the balance function: experimental studies in star marguerite belt tonjes, g.d. westfall, a.m....

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The Balance Function: Experimental Studies in STAR Marguerite Belt Tonjes, G.D. Westfall, A.M. Vander Molen, the STAR collaboration

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Page 1: The Balance Function: Experimental Studies in STAR Marguerite Belt Tonjes, G.D. Westfall, A.M. Vander Molen, the STAR collaboration

The Balance Function:Experimental Studies in STAR

Marguerite Belt Tonjes,

G.D. Westfall, A.M. Vander Molen, the STAR collaboration

Page 2: The Balance Function: Experimental Studies in STAR Marguerite Belt Tonjes, G.D. Westfall, A.M. Vander Molen, the STAR collaboration

STARSTARSSolenoidal TTracker AAt RRHIC

• large acceptance detector with near 4 coverage, study hadrons, jets, event-by-event, high pt particles, strangeness.

Page 3: The Balance Function: Experimental Studies in STAR Marguerite Belt Tonjes, G.D. Westfall, A.M. Vander Molen, the STAR collaboration
Page 4: The Balance Function: Experimental Studies in STAR Marguerite Belt Tonjes, G.D. Westfall, A.M. Vander Molen, the STAR collaboration

Selecting Good Data• Use Au+Au 130GeV

events from Year1 running, summer, 2000

• Physics events:– Central trigger

– Minimum bias trigger

• -75cm ≤ vertexz ≤ 75cm

• -1cm ≤ vertexx ≤ 1cm,

• -1cm ≤ vertexy ≤ 1cm

Page 5: The Balance Function: Experimental Studies in STAR Marguerite Belt Tonjes, G.D. Westfall, A.M. Vander Molen, the STAR collaboration

Selecting good TPC tracks

Collaboration-wide selection cuts• | | < 1.3

• 0.1 GeV/c ≤ pt ≤ 2 GeV/c

• DCA ≤ 1 cm (distance of closest approach to the primary vertex choose tracks from the vertex)

• Fit points ≥ 15• Fit points/possible points > 0.52

Page 6: The Balance Function: Experimental Studies in STAR Marguerite Belt Tonjes, G.D. Westfall, A.M. Vander Molen, the STAR collaboration

PID

• Compare measured dE/dx with Bethe-Bloch calculation of dE/dx for , K, p, and e.

• Particles within 2 of predicted ionization are tagged.

Page 7: The Balance Function: Experimental Studies in STAR Marguerite Belt Tonjes, G.D. Westfall, A.M. Vander Molen, the STAR collaboration

PID cuts• ZPid = ln( Imeas/Ihyp())

– Imeas = measured truncated mean for track

– Ihyp() = expected ionization for hypothesis

• : p≤0.7 GeV/c, and |ZPidp|≤0.2• K: p≤0.8 GeV/c, |ZpidK|≤0.2, |ZPid|>0.2, |ZPidp|

>0.2• P: p≤ 1 GeV/c, |ZPidp|≤0.2, |ZPid|>0.2, |ZPidK|>0.2• E: |ZPide|≤0.2, |ZPid|>0.2, |ZPidK|>0.2, |ZPidp|>0.2

Page 8: The Balance Function: Experimental Studies in STAR Marguerite Belt Tonjes, G.D. Westfall, A.M. Vander Molen, the STAR collaboration

Calculating the Balance Function

• For pairs:– B = 1/2 { + - /N+ + - +/N- - ++/N+ - - -/N-}

– +- = Histogram of | y(+) - y(-) |, for all possible pairs within an event. This histogram is summed over all events.

• For charged particle pairs, we sum over all charged particle pairs.– +- = Histogram of | (particle+)-(particle-)|

Page 9: The Balance Function: Experimental Studies in STAR Marguerite Belt Tonjes, G.D. Westfall, A.M. Vander Molen, the STAR collaboration

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B(( )) - y HIJING central

( )y

pairs

: 80,000 HIJING central events

HIJING has || <1.3

Page 10: The Balance Function: Experimental Studies in STAR Marguerite Belt Tonjes, G.D. Westfall, A.M. Vander Molen, the STAR collaboration

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B(( ))/ - y binsize HIJING central

( )y

pairs

: 80,000 HIJING central events

|HIJING has | <0.8

Page 11: The Balance Function: Experimental Studies in STAR Marguerite Belt Tonjes, G.D. Westfall, A.M. Vander Molen, the STAR collaboration

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B(()) - HIJING central

()

All charged particle pairs

HIJING central: 80,000 events

Page 12: The Balance Function: Experimental Studies in STAR Marguerite Belt Tonjes, G.D. Westfall, A.M. Vander Molen, the STAR collaboration

Conclusions and future analysis• More statistics are needed, and are being analyzed• We see no difference between central and

peripheral events in HIJING

Need to study beam pipe/detector effects for simulations

Study pt sensitivity

Look at pp simulations

Page 13: The Balance Function: Experimental Studies in STAR Marguerite Belt Tonjes, G.D. Westfall, A.M. Vander Molen, the STAR collaboration

Thanks to

• Gary Westfall, Skip Vander Molen, Scott Pratt for much discussion of the analysis

• The STAR Collaboration

• DOE

• NSF