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Thermal fits of hadron yields and the QCD phase diagram Talk from Gregor Dentinger 8.11.2012 | Gregor Dentinger | 1

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  • Thermal fits of hadron yields and the QCD phasediagramTalk from Gregor Dentinger

    8.11.2012 | Gregor Dentinger | 1

  • Topics

    Heavy-Ion Collisions

    Historical Meaning: Perturbation Theory vs Statistical Physics

    Thermal fits

    Phase diagram

    8.11.2012 | Gregor Dentinger | 2

  • Basic notation

    I ’High-Energy’: Energy per nucleon� nucleon massI Spectators and ParticipantsI Rapidity and pseudorapidity

    8.11.2012 | Gregor Dentinger | 3

  • Why do we use high center of mass energies?

    Figure: Particle production in dependence of√

    sNN [Andronic, 2012]

    8.11.2012 | Gregor Dentinger | 4

  • Heavy Ion collision participants

    I Difference between participants and the whole nucleusI All data has been taken from central collision

    Figure: Participants and Spectators from [www.hep.lu.se]

    8.11.2012 | Gregor Dentinger | 5

  • Rapidity and pseudorapidity

    y =12

    ln(E + p‖)(E − p‖)

    = arctanh(v‖) (1)

    Rapidity is a simplification for dealing with relativistic energies.I replace velocity with rapidityI additive under Lorentz boosts along the beam axisI not an observable

    η =12

    ln(|p| + p‖)(|p| − p‖)

    = − ln(tan θ2

    ) (2)

    I observable scattering angle θI for low hadron masses mH → 0, η = y

    Note: η ' 7 means a scattering angle of 0.1 degrees, i.e. close to the beam!

    8.11.2012 | Gregor Dentinger | 6

  • Rapidity and pseudorapidity distribution

    dNdηd2p⊥

    =|p|E

    dNdyd2p⊥

    (3)

    for midrapidity with y ≈ η ≈ 0

    dNdηd2p⊥

    ∣∣∣∣η=0

    =p⊥m⊥

    dNdyd2p⊥

    ∣∣∣∣y=0

    (4)

    8.11.2012 | Gregor Dentinger | 7

  • Experimental reference

    Figure: Rapidity and pseudorapidity distribution at√

    sNN = 200GeV [iopscience.iop.org][BRAHMS, 2004]

    8.11.2012 | Gregor Dentinger | 8

  • Historical: One Pion production

    Started with Landau in 1950 - statistical concepts for hadronic collision analysis.Probability S for a state with n particles (also used by Fermi):

    S(n) =[

    V(2π)3

    ](n−1) dQ(W )dW

    (5)

    With W := total energy of the system,dQdW

    := number of states per unit energy and

    V := volume of interaction.The n-1 corresponds to n-1 independent momenta.

    8.11.2012 | Gregor Dentinger | 9

  • Probability for states with 2 and 3 particles

    In this case we use W = Tkin and V = V0 (not Lorentz contracted↔ low energy)

    Q2 =∫

    d3q1d3q2θ(

    Tkin −q21

    2mN− q

    22

    2mN

    )δ(3)(q1 + q2)

    =∫

    d3q1θ(

    Tkin −q21mN

    )= 4π

    ∫ √TkinmN0

    q21dq1

    =4π3

    (TkinmN )3/2

    (6)

    8.11.2012 | Gregor Dentinger | 10

  • Two and three particle probability

    S(2) =[

    V(2π)3

    ]1 dQ2dTkin

    =Vm3/2N

    4π2T 1/2kin

    (7)

    For three particle production one can find

    S(3) =V 2m3/2N m

    3/2π (∆Tkin)

    2

    32√

    2π3(8)

    S(3)S(2) + S(3)

    ≈ S(3)S(2)

    ≈ Vmπ8√

    2π(Tkin −mπ)2 (9)

    8.11.2012 | Gregor Dentinger | 11

  • One pion model proved

    S(3)S(2)

    =1

    6√

    2

    (Tkinmπ− 1)2

    (10)

