Size Matters Spacetime geometry in subatomic collisions

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MA Lisa - Sambamurti Lecture, BNL - 28 J ul 2004 1 Size Matters Spacetime geometry in subatomic collisions Mike Lisa The Ohio State University What is the strong force? Why must we understand it? How can we study it? What tools do we use? Why size matters, & what it’s told us

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What is the strong force? Why must we understand it? How can we study it? What tools do we use? Why size matters, & what it’s told us. Size Matters Spacetime geometry in subatomic collisions. Mike Lisa The Ohio State University. Disclaimer. many of the concepts I will present are - PowerPoint PPT Presentation

Transcript of Size Matters Spacetime geometry in subatomic collisions

Page 1: Size Matters Spacetime geometry in subatomic collisions

MA Lisa - Sambamurti Lecture, BNL - 28 Jul 2004 1

Size MattersSpacetime geometry in subatomic

collisions

Mike Lisa

The Ohio State University

What is the strong force?Why must we understand it?

How can we study it?

What tools do we use?

Why size matters, &what it’s told us

Page 2: Size Matters Spacetime geometry in subatomic collisions

MA Lisa - Sambamurti Lecture, BNL - 28 Jul 2004 2

Disclaimermany of the concepts I will present are

“works in very active progress”

an unavoidable consequence of exciting, cutting edge science

Page 3: Size Matters Spacetime geometry in subatomic collisions

MA Lisa - Sambamurti Lecture, BNL - 28 Jul 2004 3

Forces and structures in Nature1) Gravity• one “charge” (mass)• force decreases with distance

m1 m2

2) Electric (& Magnetic)• two “charges” (+/-)• force decreases with distance

+ -

+ +

Atom

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MA Lisa - Sambamurti Lecture, BNL - 28 Jul 2004 4

Atomic nuclei and the “nuclear” force

Nuclei composed of:• protons (+ electric charge)• neutrons (no electric charge)

Does not blow up!? “nuclear force”• overcomes electrical repulsion• determines nuclear reactions

(stellar burning, bombs…)

• arises from fundamental strong force (#3)• acts on color charge of quarks

proton

neutron

quark

Page 5: Size Matters Spacetime geometry in subatomic collisions

MA Lisa - Sambamurti Lecture, BNL - 28 Jul 2004 5

Strong color fieldEnergy grows with separation !!!E=mc2 !

An analogy… and a difference!to study structure of an atom…

“white” proton

…separate constituents

Imagine our understanding of atoms or QED if we could not isolate charged objects!!

nucleus

electron

quark

quark-antiquark paircreated from vacuum

“white” proton(confined quarks)

“white” 0

(confined quarks)

Confinement: fundamental & crucial (but not understood!) feature of strong force- colored objects (quarks) have energy in normal vacuum

neutral atom

To understand the strong force and the phenomenon of confinement:Create and study a system of deconfined colored quarks (and gluons)

Page 6: Size Matters Spacetime geometry in subatomic collisions

MA Lisa - Sambamurti Lecture, BNL - 28 Jul 2004 6

Generating a deconfined state

Nuclear Matter(confined)

Hadronic Matter(confined)

Quark Gluon Plasmadeconfined !

Present understanding of Quantum Chromodynamics (QCD)• heating• compression deconfined color matter !

Mike Lisa
Would be very cool to “reverse” the animation on the heating/compression slide, showing cooling/decompression.The point would be that even if we went into a QGP, the system would rapidly rehadronize (a process we don’t understand, but must, if we are to understand the strong force) into a hadronic system– hadrons in / hadrons out we will not “see” the QGP, but must infer it from hadronic patterns in the final state
Page 7: Size Matters Spacetime geometry in subatomic collisions

MA Lisa - Sambamurti Lecture, BNL - 28 Jul 2004 7

Expectations from Lattice QCD/T4 ~ # degrees of freedom

confined:few d.o.f.

deconfined:many d.o.f.

TC ≈ 173 MeV ≈ 21012 K ≈ 130,000T[Sun’s core]

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MA Lisa - Sambamurti Lecture, BNL - 28 Jul 2004 8

The phase diagram of QCDTe

mpe

ratu

re

baryon density

Neutron stars

Early universe

nucleinucleon gas

hadron gascolour

superconductor

quark-gluon plasmaTc

0

critical point ?

vacuum

CFL

Page 9: Size Matters Spacetime geometry in subatomic collisions

MA Lisa - Sambamurti Lecture, BNL - 28 Jul 2004 9

The phase diagram of water

Analogous graphs• superfluids• superconductors• metal/insulator• …

Page 10: Size Matters Spacetime geometry in subatomic collisions

MA Lisa - Sambamurti Lecture, BNL - 28 Jul 2004 10

Bulk Matter• We must create/compress/heat a bulk (geometrically large) system

– freeze/melt a single H20 molecule?

