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							    The first two years of RHIC:
       predictions vs. reality

Summary of the workshop:
Who wins the wine, and why?

And, by the way,

What did we learn from the exercise?
   Particle yields and spectra


 global quantities
 hadron distributions
What do the data say?
                              G. Roland

           dNch/dh = 640

            Rises somewhat faster than Npart
                  Rapidity distribution

PHOBOS




dNp/dy ~ 220-230 per charge
dNK+/dy ~ 40
dNp/dy ~ 28
Net baryon density at mid-y
 small, but not 0  mB small
                     Transverse energy
PHENIX preliminary
                           ET/particle
                           ~ 0.9 GeV




                           Similar cent.
PHENIX preliminary         dependence
                           as <pt>

                           But <pt> goes
                           up with s by
                           20% while
                           ET is constant
                            particle mix
                           is changing
           Anti-particle/particle ratios
                                                 I. Bearden

                           Ratios similar to those in p+p!



                                               p+p collisions


        BRAHMS 200 GeV



At mid-rapidity:
Net-protons: dN/dy  7         ISR
proton yield: dN/dy  29       extrapolation
 ¾ from pair-production
What model can reproduce the net baryons?

                       Net baryon central
                       plateau (y=0 to ~ y=2)
                       Cannot (yet) differentiate
                       AMPT vs. HIJING/BJ
                AMPT - CheMing Ko
                                             Degree of difficulty = 3.5

 Ingredients:
     HIJING, ZPC parton cascade, ART hadronic rescatting
   ET = 750 GeV at y=0 (50% off  *)
       data say: 3.3 GeV x (300/2) = 495 GeV
   80 baryons at y= 3.9 (data say 34 at y=3.5)
     at y=0: 14 p, 10 pbar; pbar/p = 0.6 (data say 29, 22, 0.74)
                (ratio is within 25% of data  ***)
   dNch/dh ~ 800               (dNch/dh within 25%  ***)
     430 p, 60 K per unit y at mid-y (data say 640 ,230, 40)
   Central plateau |y|<1.5 for mesons
                (pion data says 1.5  *****)

                        Total score: 3.5 + 10.5 + 10.5 + 17.5= 42
               What did we learn?

 To get proper particle yields must tweak model so it no
  longer agrees with pp collisions
   Changed fragmentation function to match lower s
     data, rationale: fragmentation in dense matter

 Must add a partonic phase with large scattering cross
  sections to reproduce v2 and HBT

 To reproduce K-/K+ need additional hadronic
  rescattering channels
   Then get f  K+K- correct in s = 130 GeV/A data
                 LEXUS – Joe Kapusta
                                                Degree of difficulty = 2

 Ingredients: parameterized p+p collision results, Glauber,
    NN hard collision probability parameter l = 0.6
   Minimalist approach, which works at SPS
   Net proton density = 13 (data say 7  *)
   dNch/dy = 1200, but should have been 950 using p+p at
    proper s
     Correcting by 15% for yh, get 1020 or 800
     (800 is within 25% of data, but –1 for p+p oops  **)
   Particle spectra are too steep, but missing power law tail
   proton <pT> ~ 0.925 GeV/c (data say 0.94  *****)

                                      Total score: 2 + 4 + 10 = 16
    (so their next model will be a Bentley…?)
                What did we learn?

 Create more hadrons in LEXUS than in wounded
  nucleon model, since wounded nucleons are not sterile
  in LEXUS. Overprediction  some destructive
  interference among stopped nucleons at mid-y?

