
φ K + K − K 0 K ¯ 0 -
a 0 0 ( 980) K + K − K 0 K ¯ 0 -
K(892) ± K ± π 0 - -
K(892) 0 K 0 π 0 - -
Di-electron radiation
Excited mesons and other exotic contributions EPJC71,1615
Exotic states may contribute to the PHENIX excess:
X → K ¯ K → e + e − ν e ν ¯ e
Upper limit estimate still below the PHENIX data
Di-electron radiation
STAR measurement at 200 AGeV
STAR excess ≈ 2 with measured standard cocktail calculation Measurement of η, η', ρ 0 very challenging in A+A (QCD/pp ratios)
⇒ call for detailed dynamical modeling
Di-electron radiation
ρ 0 broadening can explain the STAR excess PRC85,024910
Broadening of ρ 0 lifts the excess region in PHSD with factor of ≈ 2
Exotic states feed the same region PHENIX acceptance
Di-electron radiation
Conclusion
SHM provides essentially parameter free calculational scheme to
study di-lepton radiation in p+p(¯p) collisions at ultra-relativistic
energies
Di-electron radiation
back up slides
Di-electron radiation
Correlated open heavy avour feed IMR
Heavy avor total cross sections Angular distribution of mothers Momentum distribution of mothers Decay form factors
Relative multiplicities (BRs)
Angular correlation of daughters
Di-electron radiation
Extended SHM for open heavy avour production
Open heavy avor is assumed to be in relative chemical equilibrium Relative yields of 6 (18) lowest D (B) mesons evaluated within SHM
with T=170MeV ; γ S hard =0.3 ; µ { B,S,Q} = 0
p+p: σ ¯ cc tot (2.76TeV)=3.6mb (experimental data) (or γ c ≈ 30) p+p: σ ¯ bb tot (2.76TeV)=1/40 σ tot ¯ cc (MC@ s HQ)
Pb+Pb: σ ¯ cc tot (2.76TeV)=N bin σ cc tot ¯ (2.76TeV) (also σ bb tot ¯ )
LHCb ALICE T=170 MeV T=150 MeV
D∗+D0 2.20 ± 0.48 2.09 2.40 2.49
D0D+ 2.07 ± 0.37 2.08 2.37 2.25
D0Ds 7.67 ± 1.67 7.98 8.55
D∗+D+ 0.94 ± 0.22 1.00 0.99 0.90
D∗+Ds 3.48 ± 0.93 3.32 3.44
D+Ds 3.70 ± 0.84 3.37 3.81
Di-electron radiation
Heavy avour rapidity distributions in p + p collisions
Probability to nd parton along the rapidity axis is dened by a triangle whose maximum is at y cm and goes to zero at
y = asinh(x 1 √
s/2m N ) & y = −asinh(x 2 √
s/2m N )
y cm = atanh( x x
11− + x x
22)
Di-electron radiation Heavy avour energy-loss and correlations
Heavy avour p T and energy loss PRC78,014904
pQCD: c and b quark cross sections & initial momentum
MC@ s HQ evolution: running coupling & improved infrared regulator HQ propagate in Heinz & Kolb hydro background
→ simultaneous R AA and v 2 @ RHIC (K coll = 2 ; K coll+rad = 0.6)
The model is in agreement with preliminary R AA of D mesons at LHC
Di-electron radiation Heavy avour energy-loss and correlations
Angular correlations of open heavy avor mesons at LHC (in)
p+p: π correlations among heavy avour mesons == hardest (up limit) central Pb+Pb: correlations are washed out == softest (low limit)
P corr ∼ R AA 2 < 10%
Di-electron radiation Heavy avour energy-loss and correlations
Angular correlations of open heavy avor mesons (out)
p+p: exact back-to-back correlations among heavy avour mesons central Pb+Pb: correlations are washed out (P corr ∼ R AA 2 < 10%)
Central Pb+Pb: J/ψ=0.3N bin J/ψ pp ; ψ'=0.4N bin ψ 0 pp PRC85,054905
Vanishing correlations in Pb+Pb → softer M spectrum (both D & B) m b > m c → due to, energy loss, D mesons M spectrum softens
more than B mesons M spectrum in Pb+Pb (model dependent ×ing)
Di-electron radiation Heavy avour energy-loss and correlations
Angular correlations at RHIC √
s NN =200 GeV
Di-electron radiation Heavy avour energy-loss and correlations