20
ISMD 2015 Oct. 4-9, 2015 Wildbad Kreuth, Germany L. Gutay Department of Physics & Astronomy Purdue University, USA in collaboration with A. S. Hirsch & R. P. Scharenberg & B. K. Srivastava 1

L. Gutay Department of Physics & Astronomy Purdue ......Inverse slope = 220 ± 20 MeV . PRL 104, 132301 (2010 ) Pb+Pb @ 2.76TeV for 0-5% . T ~265 MeV . ALICE : Direct Photon Measurement

  • Upload
    others

  • View
    2

  • Download
    0

Embed Size (px)

Citation preview

Page 1: L. Gutay Department of Physics & Astronomy Purdue ......Inverse slope = 220 ± 20 MeV . PRL 104, 132301 (2010 ) Pb+Pb @ 2.76TeV for 0-5% . T ~265 MeV . ALICE : Direct Photon Measurement

ISMD 2015 Oct. 4-9, 2015 Wildbad Kreuth, Germany

L. Gutay Department of Physics & Astronomy

Purdue University, USA

in collaboration with

A. S. Hirsch & R. P. Scharenberg & B. K. Srivastava

1

Page 2: L. Gutay Department of Physics & Astronomy Purdue ......Inverse slope = 220 ± 20 MeV . PRL 104, 132301 (2010 ) Pb+Pb @ 2.76TeV for 0-5% . T ~265 MeV . ALICE : Direct Photon Measurement

Proposal to search for QGP at the Fermi Lab CO Collider

pp At 1.8 TeV The experiment was accepted as E-735 in 1983

2

The Detector consisted of : • Scintillator vertex hodoscope • A Side arm magnetic spectrometer • A time of flight system for particle identification

Page 3: L. Gutay Department of Physics & Astronomy Purdue ......Inverse slope = 220 ± 20 MeV . PRL 104, 132301 (2010 ) Pb+Pb @ 2.76TeV for 0-5% . T ~265 MeV . ALICE : Direct Photon Measurement

E-735 Measurements Temperature as a function of

Length of multiplicity involved

Particle identity :π, K, p, , d, Freeze-out energy density

dndη

p

Conclusion: Evidence for de-confinement was published in 2002. The comparison was Made with Lattice QCD calculations. Phys. Lett. B528, 43 (2002).

Λ

3

Here we present the results which come from reanalysis of the E-735 data using Color String Percolation Model. The results are also compared with with Lattice QCD simulations.

Page 4: L. Gutay Department of Physics & Astronomy Purdue ......Inverse slope = 220 ± 20 MeV . PRL 104, 132301 (2010 ) Pb+Pb @ 2.76TeV for 0-5% . T ~265 MeV . ALICE : Direct Photon Measurement

Percolation : General It is well known that the percolation problem on a large lattice displays the features of a system undergoing a second-order phase transition. For example:

1. H. E. Stanley , Introduction to Phase Transitions and Critical Phenomena 2. D. Stauffer and A. Aharony, Introduction to Percolation Theory

* Transition from liquid to gas * Normal conductor to a superconductor * Paramagnet to ferromagnet

4

Page 5: L. Gutay Department of Physics & Astronomy Purdue ......Inverse slope = 220 ± 20 MeV . PRL 104, 132301 (2010 ) Pb+Pb @ 2.76TeV for 0-5% . T ~265 MeV . ALICE : Direct Photon Measurement

Parton Percolation

Multiparticle production at high energies is currently described in terms of color strings stretched between the projectile and target. Hadronizing these strings produces the observed hadrons. The no. of strings grow with energy and the no. of participating nuclei and one expects that interaction between strings becomes essential.

Clustering of Color Sources

De-confinement is thus related to cluster formation very much similar to cluster formation in percolation theory Critical Percolation Density

1.20cξ =

5

Page 6: L. Gutay Department of Physics & Astronomy Purdue ......Inverse slope = 220 ± 20 MeV . PRL 104, 132301 (2010 ) Pb+Pb @ 2.76TeV for 0-5% . T ~265 MeV . ALICE : Direct Photon Measurement

Multiplicity (µn)

Average Transverse Momentum

1)( µξµ sn NF= )(/1

22 ξFpp TnT >=<><

Multiplicity and <pT2 > of particles

produced by a cluster of n strings

Color Strings + Percolation = CSPM

Complete description of CSPM has been published in Phys. Rep. Sept. 2015 Braun, Deus, Hirsch, Pajares, Scharenberg, Srivastava

ξξ

ξ−−=

eF 1)( = Color suppression factor (due to overlapping of discs).

ξ is the percolation density parameter.