 Total multiplicity is fixed by energy conservation
 Baryon density fixed by Dy in each collision


 Minimalist picture works ~ OK for the simplest
  observables, but not for more complex ones
 Caution in interpreting scaling with Ncoll or Npart !
Particle Spectra @ 200 GeV




                              BRAHMS: 10% central
                              PHOBOS: 10%
                              PHENIX: 5%
                              STAR: 5%




     QM2002 summary slide (Ullrich)
      Feed-down matters !!!
                          <pT> vs. Npart          J. Velkovska
 <pT> [GeV/c]




                                <pT> [GeV/c]
                                                     •Systematic error on
                                                       200 GeV data
                                                     p (10 %), K (15 %),
                                                      p (14 %)




                open symbol :
                130 GeV data



• Increase of <pT> as a function of Npart and tends to saturate
p < K < proton (pbar)
• Consistent with hydrodynamic expansion picture.
               Radial flow

                             <pT> prediction with Tth
                             and <b> obtained from
STAR
                             blastwave fit (green line)

                             <pT> prediction for
 preliminary                 Tch = 170 MeV
 F. Wang                     and <b>=0
                             pp no rescattering,
                             no flow
                             no thermal equilibrium

                                <pT> of X and W from
                                exponential fits in mT
                                Do they flow ? Or is
                                <pT> lower due to
                                different fit function?
     Does it flow? Fits to Omega mT spectra
 M. van Leeuwen (NA49)                                C. Suire (STAR)

                                                     STAR preliminary




                                     RHIC
    SPS/NA49



                                       bT is not well constrained !


• At SPS W and X are now found to be consistent with common freeze-out
• Maybe W and X are consistent with a blastwave fit at RHIC
• Need to constrain further  more data & much more for v2 of W
                    UrQMD - Bleicher
                                               Degree of difficulty = 2

 Ingredients: excitation and fragmentation of color strings,
    formation and decay of hadronic resonances, hadronic
    rescattering
   dET/dh = 600, dNch/dh = 750, ET/Nch = 0.85 GeV
     Data say 495, 640, 0.9
     Get ET to 20%, Nch to 17%  *** and ***
   y=0: 12 net protons, 400 p-, 45 K+
     Data: 7, 230, 40  *, *, and ****
   <pT> = 375, 500, 780 for p, K, p
     Data: 400, 650, 940  ****
                                                       Score = 32
        not enough radial flow!
   v2 ~ 1% (way too low as the strings don’t collide)
        Dense set of non-interacting strings… a problem…
                  We learned that

 Need QGP-type equation of state to get the v2 and
  radial flow correctly
   UrQMD has insufficient initial pressure as the strings
     don’t scatter.

 Mass shifts of resonances very sensitive to breakup
  dynamics. Resonances are not dissolved  implies fast
  freeze-out
   Statistical model summary - Magestro
                                                  Degree of difficulty = 1
 Johanna: chemical equilibrium with T=170 MeV, mB =
  10 MeV
 Johann: sudden freezeout with incomplete chemical
  equilibrium
     Predictions (200 GeV)
                              Exptl. (130 GeV)   Exptl. (200 GeV)
                              0.66                0.75
                             0.074               0.076       T=177MeV
                              0.90                0.95
                                                             mB =29 MeV
                              0.15                0.15
                             0.75
                             STAR     PHENIX
                              0.58     0.89      Scores:
                              0.66     0.95      Johanna – within ~15%
                             0.021                       ****
                              0.19
                                                 Johann - within ~ 40%
                             0.0015                      **
       Lessons from statistical analyses

 See chemical equilibrium populations at RHIC as at SPS
   mB is lower, but not as low as predicted
   No anomalous strangeness enhancement

 Simple thermal emission produces proton spectra flatter
  than pion spectra, so they must cross someplace!
   Of course the big question is where and why there??
Elliptic flow
      Centrality dependence of v2
Note possible dependence on low pt cut
                                                         200 GeV: 0.2< pt < 2.0
                    130 GeV: 0.075< pt < 2.0
                    200 GeV: 0.150< pt < 2.0
                    4-part cumulants
           STAR


             v2=0.05



                                   STAR                     Preliminary
                                      Preliminary



                         200 GeV: Preliminary




          - Consistent results
          - At 200 GeV better pronounced decrease
            of v2 for the most peripheral collisions.

                       QM2002 summary slide (Voloshin)
                                A puzzle at high pT   Nu Xu


Adler et al., nucl-ex/0206006




 Still flowing at pT = 8 GeV/c? Unlikely!!
v2 of mesons & baryons
                                   Au+Au at sNN=200GeV



                1) High quality M.B. data!!!

