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Direct photon measurement in heavy ion collisions

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Title: Direct photon measurement in heavy ion collisions


1
Direct photon measurement in heavy ion collisions
  • Takao Sakaguchi
  • Brookhaven National Laboratory

2
Outline
  • Direct photons and their origins
  • History of direct photon measurements in high
    energy nucleon and heavy ion collisions
  • Latest photon data from RHIC
  • Current landscape of photon production
  • Future exploration of heavy ion collisions using
    direct photons

I apologize in advance that Im heavily biased by
PHENIX
3
Direct shine
4
Direct photon basics
  • Emitted at all stages then surviving unscathed
    strongly (a ltlt as, almost transparent to medium)
  • Production Process
  • Compton and annihilation (LO, direct)
  • Fragmentation (NLO)
  • Often carry thermodynamical information of the
    state
  • Temperature, Degrees of freedom

Small Rate Yield ? aas
Gordon and Vogelsang, PRD48, 3136 (1993)
5
Direct photon production in pp collisions
  • Started back in 1979-1982 at SPS. R806,
    R110(?sNN63GeV), WA70 (?sNN24GeV). Later, UA2,
    UA6 reached at ?sNN630GeV

R110, ?sNN63GeV, pp collisions.
dir. g/p0 ratio
Invariant cross-section
CMOR, NPB 327(1989)541
A compilation Vogelsang and Whalley, J. Phys.
G23 (1997)A1
6
Continued at CDF, and..
  • ppbar ?sNN1.8TeV. Prompt (isolated) photons had
    been measured
  • Data from many experiments are compiled and
    compared with pQCD

Aurenche et al., PRD73, 094007(2007)
D0, PRL77, 5011 (1996)
7
State-of-art at 200GeV
  • Extended up to 25GeV/c
  • Systematic error 20
  • Baseline for RHIC heavy ion results

8
Even fragment/prompt components are decomposed
  • Two Methods in pp 200GeV
  • Fraction of isolated/all photons, which is
    calculable from NLO pQCD. Isolation cut ( 0.1E?
    gt Econe(R0.5) )
  • Looking at angular correlation between leading
    hadrons and photons

g(Isolated)/g(all direct)
PHENIX, PRL98, 012002 (2007)
PHENIX, J. Phys. G35 (2008)104121
9
Direct photon production in heavy ion collisions
  • Purpose is to look for thermal radiation from
    possibly produced hot and dense matter in
    collisions
  • Measurements in heavy ion collisions
  • HELIOS (Z. Phys. C46(1009)369), CERES (Z. Phys.
    C71(1996)571), null result..
  • WA80, WA98 at CERN
  • PHENIX and STAR at RHIC
  • Measurements complementing heavy ion data
  • Many pp reference data
  • Some pA data (E706 produced nice results)
  • PHENIX at RHIC

10
Landscape before RHIC begins
11
Only processes admitted until 2001
  • pQCD
  • Thermal radiation from QGP (1ltpTlt3GeV)
  • S/B is 10
  • Spectrum is exponential. One can extract
    temperature, dof, etc..
  • Hadron-gas interaction (pTlt1GeV/c) ??(?) ?
    ??(?), ?K ? K?

Also, many seminal works by Sinha, Alam, Nayak,
Srivastava, Fries, Rapp et al.
A compilation on photons, PRC 69(2004)014903
12
WA80 results
  • SAu at 200GeV/u
  • ?sNN20GeV
  • g/p0 observed is compared to the one estimated
    from hadronic background calculation
  • Onset for pTgt2.5GeV/c?
  • Systematic Error 5!
  • Most interesting part is hidden by statistics

WA80, PRL76, 3506(1996)
13
WA98 results
  • A dedicated experiments for direct photon search
    in relativistic heavy Ion collisions. (PRL 85
    (2000) 3595)
  • ?sNN17.3GeV
  • Data can be either explained by kT-smearing or
    higher initial temperature
  • Any data did not see pTgt4GeV, where pQCD photons
    dominate
  • No information on kT does not allow us to resolve
    the issue.

