Title: Forward and p(d) A Physics at RHIC
1Forward and p(d)APhysics at RHIC
- Conveners
- Carl Gagliardi, Mike Leitch, Kirill Tuchin
- http//www.phenix.bnl.gov/phenix/WWW/publish/leitc
h/rhicii-forward/rhicii-forward.html
- Small-x physics and saturation
- Additional important measurements
2Mid-rapidity vs. forward rapidity
Mid Rapidity
Forward Rapidity
CTEQ6M
Gluon density cant grow forever. Saturation may
set in at forward rapidity when gluons start to
overlap.
3Nuclear Gluon Density
e.g., see M. Hirai, S. Kumano, T.-H. Nagai, Phys.
Rev. C70 (2004) 044905 and data references
therein
World data on nuclear DIS constrains nuclear
modifications to gluon density only for xgluon gt
0.02
4Gluon Shadowing and Saturation
- Leading twist gluon shadowing, e.g.
- Gerland, Frankfurt, Strikman,
- Stocker Greiner (hep-ph/9812322)
- phenomenological fit to DIS DY data, Eskola,
Kolhinen, Vogt hep-ph/0104124 - and many others
- Amount of gluon shadowing differs by up to a
factor of three between different models
- Saturation or Color Glass Condensate (CGC)
- At low x there are so many gluons, that the
quantum occupation numbers get so large that the
situation looks classical - Nuclear amplification xGA(x) A1/3xG(x),
i.e. gluon density is 6x higher in Gold than the
nucleon
Iancu and Venugopalan hep-ph/0303204
5Forward particle production in dAu collisions
BRAHMS, PRL 93, 242303
Sizable suppression in charged hadron production
in dAu collisions relative to pp collisions at
forward rapidity
6PHENIX and PHOBOS report similar effects
PRL 94, 082302
PRC 70, 061901(R)
Charged particles are suppressed in the forward
direction in dAu collsions
7? dependence of RdAu
Observe significant rapidity dependence, similar
to BRAHMS measurements and expectations from
saturation framework.
8Comparing dAu dN/d? to pemulsion
nucl-ex/0409021
PHOBOS attributes effects to limiting
fragmentation
9Heavy quarks at forward rapidity small-x
First forward rapidity prompt muon results (charm
beauty)
- J/? nuclear dependence does not scale with x2 so
appears to NOT have a dominant effect from
shadowing - PHENIX, nucl-ex/0507032
- Apparent scaling with xF is similar to limiting
fragmentation phenomena as reported by PHOBOS - but other models involving Sudakov suppression
(energy conservation) - Kopeliovich et al, hep-ph/0501260 (2005)
- or (large) initial-state gluon energy loss could
also explain this xF scaling
10Many recent descriptions of low-x suppression
A short list (probably incomplete)
Saturation (color glass condensate)
Shadowing
- R. Vogt, PRC 70 (2004) 064902.
- Guzey, Strikman, and Vogelsang, PLB 603 (2004)
173.
- Jalilian-Marian, NPA 748 (2005) 664.
- Kharzeev, Kovchegov, and Tuchin, PLB 599 (2004)
23 PRD 68 (2003) 094013. - Armesto, Salgado, and Wiedemann, PRL 94 (2005)
022002.
Parton recombination
- Hwa, Yang, and Fries, PRC 71 (2005) 024902.
Multiple scattering
- Qiu and Vitev, PRL 93 (2004) 262301
hep-ph/0410218.
Others?
Factorization breaking
- Kopeliovich, et al., hep-ph/0501260.
- Nikolaev and Schaefer, PRD 71 (2005) 014023.
11x values in saturation calculations
In CGC calculations, the BRAHMS kinematics
corresponds to ltxggt lt 0.001 (Dumitru,
Hayashigaki, and Jalilian-Marian, hep-ph/0506308)
12Is saturation really the explanation?
Difficult to explain BRAHMS results with standard
shadowing, but in NLO pQCD calculations ltxggt
0.02 is not that small (Guzey, Strikman, and
Vogelsang, PL B603, 173)
13Any difference between pp and dAu?
pp Di-jet
dAu Mono-jet?
Dilute parton system (deuteron)
PT is balanced by many gluons
Dense gluon field (Au)
Kharzeev, Levin, McLerran gives physics picture
(NPA748, 627)
Color glass condensate predicts that the
back-to-back correlation from pp should be
suppressed
14Back-to-back correlations with the color glass
The evolution between the jets makes the
correlations disappear.
(Kharzeev, Levin, and McLerran, NP A748, 627)
15Correlations in dAu
- are suppressed at small ltxFgt and ltpT,pgt
- Spp-SdAu (9.0 1.5)
- consistent with CGC picture
- are consistent in dAu and pp at larger ltxFgt
and ltpT,pgt - as expected by HIJING
STAR Preliminary
STAR Preliminary
25ltEplt35GeV
STAR Preliminary
STAR Preliminary
35ltEplt45GeV
Statistical errors only
16Saturation physics at RHIC?
- Fundamental question regarding saturation Where
does it set in? - Forward hadron production at RHIC samples similar
x values as mid-rapidity production at the LHC - Complex interplay at the LHC
- May need pp, pPb, and PbPb at the same vs to
unravel it fully
17CERN pNucleus Workshophttp//wwwth.cern.ch/pAatL
HC/pAworkshop2.html
- pA at the LHC is still officially an upgrade
- First year that LHC might run pPb 2010
- Possible target luminosity 1029 cm-2s-1
(RHIC II 20x larger) - Cant use the constant frequency solution that
worked well at RHIC - N-N center of mass not at rest in lab ?y 0.46
for full energy pPb - Company line no need for pp reference. Will
come from interpolation between Tevatron and 14
TeV - Probably okay for really hard processes
- May be problematic for measurements focused on
small-x saturation effects - If the accelerator turn-on goes well, even
getting the 14 TeV reference data may be a
challenge
18pp and dAu ? p0p0X correlations with forward
p0
hep-ex/0502040
pp in PYTHIA
dAu in HIJING
Conventional shadowing will change yield, but not
coincidence structure. Sensitive to xg few x
10-3 in pQCD scenario few x 10-4 in CGC scenario.
