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System size dependence

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Title: System size dependence


1
System size dependence
  • Comments on...
  • pp and pA collisions
  • AA with different size
  • Karel afarík, CERN
  • http//home.cern.ch/karel/fr.ppt
  • Karel.Safarik_at_cern.ch

2
Outlook (1/2)
  • Enhancement in pp and pA collisions
  • strangeness enhancement in hh collisions
  • pA data from 80s
  • do we have some knowledge ?
  • pp versus pA enhancement
  • trivial reason - isospin (pp and pn)
  • re-scattering
  • recent results
  • do we contradict to previous experiments ?
  • System size dependence for AA
  • different centrality measures

3
Outlook (2/2)
  • Multi-strange particle enhancement
  • Compatibility of strangeness data among SPS
    experiments
  • ? production in WA97 and NA49
  • Microscopic model explanations
  • prediction from QGP
  • ropes, droplets
  • string models final state re-scattering
  • multi-particle (de-)nihilation
  • Conclusions

4
Strangeness in hh
  • Data on K/p in hadron-hadron interactions show
    steady (slow) increase with energy
  • with multiplicity
  • (CERN SppS and FNAL Tevatron)
  • Possible explanations
  • experimental bias, due to high pt cut-off
  • increasing role of gluons for particle
    production
  • It is a physical effect
  • does this mean deconfinement ?

5
pA data from 80s
  • pA collisions (at that time high energies) were
    extensively studied at the beginning of 80s
  • predictions for nuclear densities that may be
    achieved in head-on collisions of large nuclei
  • A.S.Goldhaber, Nature 275 (1978) 114
  • among other also strange particle yields was
    measured
  • P.Skubic et al., Phys.Rev. D18 (1978) 3115
  • D.Antreasyan et al., Phys.Rev. D19 (1979) 764
  • D.S.Barton et al., Phys.Rev. D27 (1983) 2580
  • M.G.Abreu et al., Z.Phys. C25 (1984) 115
  • W.Busza, R.Ledoux, Ann.Rev.Nucl.Part.Sci. 38
    (1988) 119
  • D.H.Bricket al., Phys.Rev. D39 (1989) 2484, 45
    (1992) 734
  • C.De Marzo et al., Phys.Rev. D26 (1982) 1019
  • I.Derado et al., Z.Phys. C50 (1991) 31 ...

6
Centrality measures
  • In pA
  • usually
  • n A shp / shA (? A1/3)
  • assumes that incident nucleon has constant
    x-section during re-scattering
  • or just A
  • In AA
  • number of wounded nucleons (Nw n 1)
  • number of participants Np
  • sometimes identical with Nw
  • sometimes includes nucleons kicked-out in
    secondary re-scattering

7
A-dependence (1/3)
  • pion production in central region in pp and pA

8
A-dependence (2/3)
  • kaon production in central region in pp and pA

9
A-dependence (3/3)
  • K/p ratio in central region in pp and pA

10
4p data
  • Much lower statistics
  • bubble chamber or streamer chamber
  • Gray particle identification (slow protons np)
  • number of interaction np ???np event-by-event
  • total number of re-scattering nt from net charge
  • number of secondary interaction ns nt - np
  • pA 200 GeV/c (D.H.Brick et al.)
  • L large (factor 2) increase compare to pp
  • yield proportional to np and ns
  • K0 smaller increase, saturation with np and ns
  • conclusion L excess due to secondary
    re-scattering in target

11
4p data
  • pA data at 200 GeV/c (C.De Marzo et al.)
  • rapidity distribution RA(y) (dN/dy)hA /
    (dN/dy)hp
  • excess in target fragmentation region
  • plateau between 2 - 4 in y
  • above goes down, even below 1
  • RA in central region increases with A slower than
    nA
  • RXe/RAr 1.21 nXe/nAr 1.40 same for
    charged, negative, similar for L and K0 (small
    statistics)
  • energy attenuation
  • Conclusion no increase in projectile region

12
pA versus pp
  • all experiments found consistently an increase in
    yield of any secondaries between pp and
    back-extrapolation from pA
  • this enhancement sets already at first measured
    nuclei (usually C but is there already for Be !)
  • conclusions (from D.S.Barton et al.)
  • the A dependence of the inclusive cross-sections
    in projectile fragmentation region exhibits a
    remarkable simplicity
  • the A dependence is an universal, independent of
    the outgoing particle, its transverse momentum,
    and the incident energy

