femtoscopy in heavy ion collisions: two decades of progress
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Femtoscopy in heavy ion collisions: Two decades of progress. Mike Lisa Ohio State University. An experimentalist’s view of the situation B.Q.M.( * ) cf. Bysterský, Chajecki, Chaloupka, Chung, Kisiel, Kniege, Panitkin. * BQM= Before Quark Matter. Outline. Relevance of femtoscopy to R.H.I.C. - PowerPoint PPT PresentationTRANSCRIPT
mike lisa - Femtoscopy in relativistic heavy ion collisions - WPCF Aug 2005 - Kroměříž Czech Republic 1
Femtoscopy in heavy ion collisions:Two decades of progress
Mike Lisa
Ohio State University
An experimentalist’s view of the situation B.Q.M.(*)cf. Bysterský, Chajecki, Chaloupka, Chung, Kisiel, Kniege, Panitkin...
* BQM= Before Quark Matter
mike lisa - Femtoscopy in relativistic heavy ion collisions - WPCF Aug 2005 - Kroměříž Czech Republic 2
Outline
• Relevance of femtoscopy to R.H.I.C.
• Growing activitiies of a (sub)field : 2 decades of systematics
• R(√SNN, b, Npart, A, B, mT, y, , PID)• what information is encoded?• what have we mined so far?• special attention to size and shape
• comments
blastwave
comparison to modelsexperimental details
mike lisa - Femtoscopy in relativistic heavy ion collisions - WPCF Aug 2005 - Kroměříž Czech Republic 3
Spacetime - an annoying bump on the road to Stockholm?
• Non-trivial space-time - the hallmark of rhic• Initial state: dominates further dynamics• Intermediate state: impt element in exciting signals• Final state:
• Geometric structural scale is THE defining feature of QGP
STAR, PRC66 (2002) 034904 STAR, PRL93 (2004) 252301
mike lisa - Femtoscopy in relativistic heavy ion collisions - WPCF Aug 2005 - Kroměříž Czech Republic 4
Spacetime - an annoying bump on the road to Stockholm?
• Non-trivial space-time - the hallmark of rhic• Initial state: dominates further dynamics• Intermediate state: impt element in exciting signals• Final state:
• Geometric structural scale is THE defining feature of QGP
• Temporal scale sensitive to deconfinement transition (?)
QuickTime™ and aTIFF (LZW) decompressor
are needed to see this picture.
Ann.Rev.Nucl.Part.Sci. 46 (1996) 71
mike lisa - Femtoscopy in relativistic heavy ion collisions - WPCF Aug 2005 - Kroměříž Czech Republic 5
A.D. Chacon et al, Phys. Rev. C43 2670 (1991)G. Alexander, Rep. Prog. Phys. 66 481 (2003)
R = 1.2 (fm)•A1/3
Two decades of systematics
• Pion HBT @ Bevalac: “largely confirming nuclear dimensions”• Since 90’s: increasingly detailed understanding and study w/ high stats
)s(HBT
‘85 ‘90 ‘95 ‘00 ‘05
5
10
15
20AGS/SPS/RHIC HBT papers (expt)
Bo
al/
Je
nn
ing
s/G
elb
ke
Heinz/JacakWiedemann/Heinz
Csorgo
To
ma
sik
/Wie
de
ma
nn
“R = 5 fm”
mike lisa - Femtoscopy in relativistic heavy ion collisions - WPCF Aug 2005 - Kroměříž Czech Republic 6
Two decades of systematics
• Pion HBT @ Bevalac: “largely confirming nuclear dimensions”• Since 90’s: increasingly detailed understanding and study w/ high stats
T 1 2 sysˆHBT( ;p , y, b ,b,ms ,m ,A )
r
y
|b|
pT
‘85 ‘90 ‘95 ‘00 ‘05
5
10
15
20AGS/SPS/RHIC HBT papers (expt)
Bo
al/
Je
nn
ing
s/G
elb
ke
Heinz/JacakWiedemann/Heinz
Csorgo
To
ma
sik
/Wie
de
ma
nn
mike lisa - Femtoscopy in relativistic heavy ion collisions - WPCF Aug 2005 - Kroměříž Czech Republic 7
Forget homogeneity regions or fancy stuff.