N

s

SSN 1=ξ

Ns = # of strings S1 = disc area SN = total nuclear overlap area

6

Page 7: L. Gutay Department of Physics & Astronomy Purdue ......Inverse slope = 220 ± 20 MeV . PRL 104, 132301 (2010 ) Pb+Pb @ 2.76TeV for 0-5% . T ~265 MeV . ALICE : Direct Photon Measurement

The experimental pT distribution from pp data is used

2

2

0

( )( )

t ppt

AuA

n

u

p

d N b

dp Fp

ξ

=

+

a, p0 and n are parameters fit to the data.

This parameterization can be used for nucleus-nucleus collisions to account for the clustering :

Using the pT spectrum to calculate ξ Data Analysis

0

2

2( )t

n

t

d N a

pdp p=

+

pt GeV/c

2

2t

d Ndp

Charged Hadron spectrum

( ) 1ppF ξ =

( ) 0.57AuAuF ξ =

For central collisions

7

Page 8: L. Gutay Department of Physics & Astronomy Purdue ......Inverse slope = 220 ± 20 MeV . PRL 104, 132301 (2010 ) Pb+Pb @ 2.76TeV for 0-5% . T ~265 MeV . ALICE : Direct Photon Measurement

8

Page 9: L. Gutay Department of Physics & Astronomy Purdue ......Inverse slope = 220 ± 20 MeV . PRL 104, 132301 (2010 ) Pb+Pb @ 2.76TeV for 0-5% . T ~265 MeV . ALICE : Direct Photon Measurement

2k

=)(2

1

2

ξF

pT t

=

Schwinger Mechanism of Particle Production pt distribution of the produced quarks

2

2 ~ exp( )t

t

pdnd p k

π−

Thermal Distribution 2 ~ exp( )t

t

pdnd p T

π−

k is the string tension

The tension of the macroscopic cluster fluctuates around its mean value because the chromoelectric field is not constant . Assuming a Gaussian form for these fluctuations one arrives at the probability distribution of transverse momentum.

Cluster /Initial Temperature

9

Page 10: L. Gutay Department of Physics & Astronomy Purdue ......Inverse slope = 220 ± 20 MeV . PRL 104, 132301 (2010 ) Pb+Pb @ 2.76TeV for 0-5% . T ~265 MeV . ALICE : Direct Photon Measurement

Temperature

)(21

2

ξF

pT t

=

For Au+Au@ 200 GeV ( STAR data) 0-10% centrality ξ = 2.88 T ~ 195 MeV

PHENIX: Temperature from direct photon Exponential (consistent with thermal) Inverse slope = 220 ± 20 MeV PRL 104, 132301 (2010)

Pb+Pb @ 2.76TeV for 0-5% T ~265 MeV

ALICE : Direct Photon Measurement T = 304 ± 51 MeV, QM 2012

10

The connectivity or percolation threshold for the formation of the “spanning” cluster occurs when the string density is ξ = 1.2.

F(ξ) at ξ=1.2 and the Universal Hadronization Temperature T = 167 ± 2.2 MeV are used to accurately calibrate the T(ξ) scale. This accurately determines the single string momentum. √< pt

2 >1 = 207.2 ± 3.3 MeV.

CSPM result:

Page 11: L. Gutay Department of Physics & Astronomy Purdue ......Inverse slope = 220 ± 20 MeV . PRL 104, 132301 (2010 ) Pb+Pb @ 2.76TeV for 0-5% . T ~265 MeV . ALICE : Direct Photon Measurement

11

Page 12: L. Gutay Department of Physics & Astronomy Purdue ......Inverse slope = 220 ± 20 MeV . PRL 104, 132301 (2010 ) Pb+Pb @ 2.76TeV for 0-5% . T ~265 MeV . ALICE : Direct Photon Measurement

Energy Density

3/123 fmGeV

Am

dydN

pro

tc

τε

><=

Bjorken 1D expansion

Transverse overlap area Proper Time

proτ is the QED production time for a boson which can be scaled from QED to QCD and is given by

><=

tpro m

405.2τ

Introduction to high energy heavy ion collisions C. Y. Wong

J. Dias de Deus, A. S. Hirsch, C. Pajares , R. P. Scharenberg , B. K. Srivastava Eur. Phys. J. C 72, 2123 ( 2012)

ξε ∝

12

Page 13: L. Gutay Department of Physics & Astronomy Purdue ......Inverse slope = 220 ± 20 MeV . PRL 104, 132301 (2010 ) Pb+Pb @ 2.76TeV for 0-5% . T ~265 MeV . ALICE : Direct Photon Measurement

Having determined the initial temperature of the system from the data one would like to

obtain the following quantities to understand the properties of QCD matter

Shear Viscosity

Equation of State

4/ Tε

13

Page 14: L. Gutay Department of Physics & Astronomy Purdue ......Inverse slope = 220 ± 20 MeV . PRL 104, 132301 (2010 ) Pb+Pb @ 2.76TeV for 0-5% . T ~265 MeV . ALICE : Direct Photon Measurement