WA98, J. Phys. G35 (2008)104123
WA98 data and theoretical interpretation PRC69(20
04)014903
14
Then, RHIC changed the landscape..
15
Large suppression of high pT hadrons
  • A big discovery from RHIC Year-1
  • Energy loss of partons in medium
  • RAA now extended to 20GeV/c
  • Integrated RAA proved that the energy loss is
    consistent with fractional (increases with pT)

PHENIX, PRL, in press
16
Another big discovery
  • Suppression of ?0 and ? reduced background, and
    highlighted direct photons
  • Ratio increases as centrality increases
  • Hard photons, whose yield is well explained by
    NLO pQCD
  • Initial state condition is understood.
  • NO direct photon suppression (initial state), and
    large ?0 suppression (final state)

?measured / ?background
Nuclear Modification factor
Direct photons
?0
g/p0measured / g/p0background
gmeasured/gbackground
S.S.Adler, et. al. (PHENIX Collaboration), PRL
94, 232301(2005)
17
Highlights from high pT hadron results
  • Run1, Run2, Run4 AuAu high pT p0
  • Run2 AuAu 200GeV high pT direct photons
  • Run3 pp 200GeV high pT direct photons
  • Run5 pp high pT p0 200GeV
  • Run5 CuCu 22, 62 and 200GeV high pT p0

PRC75, 024909(2008) preliminary QM05
18
E-loss of partons did job on photons?
19
Yes, new production mechanism has been introduced
  • Compton scattering of hard scattered and thermal
    partons (Jet-photon conversion)
  • A recent calculation predicted yields for
    radiative and collisional E-loss case
  • This itself probes the matter on similar way as
    jets do.
  • Bremsstrahlung from hard scattered partons in
    medium

Both are thermally
Turbide et al., PRC72, 014906 (2005) R. Fries et
al., PRC72, 041902 (2005) Turbide et al.,
arXiv0712.0732 Liu et al., arXiv0712.3619, etc..
20
New contents..
  • Energy loss of high pT hadrons will reduce
    background
  • S/B increases. Effectively Signal is enhanced
  • Photon produced in fragmentation of quarks and
    gluons will also be reduced
  • Signal reduced
  • Photons produced in the interaction of
    quarks/gluons with medium
  • Same process as initial hard scattering, but the
    target is medium
  • Signal increased
  • Summary sheet tells everything is balanced?

21
Discovery of new source? 200GeV AuAu
  • Remember the extended highlight plots from
    PHENIX
  • Consistent with old published result up to
    12GeV/c
  • Direct photons suppressed at very high pT?
  • A theory F. Arleo (JHEP 0609 (2006) 015)
  • Isospin effect, in addition to jet-quenching(BDMPS
    ) and shadowing.

22
Something we have missed before..
  • Taking for example, the isospin effect Direct
    photon cross-sections for
  • pp, pn and nn are different because of
    different charge contents (? ? ?eq2)
  • Effect can be estimated from NLO pQCD calclation
    of pp, pn and nn
  • In low pT, quarks are from gluon split ? no
    difference between n and p
  • At high pT, contribution of constituent quarks
    manifests
  • Minimum bias AuAu can be calculated by

(sAA/Ncoll)/spp vs pT
(sAA/Ncoll)/spp vs xT
Same suppression will be seen in lower pT at
?sNN62.4GeV
TS, INPC07, arXiv.org0708.4265
23
A test 62GeV AuAu direct photons
  • Looks like there is an isospin effect (and/or PDF
    effect)
  • Question pp is a right reference to take?
  • Isospin effect is electric charge dependent,
    which affects to photons ?0 is color charge
    dependent
  • Therefore, e-loss models so far are still valid

18GeV/c_at_200GeV
24
Landscape expanded richly after RHIC
(fm/c)
25
Theory also become rich..
  • I personally have not seen such a drastic
    progress of theoretical works like now.

Vitev and Zhang, PLB669(2008)337
Liu et al., arXiv0811.0666
C. Gale, NPA774(2006)335
26
Direct photon v2 a photon source detector
  • Depending the process of photon production,
    angular distributions
  • of direct photons vary
  • Jet fragmentation (v2gt0), Jet-photon conversion,
    in-medium bremsstrahlung (v2lt0), Turbide, et al.,
    PRL96, 032303(2006), etc..
  • Thermal photon v2 Quark v2 (gt0), (based on
    hydro calculation)
  • Chatterjee, et al., PRL 96, 202302(2006),
    Kopeliovich et al., arXiv0712.2829, etc..

Turbide et al., arXiv0712.0732
27
Direct photon v2 in AuAu collisions
  • Hadron decay photon subtracted from inclusive
    photon v2.
  • Reached up to 8GeV/c, no significance for
    pTlt3GeV/c
  • Tends to be positive?
  • Uncertainty of gmeas/gbkgd dominates error here.
  • It is not due to v2 measurement of inclusive
    photons or ?0
  • Could be improved by internal conversion method?