19Upgrades
- STAR
- Forward Meson Spectrometer
- Forward tracker upgrade (SiGEM)
- PHENIX
- Nosecone calorimeter (W-Si)
- forward muon trigger (RPC)
- Forward Silicon Vertex detector (mini-strips)
20Double parton correlations
CDF, PRL 79, 584
PRL 88, 031801
A-dependence of 4-jet yields in pA collisions
can be used to measure x1 x2 momentum
correlations within the proton. Would require pA
collisions.
21Tagged Drell-Yan production at RHIC? (from
Jen-Chieh Peng)
One can tag on forward-going proton, neutron, ?,
? in coincidence with lepton-pair
Assuming factorization, then dsDY/dy dm dxF
(pp?nµ µ- x) dsDY/dm dxF
(pp?µµ- x) fMB(y) and fMB(y) is the
probability for p ? p n, where n carries a
fraction y of the proton momentum
Tagged Drell-Yan production could provide
information on the antiquark distribution in the
mesons of the nucleon sea and on fMB(y)
22Tagged DY with forward neutrons
Or with tagged protons
(from Jen-Chieh Peng)
ZDC
Roman pots
23Physics with tagged forward protons at
RHIC-II from Wlodek Guryn
- processes with forward tagged protons select
exchanges mediated by gluon-rich objects - color-singlet objects with vacuum quantum
numbers Pomerons - double Pomeron exchange can produce massive
systems glueballs and other gluon-rich states
24Ultra-peripheral Collisions (UPCs)
- Can ultra-peripheral reactions (UPCs) at forward
rapidity probe small-x gluon shadowing or
saturation? - e.g. J/? production probes gluon distributions
of nuclei (private comm. Mark Strikman)
QM05
25Conclusions
- dAu results provide hints that saturation
effects are becoming important - Both STAR and PHENIX have upgrade plans that will
dramatically improve their forward capabilities - RHIC may be the ideal accelerator to explore the
onset of saturation
26(No Transcript)
27One calculation within the saturation picture
RdAu
RCP
Saturation model calculation with additional
valence quark contribution (Kharzeev, Kovchegov,
and Tuchin, PL B599, 23)
28Another recent calculation
Very good description of the pT dependence of the
BRAHMS dAu ? h- X cross section at ?
3.2 (Dumitru, Hayashigaki, and Jalilian-Marian,
hep-ph/0506308)
29dAu ? p0X at 200 GeV
dAu p0 cross section at ? 4.0 is well
described by a LO CGC calculation with a K-factor
of 0.8 (Dumitru, Hayashigaki, and
Jalilian-Marian, hep-ph/0506308)
30Other possible tagged Drell-Yan measurements
(from Jen-Chieh Peng)
- p p ? ? l l - x
- Probe the p ? ? K component, and the strange
quark contents in the proton - p? p? ? n l l - x
- Measure helicity asymmetry ALL due to the meson
cloud (expect ALL 0) - p A ? A l l - x
- probe pion excess in nuclei via the
A-dependence measurement - Doubly-tagged Drell-Yan p p ? p p l l -
x - meson-meson annihilation (or pomeron
interactions)? - Other hard-diffractive processes at RHIC?
- tagged J/? production?
- tagged jet production?
- (gluon content of the meson cloud)
31Gluon saturation at small x shadowing in nuclei
Also important for AA initial state
RHIC allows study of transition. LHC always
saturated (except very high pT and ylt-3)
Especially for LHC where always saturated at
midrapidity
- Models
- gluon saturation, CGC
- leading twist shadowing (coherence)
- mass renorm. (Vitev)
- Sudakov suppr. (Kopeliovich)
- limiting fragmentation
LHC only 1-month/yr shared between pp, pA and AA
earliest pA 2010?
- How to distinguish??
- correlations
- energy,rapidity dependence
- universality
polarized and diffractive pA are useful - need
theoretical calculations.
need hard processes sensitive to gluons
- Forward hadrons
- need forw. p0 ? STAR FMS
- hadron PID for ygt1
compare open closed
Heavy-quarks (c,b) bound states
Direct photons for ygt1 ? PHENIX NCC
need cleaner way to get open-c, -b
wide kinematic range to understand physics
differentiate models
vertex detectors!
- Onia rare processes
- PHENIX onia
- Need STAR forward J/? ? ee
- separating D B in single-lepton spectra?
- use B ? J/? X measurement
- very high statistics could allow seeing 2 c?s
D ? Kp nice but difficult!
High Luminosities needed!
32Antiquark distribution in nucleon and nuclei
Also important for understanding gluon
distribution in nuclei
Flavor structure of parton distribution in nuclei
is practically unknown.
- Models
- Enhancement of antiquark in nuclei due to meson
cloud - Leading twist shadowing of antiquark at low-x
- Meson cloud explains the d-bar, u-bar asymmetry
in nucleon
Spin structure of the nucleon is closely
connected to the flavor structure of the nucleon
Nuclear shadowing of antiquark sea can be
measured at RHIC in pA
need hard process sensitive to antiquarks
Polarized Drell-Yan can probe seaquark
polarization complementary to W-production
Forward-tagging in p-p Drell-Yan can probe the
pion cloud directly
Drell-Yan process in pA and pp is ideal for
probing antiquarks
Roman pot and forward neutron tagging are
required
High Luminosities needed!