3d pion & kaon source imaging from run4 and run7 200 agev au+au collisions

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March 16, 2022 WPCF 2010, Kiev 1 3D Pion & Kaon Source Imaging from Run4 and Run7 200 AGeV Au+Au collisions Paul Chung (STAR Collaboration) NPI ASCR Prague

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Paul Chung (STAR Collaboration) NPI ASCR Prague. 3D Pion & Kaon Source Imaging from Run4 and Run7 200 AGeV Au+Au collisions. 1. PHENIX 1D Source Imaging. Phys.Rev.Lett.98:132301,2007. Phys.Rev.Lett.103:142301,2009. Outline. Run 4 Au+Au @ 200AGeV: 3D pion correlation functions - PowerPoint PPT Presentation

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April 24, 2023 WPCF 2010, Kiev 11

3D Pion & Kaon Source Imaging from Run4 and Run7 200 AGeV Au+Au collisions

Paul Chung (STAR Collaboration)NPI ASCR Prague

PHENIX 1D Source Imaging Phys.Rev.Lett.98:132301,2007

April 24, 2023 WPCF 2010, Kiev 2

Phys.Rev.Lett.103:142301,2009

April 24, 2023 WPCF 2010, Kiev 33

Outline

Run 4 Au+Au @ 200AGeV: 3D pion correlation functions Overview of 3D source shape analysis : Cartesian

Spherical Harmonic decomposition & Imaging Technique Correlation moments for low kT (0.25<kT<0.35 GeV)

pion pairs from peripheral collisions (50<cen<80%). 3D source function extraction: Moment Imaging & Fitting Therminator comparison for extracting pion source

lifetime & pion emission duration 3D Kaon correlation functions from Run 4 & Run 7

central Au+Au collisions Kaon source extraction & Therminator comparison

April 24, 2023 WPCF 2010, Kiev 44

Technique Devised by:

D. Brown, P. Danielewicz,PLB 398:252 (1997). PRC 57:2474 (1998).

Inversion of Linear integral equation to obtain source function

20( ) 1 ) (,4 ( )C K q r S rq drr

Source Source functionfunction

(Distribution of pair separations)

Encodes FSI

CorrelationCorrelationfunctionfunction

Inversion of this integral equation== Source Function

Emitting source

1D Koonin Pratt Eqn.

Extracted S(r) in pair CM frameHence Model-independent i.e Kernel independent of freeze-out conditions

No Shape assumption for S(r)

1D Imaging Formulation 1D Imaging Formulation

April 24, 2023 WPCF 2010, Kiev 55

Imaging : Inversion procedureImaging : Inversion procedure2( ) 4 ( , ) ( )C q drr K q r S r

( ) ( )j jj

S r S B r

( )

( , ) ( )

Thi ij j

j

ij j

C q K S

K dr K q r B r

2

22

( )

( )

Expti ij j

jExpt

i

C q K S

C q

Freeze-out occurs after last scattering Hence only Coulomb & BE effect included in kernel

Expansion in B-spline basis

April 24, 2023 WPCF 2010, Kiev 66

1D Imaging1D Imaging

ST

STAR PRELIMINARY STAR PRELIMINARY

April 24, 2023 WPCF 2010, Kiev 77

1 11

1 11

.... ........

.... ........

( ) ( ) (1)

( ) ( ) (2)

l ll

l ll

l lq

l

l lr

l

R q R q

S r S r

3( ) ( ) 1 4 ( , ) ( )R q C q dr K q r S r

(3)3D Koonin3D KooninPrattPratt

Plug in (1) and (2) into (3)1 1

2.... ....

( ) 4 ( , ) ( ) (4)l l

l llR q drr K q r S r

1 1

1 1

.... ....

.... ....

2 1 !!( ) ( ) ( ) (4)

! 42 1 !!

( ) ( ) ( ) (5)! 4

l l

l l

ql lq

l lrr

dlR q R q

ll dS r S rl

Invert (1)

Invert (2)

Expansion of R(q) and S(r) in Cartesian Harmonic basisExpansion of R(q) and S(r) in Cartesian Harmonic basis[Danielewicz and Pratt nucl-th/0501003 (v1)][Danielewicz and Pratt nucl-th/0501003 (v1)]

x=out-direction

y=side-direction

z=long-direction

3D Analysis Basics

April 24, 2023 WPCF 2010, Kiev 88

Monte Carlo Events:Phasemaker, Therminator

CRAB 3D C(q)