13
pA versus pp
  • Ratio (strange) / (non-strange) in pA collisions
    independent on A
  • however different (higher) than in pp

14
pp vs. pA enhancement
  • trivial reason - difference in pp and pn
    collisions
  • there is a difference in isospin which can affect
    yields
  • an exercise (just for fun)
  • PYTHIA pn versus pp at 100 GeV increses
  • ? 1
  • anti ? 2
  • ? 28
  • anti ? 14
  • second reason - re-scattering
  • increases yield of all produced particles again
    in different way and mostly in target
    fragmentation

15
Recent pA data (1/3)
16
Recent pA data (2/3)
  • K/p ratio in forward hemisphere as a function of
    centrality in pPb
  • increase for K/p by about 50
  • K-/p- independent on centrality (and anti-p/p-
    also)
  • Why is this ?
  • pA at definite centrality is something
    completely different than minimum bias pA for
    various A
  • trigger bias ?
  • pA centrality triggered by gray particles

17
Recent pA data (3/3)
  • K/p for central pPb as a function of xF (!?)
  • an increase up to a factor ?3 compare to pp data
    !
  • Comments
  • part of such increase is trivial
  • pp is not the same as pA
  • if K and p have the same momenta (xF)
  • p has substantially larger rapidity (velocity)
  • for large number of collisions n particle yields
    at high rapidities are suppressed
  • K is still not at high rapidity
  • this seems more as p suppression than K
    enhancement
  • data on K and p separately are needed !

18
Strangeness PbPb data
  • Data from SPS Pb-beam era (1996-) on strangeness
    are in unprecedented agreement
  • K yields from
  • NA44 (charged)
  • NA49 (charged and neutral)
  • WA97 (neutral)
  • in central region for central PbPb collisions
    agree within one standard deviation !
  • ? from WA97 and NA49 as well

19
Strangeness PbPb data
  • Centrality dependence of K yields
  • apparent disagreement between NA49 and WA97
  • two main differences
  • 4p (NA49) versus central (WA97) yields
  • small effect (about 7 for most central
    collisions)
  • definition of Npart
  • number of nucleons participating in initial
    collisions among themselves (WA97)
  • include on top of that also knocked-out nucleons
    (NA49)
  • at both ends of the scale the two definitions
    coincides but in the middle Npart WA97 lt Npart
    NA49
  • affects both axes vertical and horizontal

20
K centrality dependence
  • now clarified

21
K/? centrality dependence (1/2)
22
Collision geometry (1/2)
  • Pb - Pb 60 participants (NA57 class 0)

23
Collision geometry (2/2)
  • S - S 60 participants

24
Small vs. large system
  • What is the good centrality measure
  • Few proposals
  • transverse density Npart / (transverse overlap)
    (Nardi)
  • doesnt work too well
  • longitudinal thickness R - b/2 (volume to
    surface ratio, NA49)
  • works surprisingly well
  • density of produced particles vs. energy density
    (S.Kabana)
  • it works, but large uncertainties ...

25
K/? centrality dependence (2/2)
26
Particle vs. energy density
27
Multi-strangeness data
  • Agreement between WA97 and NA49 results
    concerning ? production in pA and AA collisions
  • WA97 published data for minimum bias pBe and for
    minimum bias pPb interactions
  • NA49 presented data for pp and for pPb with two
    different centralities
  • mean number of collisions are ? 3.7 (which
    approx. corresponds to minimum bias pPb) and 5.7
  • yields at first pPb point for ?, ?, ?, ? agree
    well with WA97 data
  • NA49 pp yields significantly below expectations
    from pA - strangeness enhancement in pA ?
  • However, pp yields for any particle are well
    below extrapolation from pA ...