– fundamental distinction from particle physics

• Only achievable through collisions of the heaviest nuclei (Au, Pb) at the highest available energy– at Relativistic Heavy Ion Collider (RHIC)

1000’s ofparticles producedin each collision

Page 11: Size Matters Spacetime geometry in subatomic collisions

MA Lisa - Sambamurti Lecture, BNL - 28 Jul 2004 11

RHIC BRAHMSPHOBOSPHENIX

STAR

AGS

TANDEMS

Relativistic Heavy Ion Collider (RHIC)

1 km

v = 0.99995c = 186,000 miles/sec

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MA Lisa - Sambamurti Lecture, BNL - 28 Jul 2004 12

RHIC BRAHMSPHOBOSPHENIX

STAR

AGS

TANDEMS

Relativistic Heavy Ion Collider (RHIC)

PHENIX~ 500 collaborators

Page 13: Size Matters Spacetime geometry in subatomic collisions

MA Lisa - Sambamurti Lecture, BNL - 28 Jul 2004 13

RHIC BRAHMSPHOBOSPHENIX

STAR

AGS

TANDEMS

Relativistic Heavy Ion Collider (RHIC)

STAR ~500 Collaborators

Page 14: Size Matters Spacetime geometry in subatomic collisions

MA Lisa - Sambamurti Lecture, BNL - 28 Jul 2004 14

The STAR ExperimentSTAR: Solenoidal Tracker at RHIC

multipurpose detector system for hadronic measurements

• large coverage (geometrical acceptance)• tracking of charged particles in high multiplicity environment• measure correlations of observables• study of hard processes (jet physics)

Solenoidal Tracker At RHIC

goal: track “all” charged hadrons (bags of quarks) emitted in each collision

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MA Lisa - Sambamurti Lecture, BNL - 28 Jul 2004

15

Operation of a Time Projection Chamber

SCA/ADCDAQ

Copper pads ~ 1cm2

Amplifying and digitizing electronics connected to each pad

Anode wires with +HVsitting ~5 mm above pads

Charged particle fliesthru TPC gas…

..generating a clusterof liberated electrons

Electricfield

“Avalanche” as electronsapproach anode wire...

..capacitively inducinga signal on nearby pads... ..which is amplified, digitized, and recorded for later analysis

V

t AD

Cbucket #

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MA Lisa - Sambamurti Lecture, BNL - 28 Jul 2004 16

One collision seen by STAR

TPCMomentum determined by trackcurvature in magnetic field…

…and by direction relative to beam

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MA Lisa - Sambamurti Lecture, BNL - 28 Jul 2004 17

“RHIC is big”

as seen by the Landsat-4 satellite…

• big facility• big detectors• big collaborations• “big” collisions

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MA Lisa - Sambamurti Lecture, BNL - 28 Jul 2004 18

“Big” and “Small” – in meters

100 106 1012 1018 102410-610-1210-18

1,000,000,000,000,000,000,000,000 m

0.000000000000000001 m

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MA Lisa - Sambamurti Lecture, BNL - 28 Jul 2004 19

“Short” and “long” – in seconds

Today’s lecture

100 106 1012 1018 102410-610-1210-1810-24

as many yoctoseconds (10-24 s ~ 3 fm/c) in a secondas seconds in 10 thousand trillion years

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MA Lisa - Sambamurti Lecture, BNL - 28 Jul 2004 20

Particle momentum from tracking…

… how to get particle space-timeinformation??

Page 21: Size Matters Spacetime geometry in subatomic collisions

MA Lisa - Sambamurti Lecture, BNL - 28 Jul 2004 21

Impact parameter & Reaction plane

Impact parameter vector b : beam direction connects centers of colliding nuclei

b = 0 “central collision”many particles produced

“peripheral collision”fewer particles produced

b

Page 22: Size Matters Spacetime geometry in subatomic collisions

MA Lisa - Sambamurti Lecture, BNL - 28 Jul 2004 22

Impact parameter & Reaction plane

Impact parameter vector b : beam direction connects centers of colliding nuclei

b = 0 “central collision”many particles produced

“peripheral collision”fewer particles produced

b

b

Reaction plane:

spanned by beam direction and b

Mike Lisa
Could point out that the vector b cannot be "controlled" by, like, aiming the beam or something like that. We measure all collisions, and collision-by-collision we estimate magnitude and direction of b.
Page 23: Size Matters Spacetime geometry in subatomic collisions