    I compared to 345MeV beam energy data (proton energy 1950 at Berkeley)I good agreement with dataI statistical idea works very wellI for high energies statistical consideration can be replaced with

    thermodynamic arguments

    8.11.2012 | Gregor Dentinger | 12

  • Canonical Ensembles

    I Grand canonical:I system depends on µ (for sort of particle), V and TI system can exchange particles and internal energyI in equilibrium with an external reservoir

    I Canonical:I system described with N, V and TI only internal energy may exchanged

    I Micro canonical:I system with parameters of N, V and internal energyI isolated system

    8.11.2012 | Gregor Dentinger | 13

  • The thermal model

    Ni = giV∫

    d3p(2π)3

    [exp

    (Ei (p)− µi

    T

    )+ �]−1

    (11)

    with Ni multiplicity for the ith sort of particle, gi spin degeneracy, V fireball volume,µi chemical potential, Ei total energy, T temperature and � variable for fermions(+1) or bosons (-1).

    I µi contains all chemical potentials for strong interacting matter⇒ µi = µbBi + µsSi + µI3 Ii + µCCi

    I conservation for baryon number, strangeness, isospin and charm reduces thedegrees of freedom in equation (11) to three:⇒ parameters left: µb, T and V

    8.11.2012 | Gregor Dentinger | 14

  • Thermal fit

    Calculation for thermal fits with minimizing

    χ2 =n∑

    k=1

    (Rexpk − Rmodelk

    )2σ2k

    (12)

    with Rexpk k-th measured ratio, σk corresponding error and Rmodelk the theoretical

    result for the same ratio

    I using grand canonical ensemble for the thermal modelI Rk will be replaced with the hadron yields (determine T, µb and V) or hadron

    ratios (no V)

    8.11.2012 | Gregor Dentinger | 15

  • A thermal fit

    Figure: Thermal fit from [Andronic et al., 2006]

    8.11.2012 | Gregor Dentinger | 16

  • Canonical suppression

    Figure: Suppression factor[Andronic et al., 2006]

    For low energies strangeness carry-ing particles are suppressed by anenergy depending factor

    nCi ,S = nGCi ,S

    IsI0

    (13)

    8.11.2012 | Gregor Dentinger | 17

  • A thermal fit

    Figure: Thermal fit from [Andronic et al., 2006]

    8.11.2012 | Gregor Dentinger | 18

  • More thermal fits

    Figure: Thermal fit from [Andronic et al., 2006] [Andronic et al., 2012]

    8.11.2012 | Gregor Dentinger | 19

  • Energy dependence of T, µb

    Figure: Energy dependence of T and µb [Andronic et al., 2006]

    8.11.2012 | Gregor Dentinger | 20

  • Values for T and µb

    Saturation for Tsat ∼ 164MeV

    Tchem =Tsat

    1 + exp(2.60− ln

    (√sNN [GeV ]

    )/0.45

    ) (14)For µb the empirical parametrization is

    µbchem =1303MeV

    1 + 0.286√

    sNN [GeV ]. (15)

    8.11.2012 | Gregor Dentinger | 21

  • The horn

    I the horn is well described in thethermal model[A. Andronic et al., 2009]

    I found at about 10GeVI close to the saturation

    temperature

    8.11.2012 | Gregor Dentinger | 22

  • The horn structure in K +/π+ ratio with anothermodel

    Figure: I - pure initial hardroniccalculation; II - initial partonic calculationfor higher

    √sNN [Nayak et al., 2010]

    I transport modelI calculation with pure hardronic

    assumption does not fit with theexperimental data

    I at about 10GeV partonicformation (according to thismodel)

    8.11.2012 | Gregor Dentinger | 23

  • LHC data

    Figure: All data fit [Andronic et al., 2012]

    8.11.2012 | Gregor Dentinger | 24

  • What do we see in this picture?

    I The ’all data fit’ is good for single strange baryons and also for mesonsI very poor for multi-strange baryonsI underpredicted multi-strange baryons in all thermal fitsI new data implies a much lower value for T than in lower energy experimentsI nothing like a saturation

    ⇒ what is wrong?⇒ some models showed annihilation at the phase boundary for baryons⇒ fit without p, p̄ yields⇒ annihilation for Λ, Ξ and Ω is not observed?!

