cosmic ray at star

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2012/7/23 1 Cosmic Ray at STAR Shuai Yang Center of Particle Physics and Technology University of Science and Technolo gy of China STAR Regional Meeting Weihai, China, July 23 th – 25 th , 2012

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Cosmic Ray at STAR. STAR Regional Meeting Weihai, China, July 2 3 th – 25 th , 2012. Shuai Yang C enter of P article P hysics and T echnology U niversity of S cience and T echnology of C hina. Outline. Introduction Muon charge ratio from cosmic ray EAS Cosmic ray at STAR - PowerPoint PPT Presentation

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Page 1: Cosmic Ray at STAR

2012/7/23 1

Cosmic Ray at STAR

Shuai Yang

Center of Particle Physics and TechnologyUniversity of Science and Technology of China

STAR Regional MeetingWeihai, China, July 23th – 25th, 2012

Page 2: Cosmic Ray at STAR

2012/7/23 Shuai Yang, STAR Regional Meeting, Weihai 2

Outline Introduction

•Muon charge ratio from cosmic ray EAS •Cosmic ray at STAR

Event and Track selection •Event selection•Track selection•Match muon tracks

Analysis results•Improve of momentum resolution•Reject of gamma conversion event•μ+/μ- vs. Momentum•μ+/μ- vs. Multiplicity

Summary

Page 3: Cosmic Ray at STAR

2012/7/23 Shuai Yang, STAR Regional Meeting, Weihai 3

Muon charge ratio from cosmic ray EAS

Result of the MC simulation of iron and proton induced showers

• EAS: Extensive Air Shower, A fixed target experiment beyond LHC energy

Page 4: Cosmic Ray at STAR

2012/7/23 Shuai Yang, STAR Regional Meeting, Weihai 4

Cosmic ray at STAR

Advantage:• Precisely measure muon momentum upto several hundred

GeV/c• Large acceptance to measure muon bundles

x

y

Page 5: Cosmic Ray at STAR

2012/7/23 Shuai Yang, STAR Regional Meeting, Weihai 5

Event selection

Cosm

ic triggers

Laser run

All E

vents

Reversed Full Field

tracks>=

2 &&

runId cuts

Full Field

• Global tracks >=2• Reject bad runIds• Cosmic trigger Ids & no laser trigger Id

Event Candidates

Page 6: Cosmic Ray at STAR

2012/7/23 Shuai Yang, STAR Regional Meeting, Weihai 6

Track selection

• 700>Track_flag>0• nHitsFit>=15• P > 3 GeV/c

Muon Track Candidates

Page 7: Cosmic Ray at STAR

2012/7/23 Shuai Yang, STAR Regional Meeting, Weihai 7

x

y

Match muon tracks Project tracks onto R=220cm plane,

pickup the upstream point For every two tracks with p>3 GeV/c

• Compare R*(pos_phi2-pos_phi1)• Compare pos_z2 – pos_z1• Compare p_phi2-p_phi1 and p_theta2 – p_theta1• p = -p for the track with larger firstPoint_y

For those qualified from above 2D cuts are considered as matched candidates.

Page 8: Cosmic Ray at STAR

2012/7/23 Shuai Yang, STAR Regional Meeting, Weihai 8

2D cuts to further suppress random combinatorial background

2D correlation for muon matching

Page 9: Cosmic Ray at STAR

2012/7/23 Shuai Yang, STAR Regional Meeting, Weihai 9

Improve momentum resolutionRefit_1

Page 10: Cosmic Ray at STAR

2012/7/23 Shuai Yang, STAR Regional Meeting, Weihai 10

•Refit_2: makes a direct helix refit to all the hit points from the paired tracks(still ongoing, not finish yet)

By Prof. Shao

Page 11: Cosmic Ray at STAR

2012/7/23 Shuai Yang, STAR Regional Meeting, Weihai 11

“Neutral” track

The reason of "neutral" track:• Gamma conversion (low momentum)• The charge sign for one track is wrong(large

momentum)

Page 12: Cosmic Ray at STAR

2012/7/23 Shuai Yang, STAR Regional Meeting, Weihai 12

Gamma conversion3-10GeV/c

3-10GeV/c

200-1000GeV/c

200-1000GeV/c

The charge sign is redefined from the refit after rejecting the gamma conversion events according the deflection direction

Page 13: Cosmic Ray at STAR

2012/7/23 Shuai Yang, STAR Regional Meeting, Weihai 13

Results

• μ+/μ- vs. Momentum• μ+/μ- vs. Multiplicity

Proton induced showers: low multiplicity ratio > 1 (~1.3)

Iron induced showers: high multiplicity ratio ~ 1

Page 14: Cosmic Ray at STAR

2012/7/23 Shuai Yang, STAR Regional Meeting, Weihai 14

Ratio vs. Momentum

FF

FF FF

FF

Page 15: Cosmic Ray at STAR

2012/7/23 Shuai Yang, STAR Regional Meeting, Weihai 15

Different Multiplicity definition

•MuonpairMult: Selected Muonpair events•MatchMult: flag of global track (0,700) ∈ ; flag of match >0•SingleMuonMult: Selected Muon events•GlobalMult: flag of global track (0,700) ∈ ; nHitsFit>= 15 ; firstpoint.Z() && lastpoint.Z() ∈ [-180,180] •TofMult: BTofHit(BTofHit_mTray[i]<=120)

Page 16: Cosmic Ray at STAR

2012/7/23 Shuai Yang, STAR Regional Meeting, Weihai 16

MuonpairMult. - the most reliable multiplicity definition

RFF FF

• Decrease with multiplicity?

• Reconstructed Muonpair Multiplicity is too small

Page 17: Cosmic Ray at STAR

2012/7/23 Shuai Yang, STAR Regional Meeting, Weihai 17

MatchMult.

RFF FF

Page 18: Cosmic Ray at STAR

2012/7/23 Shuai Yang, STAR Regional Meeting, Weihai 18

SingleMuonMult.

RFF FF

Page 19: Cosmic Ray at STAR

2012/7/23 Shuai Yang, STAR Regional Meeting, Weihai 19

GlobalMult.

From the ratio vs. four different multiplicity definitions:• Ratio decreases with increasing multiplicity. • Physics reason? Detector reason?

RFF FF

Page 20: Cosmic Ray at STAR

2012/7/23 Shuai Yang, STAR Regional Meeting, Weihai 20

TofMult.

• Most of the tof hits are not associated with global track.

Page 21: Cosmic Ray at STAR

2012/7/23 Shuai Yang, STAR Regional Meeting, Weihai 21

Summary

• We can matched muon tracks with good s/b ratio and efficiency

• Combined two muon tracks can improve the momentum resolution

• Can get ratio with very good precision upto several hundred GeV/c

• Can observe ratio decrease with multiplicity, but need to check the reason.