28
Multi-strangeness data
  • WA97 versus NA49 cascades

29
Multi-strangeness data
  • WA97 versus NA49 anti-cascades

30
W enhancement
  • W plus anti-W enhanced more than a factor 15

31
Multi-strange enhancement
  • Strange particle yields in central PbPb
    collisions can be described in statistical
    approach
  • large W enhancement achieved (apart of adjustment
    of thermodynamical variables) mainly due to
    enlargement of volume (phase space)
  • canonical vs. grand-canonical ensemble
  • this needs on microscopical level a very fast
    communication across large volume
  • Naturally explained in deconfined phase
    (sometimes called QGP) where a movement of
    communicators with sufficient cross-section is
    allowed across large volume

32
Microscopic models
  • String models
  • A.Capella, C.A.Salgado, S.Vance, M.Gyulassy
  • string rearrangement
  • stopping effectively baryon junction
  • sea diquark-antidiquark strings

33
Microscopic models
  • This effectively increase production of strange
    and multi-strange (anti-)baryons
  • by factor about 2 - 3 for W and anti-W
  • In order to go further binary final state
    interaction are used
  • this eventually have to lead chemical equilibrium
    and hence agreement with the data
  • but, the cross section
  • (A.C, C.A.S) use for velocitycross-section a
    mean value between 0.14 and 0.20 mb, this gives
    for the equilibration time of the order of 100 fm
    !
  • (C.M.Ko) use for strangeness exchange reaction ?
    5 mb which will give something like 30 fm
    equilibration time
  • Anyway, most of the Ws are produced in
    re-interaction
  • therefore they have to participate in radial flow
    !

34
Microscopic models
  • Antibaryon (de-)nihilation (inverse of
    annihilation)
  • C.Greiner, S.Leupold, W.Cassing
  • now we have a huge cross-section, of about 50 mb
  • this leads to short equilibration time ? 3 fm
  • this can work, however
  • asymmetry between baryons and anti-baryons
  • we start with high baryon (p and n) density
  • then using detail balance we get large rate for
    anti-hyperons
  • this argument does not work for hyperons
  • in other words anti-W is produced via
  • np 3K ? anti-W p
  • transverse momentum spectra (detailed simulation)
  • two-body (de-)nihilation (pp?WW) has threshold
    3.1 GeV !

35
Conclusions
  • Strangeness increases with energy and
    multiplicity in hh collisions
  • Enhancement between pp and extrapolation from pA
    data has been observed for different particle
  • However, particle ratios within pA data stays
    constant
  • Data for pA at 200 GeV/c do not show projectile
    enhancement
  • Possible difference in pp and pn and
    re-scattering in target region

36
Conclusions
  • NA49 data on K/p ratio show strangeness
    enhancement in pA collisions for positive charge
  • Is there contradiction to other experiments from
    80s ?
  • Needs experimental investigation
  • Different centrality behavior for different size
    systems
  • few attempts to redefine axis, best works R -b/2
    (NA49)
  • Agreement in pA data for X production between
    NA49 and WA97

37
Conclusion (cont.)
  • Multi-strange particles enhanced up to factor of
    about 15 in central PbPb collisions
  • one gets yields in agreement with statistical
    (maximum entropy) description
  • for that we probably need fast communication
  • naturally obtained in deconfined medium
  • obtained in models which itroduced something like
    deconfined medium (ropes, droplets)
  • string models (without final state) gives for W
    enhancement by factor of 3
  • one reasonably gets to the equilibrium yields for
    anti-W by anti-baryon (de-)nihilation (but W)

38
Strangeness PbPb data
  • the only unresolved issue is ?-meson data
  • NA49 measures ? ? KK decay mode
  • NA50 measures ? ? ?? decay mode (smaller
    acceptance)
  • yield at midrapidity dN/dyNA49 lt dN/dyNA50
    (factor gt 2)
  • speculation about differences in KK and ??
    channels
  • mT slopes TNA49 (300 MeV) gt TNA50 (220 MeV)
  • the width of rapidity distribution substantially
    larger in Pb-Pb than in pp (why ?)
  • S.Margetis, K.S., O.Villalobos Baillie, Ann.Rev.
    Nucl.Part.Sci. 50 (2000) 299
  • D.Röhrich, J.Phys. G 27 (2001) 355
  • K.S., J.Phys. G27 (2001) 579

39
Strangeness PbPb data
  • ?-meson (as well as W) has no resonance with p

?
40
Microscopic models
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