    8.11.2012 | Gregor Dentinger | 25

  • Fit with all data vs fit without p, p̄ yields

    Figure: Left: thermal fit with all data; right: fit without considering p, p̄ [Andronic et al., 2012]

    8.11.2012 | Gregor Dentinger | 26

  • Conclusions from fit without p, p̄

    I overall better agreement with ALICE data⇒ compare χ2

    I proton is about 1.4 times below the fitI excellent value for temperature, agrees with all low energy calculations

    8.11.2012 | Gregor Dentinger | 27

  • QCD phase diagram

    Figure: Phase diagram [Andronic et al., 2006]8.11.2012 | Gregor Dentinger | 28

  • What to say about this phase diagram?

    I only experimental connection to the phase diagramI the chemical freeze-out describes a snapshot of the time evolution of the hot

    fireball created in the collisionI saturation in T leads to a connection to the QCD phase boundaryI probably the chemical freeze-out temperature is the hadronization

    temperature

    8.11.2012 | Gregor Dentinger | 29

  • Summary: Thermal fits

    I the fits with the thermal model work, for low energies and at high energieswithout respect pp̄, really well

    I one can speak of a phase boundary temperature (saturation at (164±4)MeV)I some kind of experimental evidence for the QGP (horn)?I only way to put data on the phase diagramI chemical freeze-out is the earliest part in timeline which is measuredI thermal fit with LHC data is not good, but needs further understanding

    8.11.2012 | Gregor Dentinger | 30

  • Resources

    A. Andronic; 2012; The study of quark-gluon matter in high-energynucleus-nucleus collisions; arXiv:1210.8126v1

    A.Andronic, P.Braun-Munzinger, J.Stachel; 2006; Hadron production in centralnucleus-nucleus collisions at chemical freeze-out; Nucl.Phys.A772:167-199,2006 -arXiv:nucl-th/0511071

    A.Andronic, P.Braun-Munzinger, J.Stachel; 2009; Thermal hadron production inrelativistic nuclear collisions: the hadron mass spectrum, the horn, and the QCDphase transition; Phys.Lett.B673:142,2009 - arXiv:0812.1186

    http:

    //www.hep.lu.se/staff/tydesjo/physics/theses/lichtml/node6.html

    http://iopscience.iop.org/0295-5075/61/6/736

    8.11.2012 | Gregor Dentinger | 31

    http://www.hep.lu.se/staff/tydesjo/physics/theses/lichtml/node6.htmlhttp://www.hep.lu.se/staff/tydesjo/physics/theses/lichtml/node6.htmlhttp://iopscience.iop.org/0295-5075/61/6/736

  • Resources

    BRAHMS Collaboration; 2004; Charged meson rapidity distributions in centralAu+Au collisions at

    √sNN = 200 GeV; Phys.Rev.Lett. 94 (2005) 162301 -

    arXiv:nucl-ex/0403050

    A. Andronic, P. Braun-Munzinger, K. Redlich, J. Stachel; 2012; The statisticalmodel in Pb-Pb collisions at the LHC; arXiv:1210.7724

    Jajati K. Nayak, Sarmistha Banik and Jan-e Alam; 2010; The horn in the kaon topion ratio; Phys. Rev. C 82 (2010)024914 - arXiv:1006.2972

    P. Braun-Munzinger, J.Stachel; 2011; Hadron Production in Ultra-relativisticNuclear Collisions and the QCD Phase Diagram: an Update; arXiv:0911.4806

    8.11.2012 | Gregor Dentinger | 32

  • Time left? Volume dependence?

    For the LHC energy, thevolume is highly increased.The fits are still good. Thisindicates a fixed densityfor the chemical freeze out.[Braun-Munzinger et al., 2011]

    8.11.2012 | Gregor Dentinger | 33

    Heavy-Ion CollisionsHistorical Meaning: Perturbation Theory vs Statistical PhysicsThermal fitsPhase diagram