Carl Gagliardi – d+Au Collisions at STAR – DIS’06 1 d+Au Collisions at STAR Outline • d+Au collisions and saturation physics at RHIC • Recent STAR results • STAR plans for the future Carl A. Gagliardi Texas A&M University for the Collaboration STAR STAR
29
Embed
Carl Gagliardi – d+Au Collisions at STAR – DIS’06 1 d+Au Collisions at STAR Outline d+Au collisions and saturation physics at RHIC Recent STAR results.
This document is posted to help you gain knowledge. Please leave a comment to let me know what you think about it! Share it to your friends and learn new things together.
Transcript
Carl Gagliardi – d+Au Collisions at STAR – DIS’06 1
d+Au Collisions at STAR
Outline
• d+Au collisions and saturation physics at RHIC• Recent STAR results• STAR plans for the future
Carl A. GagliardiTexas A&M University
for the CollaborationSTARSTAR
Carl Gagliardi – d+Au Collisions at STAR – DIS’06 2
E-M Calorimeter
Time of Flight
Projection Chamber
STAR detector
Carl Gagliardi – d+Au Collisions at STAR – DIS’06 3
Mid-rapidity p+p at RHIC and NLO pQCDPRL 91, 241803
PHENIX π0
Calculations byW. Vogelsang
At 200 GeV, pQCD does a very good job describing mid-rapidity yields
STAR (h++h-)/2BRAHMS (h++h-)/2
Carl Gagliardi – d+Au Collisions at STAR – DIS’06 4
Mid-rapidity d+Au
PRL 91, 072304
Pedestal&flow subtracted
Inclusive yields and back-to-back di-hadron correlations are very similar in p+p and d+Au collisions
In contrast, Au+Au collisions are very different from p+p and d+Au – but that’s not the subject of this talk
STARSTAR
Carl Gagliardi – d+Au Collisions at STAR – DIS’06 5
Mid-rapidity vs. forward rapidity
MidRapidity
ForwardRapidity
CTEQ6M• Gluon density can’t grow forever.• Saturation may set in at forward rapidity when gluons start to overlap.• Can be explored by comparing p(d)+A to p+p.
yT es
px 2
~
Carl Gagliardi – d+Au Collisions at STAR – DIS’06 6
Forward particle production in d+Au collisionsBRAHMS, PRL 93, 242303
Sizable suppression in charged hadron production in d+Au collisions relative to p+p collisions at forward rapidity
BRAHMS
Carl Gagliardi – d+Au Collisions at STAR – DIS’06 7
ln 1x related to rapidity of
produced hadrons.
As y grows
Expectations for a color glass condensate
D. Kharzeev, hep-ph/0307037
Iancu and Venugopalan, hep-ph/0303204
Are the BRAHMS data evidence for gluon saturation at RHIC energies?
Carl Gagliardi – d+Au Collisions at STAR – DIS’06 8
Recent saturation model calculation
Very good description of the pT dependence of the BRAHMSd+Au → h− + X cross section at η = 3.2
(Dumitru, Hayashigaki, and Jalilian-Marian, NP A765, 464)
Carl Gagliardi – d+Au Collisions at STAR – DIS’06 9
Is saturation really the explanation?
Difficult to explain BRAHMS results with standard shadowing, but in NLO pQCD calculations <xg> ~ 0.02 is not that small
(Guzey, Strikman, and Vogelsang, PL B603, 173)
In contrast, <xg> <~ 0.001 in CGC calculations(Dumitru, Hayashigaki, and Jalilian-Marian, NP A765, 464 )
Basic difference:
pQCD: 2 2 CGC: 2 1
Carl Gagliardi – d+Au Collisions at STAR – DIS’06 10
Do we understand forward π0 production in p + p?
Bourrely and Soffer, EPJ C36, 371: NLO pQCD calculations underpredict the data at low s from ISR Ratio appears to be a function of angle and √s, in addition to pT
√s=23.3GeV √s=52.8GeV
xF xF
Ed
3 d
p3 [b
/GeV
3 ]
Ed
3 d
p3 [b
/GeV
3 ]
NLO calculations with different
scales:
pT and pT/2
Data-pQCD differences
at pT=1.5GeV
Carl Gagliardi – d+Au Collisions at STAR – DIS’06 11
The error bars are statistical plus point-to-point systematic
Consistent with NLO pQCD calculations at 3.3 < η < 4.0
Data at low pT trend from KKP fragmentation functions toward Kretzer. PHENIX observed similar behavior at mid-rapidity.
p+p +X at 200 GeV
nucl-ex/0602011
STARSTAR
Carl Gagliardi – d+Au Collisions at STAR – DIS’06 12
d+Au +X at 200 GeV
pT dependence of d+Au π0 cross section at <η> = 4.0 is best described by a LO CGC calculation.
(Dumitru, Hayashigaki, and Jalilian-Marian, NPA 765, 464)
nucl-ex/0602011
STARSTAR
Carl Gagliardi – d+Au Collisions at STAR – DIS’06 13
dependence of RdAu
nucl-ex/0602011
STARSTAR
pp
dAudAuR
197*2
1
• Observe significant rapidity dependence.
• pQCD calculations significantly over predict RdAu.
Carl Gagliardi – d+Au Collisions at STAR – DIS’06 14