first results from star experiment at rhic - soft hadron physics -

25
Masashi Kaneta, LBNL Masashi Kaneta for the STAR collaboration Lawrence Berkeley National Lab. First results from STAR experiment at RHIC - Soft hadron physics -

Upload: svea

Post on 12-Jan-2016

27 views

Category:

Documents


2 download

DESCRIPTION

First results from STAR experiment at RHIC - Soft hadron physics -. Masashi Kaneta for the STAR collaboration Lawrence Berkeley National Lab. Focus on. Hadrons Measured : h - , p ± , K ± , K 0 s , K *0 , K *0 , p , p , d , 3 He , 3 He , t , L , L , X - , X + , - PowerPoint PPT Presentation

TRANSCRIPT

Page 1: First results from STAR experiment at RHIC - Soft hadron physics -

Masashi Kaneta, LBNL

Masashi Kanetafor the STAR collaboration

Lawrence Berkeley National Lab.

First results from STAR experiment at RHIC- Soft hadron physics -

Page 2: First results from STAR experiment at RHIC - Soft hadron physics -

Masashi Kaneta, LBNL

Focus onHadrons

Measured : h, ±, K±, K0s, K*0, K*0, p, p, d, 3He, 3He,

t,In future : 0 +’, , J/ and more

Freeze-out conditions of low momentum hadrons by

Spectra/Ratios• Thermal/Chemical Freeze-out

Particle correlations• Size parameters, Phase space density

Event anisotropy• v2

Page 3: First results from STAR experiment at RHIC - Soft hadron physics -

Masashi Kaneta, LBNL

Spectra

Page 4: First results from STAR experiment at RHIC - Soft hadron physics -

Masashi Kaneta, LBNL

Spectra

Momentum distributionsInformation of thermal (kinetic) freeze-out

The inverse slope parameter of mT distribution reflects temperature and radial flow

Page 5: First results from STAR experiment at RHIC - Soft hadron physics -

Masashi Kaneta, LBNL

Only stat. errors are shown

p

K-

central collisions

6%11-1

8%

26-3

4%

45-5

8%

58-8

5%

Identified particle spectra

p

K-

central collisions

6%11-1

8%

26-3

4%

45-5

8%

58-8

5%

Only stat. errors are shown

Page 6: First results from STAR experiment at RHIC - Soft hadron physics -

Masashi Kaneta, LBNL

Thermal(Kinetic) freeze-out

Thermal freeze-out at RHICTemperature is similar at SPSLarger radial flow than at SPS

STAR (sNN=130 GeV)

c

T fo

60.0

MeV95

Hydrodynamical model: E. Schnedermann et al.PRC48(1993)2462

mT-mass [GeV/c2]

mass [GeV/c2]

Inve

rse

slop

e pa

ram

eter

[G

eV/c

2 ]

Page 7: First results from STAR experiment at RHIC - Soft hadron physics -

Masashi Kaneta, LBNL

Ratios

Page 8: First results from STAR experiment at RHIC - Soft hadron physics -

Masashi Kaneta, LBNL

Ratios

pT dependence anti-particle/particleTest slope for particle and anti-particle

Anti-baryon/baryon ratioStopping or transparent?

Particle ratios from hadronsChemical freeze-out parameters

Page 9: First results from STAR experiment at RHIC - Soft hadron physics -

Masashi Kaneta, LBNL

p/p ratio

Minimum bias dataNo or weak pT dependence

Submitted to PRLSystematic errors<10%

Page 10: First results from STAR experiment at RHIC - Soft hadron physics -

Masashi Kaneta, LBNL

/ ratio

No significant pT dependence in the ratio

The mean ratio = 0.72±0.04

From 200 K Central trigger Au+Au Events (top ~15% multiplicity.)

Systematic errors are under evaluation

|y|<0.5

r

atio

Page 11: First results from STAR experiment at RHIC - Soft hadron physics -

Masashi Kaneta, LBNL

K+/K ratiora

tio

pT [GeV/c]

STAR Preliminary

|y|<0.5Event fraction = top 7%

Page 12: First results from STAR experiment at RHIC - Soft hadron physics -

Masashi Kaneta, LBNL

Multiplicity dependence of ratios

Not baryon free at mid-rapidity

An effect of anti-baryon absorption in central collisions?