                2) Consistent between
                   PHENIX and STAR

                pT < 2 GeV/c
                  v2(light) > v2(heavy)
                                                         v2
                pT > 2.5 GeV/c
                  v2(light) < v2(heavy)




                Model: P.Huovinen, et al., Phys. Lett.
                       B503, 58 (2001)
  Hydrodynamics – Ulrich Heinz, Peter Kolb
                                     Predictions of major importance!

 Ingredients: thermal with some initial conditions, QGP EOS
  early with transition to resonance gas, geometry + Glauber,
  hydrodynamics
 Predictions:
   Thermalization by 0.6 fm/c at RHIC
   v2 as function of pion multiplicity density (to fix initial cond.)
   v2 has a dip (~5%) due to phase transition softening EOS
     RHIC is near this point (data says v2 ~ 6%)
   v2 vs. pT increases to 2 GeV/c
   v2(mesons) > v2 (baryons)
   spectra (once initial condition is fixed)
 Lessons: v2 requires early rescattering! Hadronization follows
  thermalization by 5-7 fm/c. But, final state decoupling needs
  work (get HBT wrong)
    Hydrodynamics –Teaney & Shuryak

 Ingredients: hydrodynamics + RQMD for hadronic
  state and freeze-out
 Predictions:
   RHIC should be near softest point in EOS
   s dependence of v2 correctly predicted for b=6 fm
   fixed initial conditions, then got spectra correct
   Predict particle yields without rescaling
   Initial entropy too high, HBT radii too large!
 Lessons: hydro good to pT ~ 1.5 GeV/c
   Viscosity corrections may be important; cause v2 to
      bend over at 1 GeV/c pT (compared to ideal gas).
      Also helps reduce HBT radii. Maybe small viscosity
      early, but increases in hadron gas phase?
  Parton transport theory – Denes Molnar
                                         Degree of difficulty = 5

 Next step beyond hydro – calculate parton transport, fixing
  s (i.e. transport opacity c)
 Predictions & insights:
   ET loss due to pdV work so (ET)cent < (ET)peripheral
     ET results require small s (3 mb)
     can’t easily fix up with inelastic collisions
     need parton subdivision to avoid numerical “viscosity”
   Can reproduce v2 if dNgluon/dy very large or sel= 45 mb
   But large opacity underpredicts HBT spectra!

   pQCD fixes dNgluon/dy at large pT
   pQCD fixes partons at large Q2
    Picture doesn’t want to hang together!
                    Next, jets and high pT

  summary from
Thomas Peitzmann,
    QM2002
                              Charged Hadron Spectra

200 GeV results
from all experiments

Shape changes from peripheral  central

   Preliminary sNN = 200
   GeV




            Preliminary sNN = 200 GeV                 C. Roland,
                                                       PHOBOS
                                                       Parallel Saturday
                 p/p at high pT

                                   Higher than in p+p
                                   collisions or fragmentation
                                   of gluon jets in e+e-
                                   collisions




                                 Vitev & Gyulassy nucl-th/0104066


Can explain by combination of
hydro expansion at low pT with
jet quenching at high pT
Jet Quenching – Gyulassy, Wang, Vitev, Levai
                                            Degree of difficulty = 5

  HIJING: Beam jets @ pt<2 GeV (LUND), pQCD mini
   jets @ pt>2 GeV (PYTHIA), geometry (Glauber), 1D
   expansion, conservation laws; tuned to pp data 10-103 GeV
  + nuclear shadowing and parton energy loss “knobs”

 GLV “Thin” Plasma Limit

  L/ lg Opacity Expansion
                                                   No Shadow,
                                                    No Quench
                                                    No Shadow,
                                                 dEg/dx=0.5 GeV/fm
BDMS “Thick” Plasma Limit
                                                  Default: Shadow,
                                                     dEg/dx=2.0
                                   Nbinary
                                                                  ? 2003 ?

                                     PHENIX 130

BRAHMS
                                         hch
                                         STAR 130
PRL88(02)



                          Npart/2


15% too many particles, baryons over-quenched, but predicted the suppression
BUT: dE/dx =2 GeV/fm or 0.5 GeV/fm or not linear with x?
                        Vitev: they can get v2 right


• There is a quantitative difference
   Calculations/fits with flat  v2 = const  .
   or continuously growing  v2  ln pT / m  .