Correlation MomentsSource FITTING

Source IMAGING

SourceFunction

Model calculation from space points

SIMULATION PROCEDURE

April 24, 2023 WPCF 2010, Kiev 9

Fit Functions

Ellipsoid Fit (3D Gaussian) : G = lambda exp[-{ (x/2rx)2 + (y/2ry)2 + (z/2rz)2 }]

Hump Fit :H = exp[- Fs { (x/2rxs)2 + (y/2rys)2 + (z/2rzs)2 }] x

exp[- Fl { (x/2rxl)2 + (y/2ryl)2 + (z/2rzl)2 }]

Fs = 1/[1 + (r/r0)2 ]

Fl = 1 - Fs

April 24, 2023 WPCF 2010, Kiev 1010

Simulation – Therminator

April 24, 2023 WPCF 2010, Kiev 11

Comparison- C0 moment vs 1D C(q)

STAR PRELIM.STAR PRELIMINARY

L=2 & 4 moments

April 24, 2023 WPCF 2010, Kiev 12

STAR PRELIMINARY STAR PRELIMINARY

April 24, 2023 WPCF 2010, Kiev 13

L=6 moments

STAR PRELIMINARY

April 24, 2023 WPCF 2010, Kiev 1414

Imaging C2x2 & C2

y2

STAR PRELIMINARY STAR PRELIMINARY

April 24, 2023 WPCF 2010, Kiev 15

3D Imaging – S(r) & restored C(q)

STAR PRELIMINARY

STAR PRELIMINARY

April 24, 2023 WPCF 2010, Kiev 16

Ellipsoid vs Hump Fit : l=0 & 2 mom.

STAR PRELIMINARY

April 24, 2023 WPCF 2010, Kiev 17

Ellipsoid vs Hump Fit : l=4 moments

STAR PRELIMINARYSTAR PRELIMINARY

April 24, 2023 WPCF 2010, Kiev 18

Ellipsoid vs Hump Fit : l=6 moments

STAR PRELIMINARY

April 24, 2023 WPCF 2010, Kiev 19

Image vs Ellipsoid & Hump S(r)

STAR PRELIMINARY STAR PRELIMINARY

April 24, 2023 WPCF 2010, Kiev 20

3D C(q) : Ellipsoid vs Hump Fit

STAR PRELIMINARY STAR PRELIMINARY

April 24, 2023 WPCF 2010, Kiev 21

Therminator BW: Source lifetime & Pion emission duration extractionTherminator (Kisiel et al PRC

73, 064902 2006) : Production of particles from thermalized and expanding system with

Boost invariance & cylindrical symmetry

BW mode: Freeze-out hypersurface defined by constant laboratory time independent of transverse radius

April 24, 2023 WPCF 2010, Kiev 22

STAR vs PHENIX comparison

STAR PRELIMINARY STAR PRELIMINARY

Source extraction – central collisions PRL100, 232301 (2008) (PHENIX) Transverse dimension = 8.9fm

Source lifetime = 8.5fm/cEmission duration = 2fm/c

Source parameters larger for central collisions than for peripheral collisions

Full centrality dependence extraction underway

April 24, 2023 WPCF 2010, Kiev 23

April 24, 2023 WPCF 2010, Kiev 24

Run 7 & Run 4 KK : C0 vs 1D C(qinv)

STAR PRELIMINARY STAR PRELIMINARY

April 24, 2023 WPCF 2010, Kiev 25

Run 7 + Run 4 KK : C0 vs 1D C(qinv)

STAR PRELIMINARY

Run 7 + Run 4 KK : l=2 & l=4 moments

April 24, 2023 WPCF 2010, Kiev 26

STAR PRELIMINARY STAR PRELIMINARY

KK: Ellipsoid Fit

April 24, 2023 WPCF 2010, Kiev 27

STAR PRELIMINARY STAR PRELIMINARY

THERMINATOR Model comparison

April 24, 2023 WPCF 2010, Kiev 28

April 24, 2023 WPCF 2010, Kiev 2929

Conclusion

Correlation moments for low kT pion pairs from Run4 peripheral Au+Au collisions well described by the Hump Fit function.

For low kT pion pairs from peripheral collisions, inferred pion source lifetime ~ 3.5 fm/c & pion emission duration ~ 1 fm/c < central collisions.

Extracted Kaon source function essentially Gaussian – No significant non-Gaussian tail observed.

Kaon source dimension & lifetime smaller than for pion source; Kaon emission instantaneous (Therminator)