MA Lisa - Sambamurti Lecture, BNL - 28 Jul 2004 23

How do semi-central collisions evolve?

b

1) Superposition of independent p+p:momenta pointed at randomrelative to reaction plane

Page 24: Size Matters Spacetime geometry in subatomic collisions

MA Lisa - Sambamurti Lecture, BNL - 28 Jul 2004 24

How do semi-central collisions evolve?

b

1) Superposition of independent p+p:

2) Evolution as a bulk system

momenta pointed at randomrelative to reaction plane

highdensity / pressure

at center

“zero” pressurein surrounding vacuum

Pressure gradients (larger in-plane) push bulk “out” “flow”

more, faster particles seen in-plane

Mike Lisa
in practice with Uli and Mercedes, took 1/2 hour to get to this slide
Page 25: Size Matters Spacetime geometry in subatomic collisions

MA Lisa - Sambamurti Lecture, BNL - 28 Jul 2004 25

How do semi-central collisions evolve?

1) Superposition of independent p+p:

2) Evolution as a bulk system

momenta pointed at randomrelative to reaction plane

Pressure gradients (larger in-plane) push bulk “out” “flow”

more, faster particles seen in-plane

N

-RP (rad)0 /2 /4 3/4

N

-RP (rad)0 /2 /4 3/4

Mike Lisa
in practice with Uli and Mercedes, took 1/2 hour to get to this slide
Page 26: Size Matters Spacetime geometry in subatomic collisions

MA Lisa - Sambamurti Lecture, BNL - 28 Jul 2004 26

Azimuthal distributions at RHICSTAR, PRL90 032301 (2003)

b ≈ 4 fm

“central” collisions

b ≈ 6.5 fm

midcentral collisions

Page 27: Size Matters Spacetime geometry in subatomic collisions

MA Lisa - Sambamurti Lecture, BNL - 28 Jul 2004 27

Azimuthal distributions at RHICSTAR, PRL90 032301 (2003)

b ≈ 4 fmb ≈ 6.5 fmb ≈ 10 fm

peripheral collisions

Page 28: Size Matters Spacetime geometry in subatomic collisions

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Elliptic flow – collectivity& sensitivity to early system

STAR, PRL90 032301 (2003)

“v2”

“Elliptic flow”• evidence of

collective motion

• quantified by v2

• geometrical anisotropy momentum anisotropy

• sensitive to early pressure

• evidence for• early thermalization• QGP in early stage

Hydrodynamiccalculation ofsystem evolution

Page 29: Size Matters Spacetime geometry in subatomic collisions

MA Lisa - Sambamurti Lecture, BNL - 28 Jul 2004 29

A more direct handle?• elliptic flow (v2) and other measurements (not discussed)

evidence towards QGP at RHIC– indirect connection to geometry

• Are there more direct handles on the space-time geometry of collisions?

– yes ! Even at the 10-15 m / 10-23 s scale !• What can they tell us about the QGP and system evolution?

Warning: some quantum mechanics coming(feel free to concentrate on “bottom line”) !!

Page 30: Size Matters Spacetime geometry in subatomic collisions

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222111 p)xr(i22

p)xr(i11T e)p,x(Ue)p,x(U

probing source geometry through interferometry

12 ppq

2

21

2121 )q(~1

)p(P)p(P)p,p(P)p,p(C C

(Qin

v)

Qinv (GeV/c)

1

2

0.05 0.10

Width ~ 1/R

Measurable! F.T. of pion source

)xx(iq2

*21

*1T

*T

21e1UUUU

Creation probability (x,p) = U*U5 fm

1 m source

(x)

r1

r2

x1

x2

{2

1

}e)p,x(Ue)p,x(U 212121 p)xr(i21

p)xr(i12

p1

p2

The Bottom line…if a pion is emitted, it is more likely to emit another

pion with very similar momentum if the source is small

experimentally measuring this enhanced probability: quite challenging

Page 31: Size Matters Spacetime geometry in subatomic collisions

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Correlation functions for different colliding systems

C2(Q

inv)

Qinv (GeV/c)

STAR preliminary p+pR ~ 1 fm

d+AuR ~ 2 fm

Au+AuR ~ 6 fm

Different colliding systems studied at RHIC

Interferometry probes the smallest scales ever measured !