20-40 result is similar.
FYI, WA98 Result, EPCJ41(2005)287, no significance
28
Be frontier to a new degree of freedom
29
g measurement from RHIC
  • pT spectra as a function of invariant mass
  • Known hadron decay components (cocktail) in lines
  • Caveat cocktail calculation here does not
    include contribution from internal conversion of
    direct photons

2 single exponential fits Low-pT 0ltmTlt1
GeV High-pT 1ltmTlt2 GeV
30
Landscape after merging with Dileptons
hard scatt isospin effect
Cartoon only sources of g, mean pT vs time
(dashed hadrons)
pT
(GeV/c)
jet Brems.
jet-thermal
jet fragmentation
sQGP
hadron gas
hadron decays
qg -gt qg meets qqbar -gtg
log t
Mass (GeV/c2)
1
10
107
1
(fm/c)
Conventional dilepton contribution becomes
smaller in low mass and high pT
2
31
Low pT photons at RHIC
  • PHENIX applied internal conversion technique
  • Real photons can convert to virtual photons
  • Inv. mass shapes for Dalitz decay of mesons are
    calculable using Kroll-Wada formula
  • If MltltpT, the ratio of observed inv. mass to
    expected is proportional to direct photon excess
    ratio
  • Take ratio where p0 contribution is small ? S/B
    increases

32
Thermal Photons?
  • The result came out.

Fit results Cent. dN/dy(pTgt1GeV/c) T(MeV)
?2/DOF 0-20 1.10?0.20?0.30 221?23?18
3.6/4 20-40 0.52?0.08?0.14 215?20?15
5.2/3 MB 0.33?0.04 ?0.09 224?16?19
0.9/4
PHENIX, arXiv0804.4168
33
Where do we go?
34
Something we may have missed..
  • Initial multiple scattering effect should exist?
  • ? kT broadening, p0 kT broadening
    recombination.
  • Detail study of pA or dA should help
  • RHIC Run-8 dAu collision data are coming

PHENIX, dAu, RAA
STAR, dAu, gmeas/gbkgd
Russcher (STAR), QM06
Peressounko (PHENIX), QM06
35
g-Jet correlation
  • Subtract p0-h, h-h from (incl g)-h
  • If the result is true, the jet-emission is not
    always tangential.
  • ? is not necessarily the direct. Fragment,
    bremsstrahlung, Jet-conversion photons could
    significantly contribute
  • similar to h-h correlation? Isolation of direct
    photons would be needed
  • Ridge structure, same RAA and IAA
  • Red points integrated RAA from single p0
    measurement (pTgt5GeV/c)
  • Blue points Same (integrated away side yield
    IAA) from g-h measurement (Assoc. pTgt5GeV/c)

Df
36
Direct photons in LHC era?
  • Hard scattering cross-section even goes higher
  • ?-Jet correlation analysis is the primary target
  • Key issue of the analysis is how clean tagged
    photon samples can be

Input and Reconstructed fragmentation function
from direct photon tagged events (0-10 PbPb)
Discrimination power of photons to hadrons
Morsch (ALICE), QM08
Loizides (CMS), QM08
37
What do we expect at LHC?
  • A calculation tells that even in low pT
    region(pT2GeV/c), jet-photon conversion
    significantly contributes to total
  • What do we expect naively?
  • Jet-Photon conversions ? Ncoll ? Npart ? (s1/2)8
    ? f(xT), 8 is xT-scaling power
  • Thermal Photons ? Npart ? (equilibrium duration)
    ? (s1/2)1/4 2
  • LHC would see huge Jet-photon conversion
    contribution over thermal.
  • Together with v2 measurement, the thermal
    region would be a new probe of medium response
    to partons

Turbide et al., arXiv0712.0732
38
More future interest
  • Determining Time evolution scenario by looking at
    forward direct photons
  • Landau expansion will make one order reduction
    at pT4GeV/c at y2 compared to y0
  • Nose-cone calorimeter upgrade in PHENIX (Covering
    1ltylt3)
  • Forward Photon Detector in STAR (Covering
    -3.7ltylt-2.3)

39
Summary
  • Direct photons become indispensable probe for
    characterizing matter
  • Starting from 1979, they have been a probe of the
    initial condition the h-h and heavy-heavy
    collisions.
  • RHIC has developed many new sources of direct
    photons
  • Jet interacting with medium produces photons, and
    would be a useful tool for parton E-loss
    mechanism study
  • The process will be much useful in LHC era.
  • Isospin effect may have been observed in AuAu.
  • low pT photon emission suggests a thermalized
    state.
  • Photon production at high rapidity would help
    determining the system expansion scenario
  • And.

40
This is the place to live!
Thank you!
41
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