(nch/nmax)

/ Preliminary

Preliminary

P e r i p h e r a l C e n t r a l

p/p submitted to PRL pT 0.6-0.8 GeV/c |y|<0.3

Only statistic errors are shown Systematic errors p/p : 10%

and : under evaluation

ratio

Page 13: First results from STAR experiment at RHIC - Soft hadron physics -

Masashi Kaneta, LBNL

Chemical freeze-out

Baryonic Potential B [MeV]

Chem

ical Tem

pera

ture

Tch

[M

eV

]

0

200

250

150

100

50

0 200 400 600 800 1000 1200

AGS

SIS

LEP/

SppS

SPS

quarks-gluons

hadrons

RHIC

Experimental ratio

Mod

el p

redi

ctio

n of

rat

io

48±12B

Page 14: First results from STAR experiment at RHIC - Soft hadron physics -

Masashi Kaneta, LBNL

HBT

Page 15: First results from STAR experiment at RHIC - Soft hadron physics -

Masashi Kaneta, LBNL

HBT

Pion HBTCentralityTransverse momentumThe HBT excitation function

Phase space densityEvent-by-Event HBTK0

s K0s,

pp, pp correlationsNon-identical particles

Many topics in STAR measurement

The HBT excitation function Focus in this talk

Page 16: First results from STAR experiment at RHIC - Soft hadron physics -

Masashi Kaneta, LBNL

The HBT excitation function

Compilation 3D -HBT parameters as a function of s

• ~10% Central Au+Au(Pb+Pb) events• y ~ 0 • kT 0.17 GeV/c

STAR PreliminaryNo significant jump

from SPS to RHICWe need energy scan between both energy

Page 17: First results from STAR experiment at RHIC - Soft hadron physics -

Masashi Kaneta, LBNL

EventAnisotropy

Page 18: First results from STAR experiment at RHIC - Soft hadron physics -

Masashi Kaneta, LBNL

Event anisotropy

In momentum spaceAnisotropy measured as second harmonic parameter v2

v2 will be scale to initial shape parameter ,

if the source has a hydrodynamical expansion

x

y

p

patan2cos2 v

Momentum space

Almond shape overlap region in coordinate space

y2 x2 y2 x2

Page 19: First results from STAR experiment at RHIC - Soft hadron physics -

Masashi Kaneta, LBNL

Charged particle v2 versus Multiplicity

PRL 86, (2001) 402

|| < 1.3

0.1 < pT < 2.0

Boxes show “initial spatial anisotropy” scaled by 0.19-0.25

nch = primary tracks in || < 0.75

Page 20: First results from STAR experiment at RHIC - Soft hadron physics -

Masashi Kaneta, LBNL

Charged and p+p, v2(pT) (M.B.)

Page 21: First results from STAR experiment at RHIC - Soft hadron physics -

Masashi Kaneta, LBNL

Comparison with a hydrodynamical model

Hydrodynamical calculations: Huovinen, Kolb and Heinz

Page 22: First results from STAR experiment at RHIC - Soft hadron physics -

Masashi Kaneta, LBNL

Charged particle anisotropy 0<pT<4.5 GeV/c

Minimum bias data

Only statistical errors

Systematic error 10% - 20% for pt = 2 – 4.5 GeV/c

Page 23: First results from STAR experiment at RHIC - Soft hadron physics -

Masashi Kaneta, LBNL

Summary

Net-baryon 0 at mid-rapidityAnti-baryon/baryon ratios are toward 1, but still <1

Chemical Freeze-outTch : same or higher than at SPS

B : smaller than at SPS

HBT parametersSimilar to SPS

Large anisotropic flowFrom mid-central to central data,Hydrodynamical model can describe v2 at low pT (<2GeV/c)

Thermal Freeze-outTfo : similar to SPS/AGSLarge radial flow

We need energy scan between SPS and RHIC!

Page 24: First results from STAR experiment at RHIC - Soft hadron physics -

Masashi Kaneta, LBNL

Future plansTOF

PID up to 2GeV/c of pT

SVTIncreasing momentum resolutionMore strangeness baryons

EMCElectron measurement

Full fieldsHigher pT measurementIncreasing momentum resolution

With high statistics

Physics of0, and resonances

Page 25: First results from STAR experiment at RHIC - Soft hadron physics -

Masashi Kaneta, LBNL

Typical e+e pairfrom

e+

e+

e+

e+

e-

e-

e-e-

invariant mass [GeV]

STAR Preliminary

and0

The e+e pair from conversion is measured

Large acceptance pT = 50 MeV/c to ~4 GeV/c, ||<1.8