Check against high-pT data (200 AGeV)

                                     b~7 fm                                        b=7 fm

                          Same for 0-50%            C. Adler et al. [STAR Collab.],
                                                    arXiv: nucl-ex/0206006

                                                  • The decrease with pT is now
                                                  supported by data
                                                  • For minimum bias this rate is
                                                  slightly slower
      K. Filimonov [STAR Collab.],
                                                    See: N.Borghini, P.Dinh, J-Y.Ollitrault,
      arXiv: nucl-ex/0210027                             Phys.Rev. C 64 (2001)
              Other penetrating probes

 Open Charm
 J/Y
 Dileptons




    Need (a lot) more statistics in the data
    But getting a first sniff of physics already
                          J/Y




     Energy/Momentum




Data consistent with:
Hadronic comover breakup (Ramona Vogt) w/o QGP
Limiting suppression via surface emission (C.Y. Wong)
Dissociation + thermal regeneration (R. Rapp)
Open charm - Lin

                     about x2 within
                     predicted curves
                     with or w/o
                     energy loss

                   no x4 suppression
                   from peripheral to
                   central,
                   as predicted for
                   dE/dx=-0.5GeV/fm

                   But -
                   Is 40-70% peripheral
                   enough? error bars
                   still big!
    Some old things and some new things

 HBT
 High pT baryons
 Dijets vs. monojets
   Well, there was a prediction but for 10x the pT
 Parton saturation
HBT – lots of questions
                          Panitkin, Pratt


             • How to increase R
             without increasing
             Rout/Rside?
                  EOS, initial T and r
                 profiles (Csőrgó),
                 emissivity?

             • Why entropy looks low?
                Low entropy implies
                equilibrated QGP ruled
                out
                      Baryons at high pT      Jia, Sorenson




                               protons

                                p0, h

Yields scale with Ncoll near
pT = 2 – 3 GeV/c
Then start to fall
Meaning of Ncoll scaling?
Accident? Complex hard/soft interplay?
Medium modified jet fragmentation function?
            Away-side Jet Suppression
                                                  D. Hardtke

 trigger-jet
   not much
   modification
    (the trigger
   particles
   from jets!)

 Away side:
   strong jet
   suppression
       Strong jet suppression  surface emission of jets?
       Color glass back-to-back jets simply not created…
                 Parton saturation
                         Dima Kharzeev, Jamal Jalilian-Marian

 Hadron multiplicities imply a coherent initial state
   Initial NN interactions are NOT independent!
   High parton density  weak coupling  CGC
 Saturation at y=0, and even more so at forward y
     affects QCD evolution, even at Q2 > Qs2
     causes multiplicity to scale with Npart, even at high pT
     hard parton scattering suppressed by CGC 
     monojets
 does saturation set in already at s ~ 20GeV? I doubt this!
 Should measure in forward y in p+A, where Qs is larger
  and CGC is magnified.
     This should clarify initial vs. final state effect in AA!
                       conclusions

 Have early pressure buildup – high dNg/dy & they scatter!
    success of hydro, need for string melting, large s…
 High pT, high mass data look like pQCD + something
   Jet quenching works; surface emission??
   Baryon flow is a nuclear effect!
   Color glass is intriguing, but where does the collectivity
     come from?
 Event generators (still) a valuable tool to investigate
  sensitivity of observables to physics ingredients
 Integrated quantities are simple (conservation laws!)
    Caution in interpreting scaling with Npart or Ncoll

    e+e- scaling with Npart is arbitrary, agreement irrelevant

Experiments: homework to allow quantitative comparisons
  (multiple 15% factors = sloppy interpretations!)
                And the winners are…

 Best predictions of general features by event generator
   AMPT (Ko, Lin, Zhang)

 Novel approach, theoretically intriguing (+ agrees with data)
   Baryon junctions (Kharzeev, Vance, Gyulassy, Wang)