Do femtoscopic length scales increase when they “should?”
Also• SPS [NA44(‘99),NA49(‘00)]• RHIC [STAR(‘05)]
Repeating most basic sanity check at relativistic energies...
p-p correlations
* big bump small source
mike lisa - Femtoscopy in relativistic heavy ion collisions - WPCF Aug 2005 - Kroměříž Czech Republic 8
ˆT 1b ys2 sHBT( ;p , y, ,b ,m ,m ,A )s φr
•Generalize A1/3 Npart1/3
•not bad @ RHIC!•connection w/ init. size?
Varying initial “source size”
Fixed A+B : vary b
Fixed b : vary A (& B!)
Likely scaling variable: Npart
b
PHENIX, PRL 2004
Au+Au sNN =200 GeV
mike lisa - Femtoscopy in relativistic heavy ion collisions - WPCF Aug 2005 - Kroměříž Czech Republic 9
•Generalize A1/3 Npart1/3
•not bad @ RHIC!•connection w/ init. size?
•Heavy and light data from AGS, SPS, RHIC•~s-ordering in “geometrical” Rlong, Rside
•Mult ~ K(s)*Npart
•source of residual s dep?
• ...Yes! common scaling• final state drives radii, not init. geometry
•(breaks down s < 5 GeV)
ˆT 1b ys2 sHBT( ;p , y, ,b ,m ,m ,A )s φr
PHOBOS
LPSW nucl-ex/0505014
NB: not constant density
mike lisa - Femtoscopy in relativistic heavy ion collisions - WPCF Aug 2005 - Kroměříž Czech Republic 10
We are not alone...
H. Caines (STAR) QM05
Tounsi, Mischke, RedlichNPA715 565 (2003)
H. Caines (STAR) QM05
NA57 (open)STAR (filled)
NA57 (open)STAR (filled)
S. Manly (PHOBOS) QM05
Entropy determines “everything” at bulk level (soft sector) ?
NB: scaling violated s < 4 GeV(as with femtoscopy)
mike lisa - Femtoscopy in relativistic heavy ion collisions - WPCF Aug 2005 - Kroměříž Czech Republic 11
Refinement: chemical effects
• different behaviour below/above AGS
• violates “universal” scaling
• baryon meson dominance
• neglect time/dynamics: gross F.O.
geometry appears determined by
• chemistry
• “universal” mean free path ~ 1 fm (!?)
fm 1~ ⇒==σσ
ρλ
NVff
fm.f.p
2sidelong
2/3)2( RRV f π≡~ FO volume
∑ +=≡i
NNii NNNN πππππ σσσσx-section:
Vf
Nσ
CERES, PRL 90 (2003) 022301
mike lisa - Femtoscopy in relativistic heavy ion collisions - WPCF Aug 2005 - Kroměříž Czech Republic 12
Messages from systematics• AB, |b|, Npart systematics
• sanity check on overall size dependence • final state multiplicity/chemistry determines rough geometry...
c.f. Chajecki - lighter systems
collective/flow-like expansion? probe anisotropically!
...and that geometry is ~2x initial size
mike lisa - Femtoscopy in relativistic heavy ion collisions - WPCF Aug 2005 - Kroměříž Czech Republic 13
Strongly-interacting 6Li released from an asymmetric trapO’Hara, et al, Science 298 2179 (2002)
T ˆ 1 ysb 2 sHBT( ;p , y, b , ,m ,m ,A )s φr
What can we learn?
in-plane-extended
out-of-plane-extended
Teaney, Lauret, & Shuryak nucl-th/0110037
transverse FO shape+ collective velocity evolution time estimate
check independent of RL(pT)
?