Energy Density /T4

14

Page 15: L. Gutay Department of Physics & Astronomy Purdue ......Inverse slope = 220 ± 20 MeV . PRL 104, 132301 (2010 ) Pb+Pb @ 2.76TeV for 0-5% . T ~265 MeV . ALICE : Direct Photon Measurement

The viscosity can be estimated from kinetic theory to be

4 1 ( )( )15 5 ( )

3( )41

( )

5

mfptr

trtr

mfp

T s TTn T

T Ts

nT

s

η ε λσ

ε

λσ

λη

≈ ≈

=

=

ε Energy density s Entropy density n the number density mfpλ Mean free path

trσ Transport cross section

ξλ−−

=eL

mfp 1T

eL

s ξη

−−≈

151

21tp< >

Average transverse momentum of the single string

Hirano & Gyulassy, Nucl. Phys. A769, 71(2006) L is Longitudinal extension of the source 1 fm

15

Page 16: L. Gutay Department of Physics & Astronomy Purdue ......Inverse slope = 220 ± 20 MeV . PRL 104, 132301 (2010 ) Pb+Pb @ 2.76TeV for 0-5% . T ~265 MeV . ALICE : Direct Photon Measurement

Shear Viscosity to Entropy Density ratio

16

Page 17: L. Gutay Department of Physics & Astronomy Purdue ......Inverse slope = 220 ± 20 MeV . PRL 104, 132301 (2010 ) Pb+Pb @ 2.76TeV for 0-5% . T ~265 MeV . ALICE : Direct Photon Measurement

Trace Anomaly

17

COMPARE the trace anomaly Ansatz (η/S)-1= S/η with the trace anomaly from hot QCD Δ (T) =(ε -3p)/T4

S/η (T) and Δ (T) have the same magnitude and temperature dependence. Ansatz: we will use S/η (T) to correlate ε(T) and p(T) for T>TC

Page 18: L. Gutay Department of Physics & Astronomy Purdue ......Inverse slope = 220 ± 20 MeV . PRL 104, 132301 (2010 ) Pb+Pb @ 2.76TeV for 0-5% . T ~265 MeV . ALICE : Direct Photon Measurement

Sound Velocity 4

3pT

ε −∆ = 2 /

sdp dp pCd d

εεε ε ε

= = +

CS2 = (−0.33) ξe−ξ

1− e−ξ − 1

+ 0.0191(∆ / 3)ξe−ξ

(1− e−ξ )2 −

11− e−ξ

18

Page 19: L. Gutay Department of Physics & Astronomy Purdue ......Inverse slope = 220 ± 20 MeV . PRL 104, 132301 (2010 ) Pb+Pb @ 2.76TeV for 0-5% . T ~265 MeV . ALICE : Direct Photon Measurement

Summary The p¯p collisions at √s = 1.8 TeV from the E735 experiment have been

re-analyzed in using the clustering of color sources data based phenomenology.

The Percolation framework provide us with a microscopic partonic

structure which explains the early thermalization. The Bjorken ideal fluid description of the QGP , when modified by the

color reduction factor and the trace anomaly ∆ represented by s/η is in remarkable agreement with the Lattice Quantum Chromo Dynamics(LQCD) simulations.

These results prove that even in small systems at high energy and high multiplicity events , QGP formation is possible as seen in collisions at

√s= 1.8 TeV. A further definitive test of clustering phenomena can be made at LHC energies by comparing h-h and A-A collisions.

pp

19

Page 20: L. Gutay Department of Physics & Astronomy Purdue ......Inverse slope = 220 ± 20 MeV . PRL 104, 132301 (2010 ) Pb+Pb @ 2.76TeV for 0-5% . T ~265 MeV . ALICE : Direct Photon Measurement

References 1. De-Confinement and clustering of color sources in nuclear collisions To appear in Phys. Rep. ( Sept. 2015)* 2. Clustering of Color sources and shear viscosity to entropy density Eur. Phys. J. C 72, 2123 (2012)** 3. Percolation of color sources and the equation of state of QGP…. Eur. Phys. J. C 71, 1510 (2011)*** 4. The QGP EOS by measuring the color suppression factor at RHIC and LHC R. P. Scharenberg , CPOD 2013, 017 (2013) 5. Percolation approach to initial stage effects in high energy collisions B. K. Srivastava , Nucl. Phys. A926, 142(2014) * Braun, Deus, Hirsch, Pajares, Scharenberg and Srivastava ** Deus, Hirsch, Pajares, Scharenberg and Srivastava *** Scharenberg, Srivastava and Hirsch

20