 Important prediction with potential great insights to QGP
   Hydrodynamics (Heinz & Kolb, Teaney & Shuryak, Bass &
    Dumitru, Ollitrault for “inventing” v2 analysis)

 Much promise for understanding properties of QGP
   Jet energy loss (Gyulassy,Wang, Vitev, Levai)
          yield in AuAu vs. p-p collisions
                                                  D. d’Enterria

                                  Yieldcentral/  N binary  central
Yield ratio s=200/130 GeV
Consistent at at high pT with                Yieldpp
pQCD predictions (STAR)


          PHENIX Preliminary




  70-80% Peripheral
  Ncoll =12.3 ±4.0
                       kT dependence of R
                                             Centrality is in top 30%




•Broad <kT> range : 0.2 - 1.2 GeV/c
•All R parameters decrease as a function of kT
             consistent with collective expansion picture.
• Stronger kT dependent in Rlong have been observed.
                                                 kT : average momentum of pair
Comparison of kaon to pion
                       In the most 30% central
        Comparison with hydrodynamic model
                                           Centrality is in top 30%

Recent hydrodynamic calculation
by U.Heinz and P. F. Kolb
(hep-ph/0204061)

           Hydro w/o FS
• Standard initialization and freeze out
which reproduce single particle spectra.

         Hydro at ecrit
• Assuming freeze out directly at the
hadronization point. (edec = ecrit)


kT dependence of Rlong indicates the
early freeze-out?
        kT dependence of Rout/Rside
                                         A. Enikizono
                                           QM2002




C.M. Kuo, QM2002 poster (PHOBOS) 200 GeV:
     1.16  0.09  0.25( syst .) @0.25 GeV/c
HBT PUZZLE
             Small Rout implies small Dt

                                                   P.Kolb




                                 Small Rbeam implies
Large Rside implies large R      small breakup t,~10 fm/c
Jet Evidence in Azimuthal Correlations at RHIC


 near-side correlation of           also seen in g (p0) triggered
  charged tracks (STAR)                events (PHENIX)
   trigger particle pT = 4-6            trigger particle pT > 2.5
   GeV/c                                GeV/c
                                         Df distribution for pT = 2-4
    Df distribution for summary slide (Peitzmann)
              QM2002 pT > 2
   GeV/c                                GeV/c
 signature of jets                




                                                  M. Chiu, PHENIX Parallel Saturday
     Identifying Jets - Angular Correlations

 Remove soft background
   by subtraction of mixed event distribution

 Fit remainder:                                  raw differential yields
   Jet correlation in Df;             PHENIX Preliminary 2-4 GeV
     shape taken from
     PYTHIA
   Additional v2 component
      to correct flow effects
Verify PYTHIA using p+p collisions

       Df(neutral E>2.5 GeV + 1-2 GeV/c charged partner)

             Make cuts in Dh to enhance
             near or far-side correlations
             Blue = PYTHIA
          |Dh|<.35                         |Dh|>.35
    In Au+Au collisions
                                              Df(neutral E>2.5 GeV + charged partner)

1-2 GeV partner
                                   Correlation after mixed event background
                                          subtraction
                                   Clear jet signal in Au + Au
                                   Different away side effect than in p+p

                                      |Dh|<.35                            |Dh|>.35
                  1/Ntrig dN/dDf




                                                         1/Ntrig dN/dDf
                  jets or flow correlations? fit pythia + 2v2vjcos(2f)

                  partner = .3-.6 GeV   .6-1.0 GeV/c   1-2 GeV/c   2-4 GeV/c
1/Ntrig dN/dDf




                                                                               Df
v2vj




                                                               Jet strength
                 See non-zero jet strength as partner pT increases!
How do protons scale with Ncoll/Npart?