mike lisa - Femtoscopy in relativistic heavy ion collisions - WPCF Aug 2005 - Kroměříž Czech Republic 14
• observe the source from all angles
with respect to RP• expect oscillations in HBT radii
big RS
small RS
T ˆ 1 ysb 2 sHBT( ;p , y, b , ,m ,m ,A )s φr
mike lisa - Femtoscopy in relativistic heavy ion collisions - WPCF Aug 2005 - Kroměříž Czech Republic 15
• observe the source from all angles
with respect to RP• expect oscillations in HBT radii
(including “new” cross-terms)
out
side
out
side
R2out-side<0
when pair=135º
T ˆ 1 ysb 2 sHBT( ;p , y, b , ,m ,m ,A )s φr
mike lisa - Femtoscopy in relativistic heavy ion collisions - WPCF Aug 2005 - Kroměříž Czech Republic 16
STAR, PRL93 012301 (2004)Measured final source* shape
* model-dependent, but see Retiere & MAL PRC70 044907 2004
R2out-side<0
when pair=135º
T ˆ 1 ysb 2 sHBT( ;p , y, b , ,m ,m ,A )s φr
ever see that symmetry at ycm ?
mike lisa - Femtoscopy in relativistic heavy ion collisions - WPCF Aug 2005 - Kroměříž Czech Republic 17
STAR, PRL93 012301 (2004)
centralcollisions
mid-centralcollisions
peripheralcollisions
Measured final source* shape
T ˆ 1 ysb 2 sHBT( ;p , y, b , ,m ,m ,A )s φr
* model-dependent, but see Retiere & MAL PRC70 044907 2004
Expected evolution:
mike lisa - Femtoscopy in relativistic heavy ion collisions - WPCF Aug 2005 - Kroměříž Czech Republic 18
Evolution of size and shape - “the rule of two”
€
R s;pT ,y,r b ,AB,φˆ b
,m1,m2( )
initi
al= fin
al
STAR PRL93 012301 (2004)
Initial size/shape estimated by Glauber calculationFinal config according to Retiere & MAL PRC70 044907 2004
~ x2 size increase ~ 1/2 shape reduction
c.f. Chajecki - lighter systems
2x
2y
2x
2y
RR
RR
+−
≡
mike lisa - Femtoscopy in relativistic heavy ion collisions - WPCF Aug 2005 - Kroměříž Czech Republic 19
• non-trivial excitation function• does it make sense? Is it
related to bulk dynamics? YES
sNN (GeV)
(approximately same centrality)
AGS: FO init
RHIC: FO < init
“Anisotropic sanity check”
€
Δ ≈β ⊗ v2 ⊗ τ ???
is relation b/t final and near quantitatively sensible?
mike lisa - Femtoscopy in relativistic heavy ion collisions - WPCF Aug 2005 - Kroměříž Czech Republic 20
A simple estimate – 0 from init and final
0Y,XY,X
t.)O.F()t(
ββ ⋅=→
“radial flow”
P. Kolb, nucl-th/0306081
• BW → βX, βY @ F.O. (βX > βY)
• hydro: flow velocity grows ~ t
• From RL(mT): 0 ~ 9 fm/c
consistent picture• Longer or shorter evolution times
X inconsistent
toy estimate: 0 ~ 0(BW)~ 9 fm/c
• too short to account for expansion??
• Need a real model comparison→ asHBT workable “evolutionary clock” constraint for models MAL ISMD03
mike lisa - Femtoscopy in relativistic heavy ion collisions - WPCF Aug 2005 - Kroměříž Czech Republic 21
Messages from systematics• AB, |b|, Npart systematics
• sanity check on overall size dependence • final state multiplicity/chemistry determines rough geometry...