Page 32: Size Matters Spacetime geometry in subatomic collisions

MA Lisa - Sambamurti Lecture, BNL - 28 Jul 2004 32

beam directio

n

More detailed geometryRelative momentum between pions is a vector can extract 3D shape information

1 2q p p

p2

p1

q1 2K p p

R long

RsideRout

Rlong – along beam directionRout – along “line of sight”Rside – “line of sight”

Page 33: Size Matters Spacetime geometry in subatomic collisions

MA Lisa - Sambamurti Lecture, BNL - 28 Jul 2004 33

• “observe” the source from all angles relative to the reaction plane

• expect oscillations in radii for non-round sources

big RSIDE

small RSIDE

Source shapeR

SID

E

-RP (rad)0 /2 /4 3/4

reaction plane

Page 34: Size Matters Spacetime geometry in subatomic collisions

MA Lisa - Sambamurti Lecture, BNL - 28 Jul 2004 34

STAR, PRL93 012301 (2004)

Measured final source shapecentral

collisions

mid-centralcollisions

peripheralcollisions

Expected evolution:

Page 35: Size Matters Spacetime geometry in subatomic collisions

MA Lisa - Sambamurti Lecture, BNL - 28 Jul 2004 35

More informationRelative momentum between pions is a vector can extract 3D shape information

1 2q p p

p2

p1 1 2K p p

Rout

Rlong – along beam directionRout – along “line of sight”Rside – “line of sight”

Rside

study as K grows…

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MA Lisa - Sambamurti Lecture, BNL - 28 Jul 2004 36

Why do the radii fallwith increasing momentum ??

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Why do the radii fallwith increasing momentum ??

It’s collective flow !!

Direct geometrical/dynamical evidencefor bulk behaviour!!!

Amount of flow consistent with p-space

Page 38: Size Matters Spacetime geometry in subatomic collisions

MA Lisa - Sambamurti Lecture, BNL - 28 Jul 2004 38

Timescales• Evolution of source shape

– suggests system lifetime is shorter than otherwise-successful theory predicts

• Is there a more direct handle on timescales?

Page 39: Size Matters Spacetime geometry in subatomic collisions

MA Lisa - Sambamurti Lecture, BNL - 28 Jul 2004 39

Disintegration timescaleRelative momentum between pions is a vector can extract 3D shape information

1 2q p p

p2

p1

q1 2K p p

Rout

Rlong – along beam directionRout – along “line of sight”Rside – “line of sight”

Rside

increases with emission timescale

OUT

SIDE

RR

Page 40: Size Matters Spacetime geometry in subatomic collisions

MA Lisa - Sambamurti Lecture, BNL - 28 Jul 2004 40

Disintegration timescale - expectation

3D 1-fluid Hydrodynamics Rischke & Gyulassy, NPA 608, 479 (1996)

withtransition

withtransition

“” “”

Long-standing favorite signature of QGP:• increase in , ROUT/RSIDE due to deconfinement confinement transition

• expected to “turn on” as QGP energy threshold is reached

Page 41: Size Matters Spacetime geometry in subatomic collisions

MA Lisa - Sambamurti Lecture, BNL - 28 Jul 2004 41

Disintegration timescale - observation

4

6

8

4

6

8

1.0

1.25

1.5R

O (f

m)

RS (f

m)

RO

/ R

S

increasing collision energy

RHIC

• no threshold effect seen

• RO/RS ~ 1

Page 42: Size Matters Spacetime geometry in subatomic collisions

MA Lisa - Sambamurti Lecture, BNL - 28 Jul 2004 42

Disintegration timescale - observation

• no threshold effect seen

• RO/RS ~ 1

• toy model calculations suggest very short timescales

Page 43: Size Matters Spacetime geometry in subatomic collisions

MA Lisa - Sambamurti Lecture, BNL - 28 Jul 2004 43

Disintegration timescale - observation

PCM & clust. hadronization

NFD

NFD & hadronic TM

PCM & hadronic TM

CYM & LGT

string & hadronic TM

N()

Heinz & Kolb, hep-ph/0204061

• no threshold effect seen

• RO/RS ~ 1

• toy model calculations suggest very short timescales• rapid, explosive evolution• too explosive for “real” models

which explain all other data

An important space-time“puzzle” at RHIC

- actively under study

Page 44: Size Matters Spacetime geometry in subatomic collisions

MA Lisa - Sambamurti Lecture, BNL - 28 Jul 2004 44

Summary• Crucial feature of strong force: confinement

– study bulk system of deconfined quarks

• bulk system is created in heavy ion collisions at RHIC !

• geometric (v2) and other measurements strongly suggest bulk deconfined matter !

• We can access the smallest size and time scales through quantum-mechanical mechanism of interferometry

– close investigation of space-time: our understanding of the hot, dense system evolution is incomplete

• Focusing on holes in understanding-- key to scientific progress– these are exciting times in our study of the least well-understood force

in Nature … and clearly size matters in this quest !