                         Scale with Ncoll (unlike p)?!
            High pT baryons scale with Ncoll!
                                                    J. Velkovska


                                Low pT near Npart scaling




But baryons with pT > 2 GeV/c
behave very differently!
From jets? Unsuppressed??
Charm cross section at RHIC
Centrality dependence of charm
      Homework assignment (PHENIX & STAR)

   Yieldcentral/  N binary  central
Yieldperipheral /  N binary  peripheral

  Charged larger than p0
  But difference not same
    as for RAA
  PHENIX and STAR RAA
    not the same
  Different reference in
    each case!
  Systematic difference
    between experiments
                      Charged hadron correlations - small Df

                          pT
                                jT   Correlation width  jT/pT
Correlation width




                    •Fit charged correlations with v2 + Gaussian (fixed pT)
                    •Jet signal visible via s
                           Width of near-side Gaussian decreases with pT
                           No significant centrality dependence on near-side
               How do high pT yields scale?
 vs. binary collisions:
   continuous decrease as
      function of centrality
   factor ~ 3.5 from
      peripheral to central
 vs. participants:
   first increase, then
      decrease as function of
      centrality
   for Npart > 100 have 3s
      change (scaling or no?)
   surface emission?
   re-interactions?
   accident?
18% scaling uncertainty from corrections
                                                   dN/dy

dN/dy / (0.5 Npart)        PHENIX Preliminary                  PHENIX Preliminary

                      Au+Au at sqrt(sNN) =200GeV           Au+Au at sqrt(sNN) =200GeV


                                             p+                                   p+

                                              K+                                    K-


                                              p
                      open symbol :                                            pbar
                      130 GeV data
                      Positive                             Negative

                                              Npart                                 Npart
      • Similar centrality dependence 130 GeV and 200 GeV
        Opaque, expanding source would mean:

  R - R = b ( Dt ) + ( X - Y ) - 2 b s
    2
    o
            2
            s
                    2
                    
                              2          2        2                     2
                                                                        xt
                                        Opaque              Expanding

                                  Y (side)

                          X (out) 

                                                 Rs( half -shell )   5
Rischke RIKEN workshop (2002):                        ( sphere)
                                                                   =   = 1.29
                                                  Rs                 3
Such strong xt correlations probably
require a lack of boost-invariance...        Ro half -shell )
                                              (
                                                                 5
                                                 ( sphere)
                                                              =    = 0.65
                                              Ro                12
                     Energy Dependence

                            Assumptions:
PHENIX preliminary
                               in Lab             in C.M.
                               dX dX             dX       dX
                                                    1.2
                               dy dh             dy       dh

                            Energy density (Bjorken):
                                 1 dEt         R = 1.18 fm  A1/ 3
                              = 2
                                pR t dy       t = 1 fm / c
PHENIX preliminary
                               2% most central at sNN=200 GeV:
                                 5.5 GeV/fm3

                            From AGS, SPS to RHIC:
                               Transverse energy and charged particle
                               multiplicity densities per participant
                               consistent with logarithmic behaviour
p,K,P spectra from Star
                 High quality data over
                   9 centrality selections
                 Shape described by
                blast wave fit
          K-/K+ and p/p from AGS to RHIC
I. Bearden (BRAHMS)

Becattini caluclation using
statistical model:
T=170, gs=1 (weak dependency)
vary mB/T  K+/K- andp/p

K- /K+=(p/p)1/4 is
a empirical fit to the data points

K-/K+ driven by ms
~ exp(2ms/T)

p/p driven by mB
~ exp(-2mB/T)

ms = ms (mB) since <S> = 0
                                        QM2002 summary slide (Ullrich)
                  BUT: Holds for y  0 (BRAHMS y=3)
                             The K*0 story




                                    STAR Preliminary
   K*0/Ksuppressed in AA versus pp
 f/K*0 appears enhanced versus pp

pp  uncorrected for trigger bias
and vertex finding efficiency




                                    STAR QM Talks: E. Yamamoto and P. Fachini
                  v2 at high pT

min bias 200 GeV Au+ Au
             Centrality dependence of p/pi

•Ratios reach ~1 for
central collisions                           +
•Peripheral collisions
lower, but still above gluon
jet ratios at high pT

•Maybe not so surprising
1)“peripheral” means 60-
91.4% of stotal                              -
2) p/pi = 0.3 at ISR
Note pbar/p behavior

           Centrality dependence only
           for pT > 3 GeV/c

           Peripheral collisions have
           quite a few protons at mid-y

						
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