, |b|, s systematics• sanity check on shape evolution • geometric evolution ~ consistent with collective bulk dynamics (flow)
look for dynamic signatures & substructure
• more than T versus mass• more than spectral shapes• more than v2
• ...flow is defined by space-momentum correlations
only femtoscopy can probe substructureof dynamic bulk behaviour
mike lisa - Femtoscopy in relativistic heavy ion collisions - WPCF Aug 2005 - Kroměříž Czech Republic 22
Spectra
v2
HBT
Flow-dominated“Blast-wave” modelPRC70 044907 (2004)
mike lisa - Femtoscopy in relativistic heavy ion collisions - WPCF Aug 2005 - Kroměříž Czech Republic 23
ˆ 1 2 sysbTHBT( ; , y, b , ,m ,m ,A )ps φr
Kolb & Heinz, QGP3 nucl-th/0305084
Decreasing R(pT)
• usually attributed to collective flow
• flow integral to our understanding of R.H.I.C.; taken for granted
• femtoscopy the only way to confirm x-p correlations – impt check
mike lisa - Femtoscopy in relativistic heavy ion collisions - WPCF Aug 2005 - Kroměříž Czech Republic 24
ˆ 1 2 sysbTHBT( ; , y, b , ,m ,m ,A )ps φr
Decreasing R(pT)
• usually attributed to collective flow
• flow integral to our understanding of R.H.I.C.; taken for granted
• femtoscopy the only way to confirm x-p correlations – impt check
Non-flow possibilities• cooling, thermally (not collectively)
expanding source
• combo of x-t and t-p correlationsearly times: small, hot source
late times: large, cool source
mike lisa - Femtoscopy in relativistic heavy ion collisions - WPCF Aug 2005 - Kroměříž Czech Republic 25
ˆ 1 2 sysbTHBT( ; , y, b , ,m ,m ,A )ps φr
Decreasing R(pT)
• usually attributed to collective flow
• flow integral to our understanding of R.H.I.C.; taken for granted
• femtoscopy the only way to confirm x-p correlations – impt check
Non-flow possibilities• cooling, thermally (not collectively)
expanding source
• combo of x-t and t-p correlations
MAL et al, PRC49 2788 (1994)
mike lisa - Femtoscopy in relativistic heavy ion collisions - WPCF Aug 2005 - Kroměříž Czech Republic 26
ˆ 1 2 sysbTHBT( ; , y, b , ,m ,m ,A )ps φr
Decreasing R(pT)
• usually attributed to collective flow
• flow integral to our understanding of R.H.I.C.; taken for granted
• femtoscopy the only way to confirm x-p correlations – impt check
Non-flow possibilities• cooling, thermally (not collectively)
expanding source
• combo of x-t and t-p correlations
• hot core surrounded by cool shell
• important ingredient of Buda-Lund hydro picturee.g. Csörgő & LörstadPRC54 1390 (1996)
mike lisa - Femtoscopy in relativistic heavy ion collisions - WPCF Aug 2005 - Kroměříž Czech Republic 27
ˆ 1 2 sysbTHBT( ; , y, b , ,m ,m ,A )ps φr
Decreasing R(pT)
• usually attributed to collective flow
• flow integral to our understanding of R.H.I.C.; taken for granted
• femtoscopy the only way to confirm x-p correlations – impt check
Non-flow possibilities• cooling, thermally (not collectively)
expanding source
• combo of x-t and t-p correlations
• hot core surrounded by cool shell
• important ingredient of Buda-Lund hydro picturee.g. Csörgő & LörstadPRC54 1390 (1996)
t
Each scenario generatesx-p correlations but…
x2-p correlation: yesx-p correlation: yes
x2-p correlation: yesx-p correlation: no
x2-p correlation: yesx-p correlation: no
mike lisa - Femtoscopy in relativistic heavy ion collisions - WPCF Aug 2005 - Kroměříž Czech Republic 28
ˆ 1 2 sysbTHBT( ; , y, b , ,m ,m ,A )ps φr
• flow-dominated “models” can reproduce soft-sector x-space observables
• imply short timescales
• however, are we on the right track? [flow]• puzzles? check your assumptions!• look for flow’s “special signature”
x-p correlation
• In flow pictures, low-pT particles emitted closer to source’s center (along “out”)
• non-identical particle correlations(FSI at low Δv) probe:
(x1-x2)2 (as does HBT)
x1-x2
Csanád, Csörgő, Lörstad nucl-th/0311102 and nucl-th/0310040
[click for more details on non-id correlations]
F. Retiere & MAL, nucl-th/0312024
pT
βT
K
p
π
mike lisa - Femtoscopy in relativistic heavy ion collisions - WPCF Aug 2005 - Kroměříž Czech Republic 29
ˆT 2 sysb 1HBT( ;p , y, b , m ,m, ,A )s φr
• In flow pictures, low-pT particles emitted closer to source’s center (along “out”)
• non-identical particle correlations(FSI at low Δv) probe:
(x1-x2)2 (as does HBT)
x1-x2
• extracted shift in emission point x1-x2 consistent w/ flow-dominated blastwave
A. Kisiel (STAR) QM04
Δx
(fm
)Δ
x (
fm)
βT βT
QuickTime™ and aTIFF (LZW) decompressor
are needed to see this picture.
QM02
mike lisa - Femtoscopy in relativistic heavy ion collisions - WPCF Aug 2005 - Kroměříž Czech Republic 30
RHIC femtoscopy with wide variety of particle species
π+ π- K+ K- K0S p p
π+
π-
- K+
K-
- - K0S
p
p
R(√SNN, b, Npart, A, B, mT, y, , PID1, PID2)
= prelim or final result available
mike lisa - Femtoscopy in relativistic heavy ion collisions - WPCF Aug 2005 - Kroměříž Czech Republic 31
Strong flow confirmed by all expts...
€
R s;pT ,y,r b ,AB,φˆ b
,m1,m2( )LPSW(05) - DATA in color-- experimentalist’s plot
what agreement!! (what agreement?)
mike lisa - Femtoscopy in relativistic heavy ion collisions - WPCF Aug 2005 - Kroměříž Czech Republic 32
€
R s;pT ,y,r b ,AB,φˆ b
,m1,m2( )
€
R i mT( ) =′ R i
mTα i
Strong flow confirmed by all expts...
Central (~10%) AuAu (PbPb) collisions at y~0
mike lisa - Femtoscopy in relativistic heavy ion collisions - WPCF Aug 2005 - Kroměříž Czech Republic 33
Another implication of strong flow: ~mT scaling
€
R s;pT ,y,r b ,AB,φˆ b
,m1,m2( )
mike lisa - Femtoscopy in relativistic heavy ion collisions - WPCF Aug 2005 - Kroměříž Czech Republic 34
Motivation Formalism Experiment Trends Models
Some longitudinal systematics
€
R s;pT ,y,r b ,AB,φˆ b
,m1,m2( )
cons
istent w
ith bo
ost-inva
riance
QuickTime™ and aTIFF (LZW) decompressor
are needed to see this picture.
inconsis
tent with
boost-inva
riance
PHOBOS nucl-ex/0410022
mike lisa - Femtoscopy in relativistic heavy ion collisions - WPCF Aug 2005 - Kroměříž Czech Republic 35
beam
“Dynamic” BI without “Chemical” BI ?Only femtoscopy can tell!
mike lisa - Femtoscopy in relativistic heavy ion collisions - WPCF Aug 2005 - Kroměříž Czech Republic 36
beam
“Dynamic” BI without “Chemical” BI ?Only femtoscopy can tell!
mike lisa - Femtoscopy in relativistic heavy ion collisions - WPCF Aug 2005 - Kroměříž Czech Republic 37
qX (GeV/c) qY (GeV/c) qZ (GeV/c)
C
E877, Miskowiec CRIS’98 nucl-ex/9808003
p-π-
Greater detail - π-p correlations @ AGS
€
R s;pT ,y,r b ,AB,φˆ b
,m1,m2( )
QuickTime™ and aTIFF (LZW) decompressor
are needed to see this picture.
sizes and offsets in impact parameterand longitudinal directions
b
z
10 fm
mike lisa - Femtoscopy in relativistic heavy ion collisions - WPCF Aug 2005 - Kroměříž Czech Republic 38
Comments• massive systematic program provides tremendous geometric detail
• each element reasonable by itself not really “puzzling.”
• “critical mass” in the femtoscopy community• Related, but not in my talk: important new directions [talks @ WPCF]
• moments analysis• imaging• continued emphasis on non-identical particle correlations• connection to “elementary” systems - communication “across lines”
• Important puzzles beyond central Au+Au at top energy
• Ignoring femtoscopy to pursue “perfection” is unjustified• Space-time is the defining feature of R.H.I.C.• Femtoscopy does measure space-time• The measurements are sensitive to underlying physics
We are working on the many slowly crawling ants...We are working on the many slowly crawling ants...
... don’t give up your dreams!!... don’t give up your dreams!!