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Future prospects for NA61 heavy ions: rare observables Connecting to high-energy (RHIC) results M. van Leeuwen, Utrecht University and the NA61 collaboration Workshop: New Opportunities in the Physics Landscape at CERN 11-14 May 2009

Future prospects for NA61 heavy ions: rare observables

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Future prospects for NA61 heavy ions: rare observables. Connecting to high-energy (RHIC) results. M. van Leeuwen, Utrecht University and the NA61 collaboration. Workshop: New Opportunities in the Physics Landscape at CERN 11-14 May 2009. Motivation. - PowerPoint PPT Presentation

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Page 1: Future prospects for NA61 heavy ions: rare observables

Future prospects for NA61 heavy ions: rare observables

Connecting to high-energy (RHIC) results

M. van Leeuwen, Utrecht Universityand the NA61 collaboration

Workshop:New Opportunities in the Physics Landscape at CERN11-14 May 2009

Page 2: Future prospects for NA61 heavy ions: rare observables

2M. van Leeuwen, Future prospects for NA61: rare probes

Motivation

• Heavy ion collisions: study strong interactions bulk matter

– Identify phase transition to Quark-Gluon-Plasma

• Pure bulk = soft QCD, theoretically difficult

• Hard-soft interplay studied at RHIC shows many unexpected results – do these effects exist at SPS energies?

– Can we ‘switch off’ some effects – transition ?

Page 3: Future prospects for NA61 heavy ions: rare observables

3M. van Leeuwen, Future prospects for NA61: rare probes

Jet-like di-hadron correlations at RHIC

At high pT > 4-6 GeV: Clear di-jet signatureAway-side suppression due to energy loss

associated

trigger

8 < pTtrig < 15 GeV

pTassoc > 3 GeV

Use di-hadron correlations to probe the jet-structure in p+p, d+Au

Near side Away side

and Au+Au

Combinatorialbackground

STAR, PRL97, 162301

p+p event display

Page 4: Future prospects for NA61 heavy ions: rare observables

4M. van Leeuwen, Future prospects for NA61: rare probes

Lowering pT: bulk response?

3.0 < pT

trig < 4.0 GeV/c

1.3 < pT

assoc < 1.8 GeV/c

Near sideEnhanced yield in Au+Au

Away-side:Strong broadening in central Au+Au

‘Dip’ at =

STAR, M. Horner, M. van Leeuwen, et al

Au+Au 0-10%STAR preliminary

Jet-like peak

`Ridge’: associated yield at large dN/d approx. independent of

d+Au, 200 GeV

Large modifications of di-hadron structure at intermediate pT

Modified fragmentation? Bulk response?

ST

AR

, Putschke et al

3 < pt,trigger < 4 GeVpt,assoc. > 2 GeV

Page 5: Future prospects for NA61 heavy ions: rare observables

5M. van Leeuwen, Future prospects for NA61: rare probes

Comparing SPS and RHIC

SPS full energy: di-hadron structure similar to RHIC yields lower lower ‘jet’ energy

M. S

zuba, Hot Q

uarks 2008

CERES, NA49 158 AGeV

Page 6: Future prospects for NA61 heavy ions: rare observables

6M. van Leeuwen, Future prospects for NA61: rare probes

Energy dependence of di-hadron correlations at SPS

Qualitative change from low to high energy: from near-side dip to near-side peak

Clear turn-on as a function of energy. What is the mechanism?

M. S

zuba, HQ

08

New data needed to study , pT-dependence, above and below transition

40 AGeV 20 AGeV

Page 7: Future prospects for NA61 heavy ions: rare observables

7M. van Leeuwen, Future prospects for NA61: rare probes

Charm production at RHIC

Low pT, RAA~ 1Total cross section scales with Ncoll as expected

Suppression at high-pt: charm interacts with medium

Does charm thermalise? Measure charm spectra at low pt, v2

Will be measured at RHIC (STAR, PHENIX upgrades)and LHC (ALICE, ...)Can we measure this at SPS? Thermalised charm at SPS?

ST

AR

, PR

L 9

8 (2

00

7) 1

92

30

1

p+pTcoll

Au+AuTAA |dpdNN

|dpdN=R

//

Page 8: Future prospects for NA61 heavy ions: rare observables

8M. van Leeuwen, Future prospects for NA61: rare probes

Charm with NA61?

NA49: D0 K 3.8M events

Would need ~300M events (300 days running) for 1 Need vertex detector to measure D0, pT spectra, v2

Ph

ys.Re

v.C7

3:0

34

91

0,2

00

6

N(D0+D0) = -0.36 0.74 per eventN(D0+D0) < 1.5 per event (C.L. 98%)

NA61: c + -

μb4.13.15.9 ppcc

EPJ C59, 607

N(D0+D0) expected: ~ 0.11 per central event

e.g. 20M central events gives 80k D0 K

Page 9: Future prospects for NA61 heavy ions: rare observables

9M. van Leeuwen, Future prospects for NA61: rare probes

Technology candidate: GOSSIP

GridPix/InGridGOSSIP

Gas on Slimmed Silicon Pixels

H. van der Graaf et al., NIKHEF

Pixel size 55 x 55 m+ time

Use time-dependence toimage track in gas layer

Thin, precise and cheap !

Gas amplification + pixel readout

Page 10: Future prospects for NA61 heavy ions: rare observables

10M. van Leeuwen, Future prospects for NA61: rare probes

Occupancy for vertex detector

Central Pb+Pb at 158 AGeV

Hits at z = 10 cm2-track distance

For y < 4 ~ R > 0.3 cm, two-track distance ~ 300 m

z = 10 cm safe choice for first plane

ycms < 1

Page 11: Future prospects for NA61 heavy ions: rare observables

11M. van Leeuwen, Future prospects for NA61: rare probes

Vertex resolution with vertex detector

Decay distance along beam Decay length resolution

158 AGeV collisions Including Mult scatt ~600 m Si per plane

Geometry:6 planes, 10, 15 … 40 cm

Lorentz boost: large decay lengths (mm scale)

Looks promising: typical decay length >> resolution

Page 12: Future prospects for NA61 heavy ions: rare observables

12M. van Leeuwen, Future prospects for NA61: rare probes

Summary of proposal

• 2 runs of NA61 ~10 weeks, 70M events(after baseline heavy ion program, 2014+)

– Highest SPS energy: 158 AGeV

– Low energy: 20/30 AGeV

• Measurement 1: jet-like di-hadron structure– Peak-dip transition, explore pT-dependence, - structure –

connection to bulk response effects at RHIC

• Measurement 2: charm production– Need vertex detector

– Measure yield, pT spectra (radial flow) and v2

Page 13: Future prospects for NA61 heavy ions: rare observables

13M. van Leeuwen, Future prospects for NA61: rare probes

Reflections about EXChALIBUR, the exclusive 4 detector for EXCLUSIVE measurements of hadronic interactions

needed for deeper understanding of QCD

G. Vesztergombi

New opportunities in the physics landscape at CERN

11/13 May ’09 Geneva

Presented on the Workshop:

Page 14: Future prospects for NA61 heavy ions: rare observables

14M. van Leeuwen, Future prospects for NA61: rare probes

Towards a 4 detector?

• Qualitative step forward in hadron production experiments

• Goal: address unsolved issues from ISR era:– Cronin effect – connection to long range correlations?– Changeover/interplay soft-hard production – emergence of

jetty structure– Baryon formation/transfer– Others?

Concept: a large acceptance detector for ‘all’ particles (EM + charged hadrons + neutral hadrons) to perform exclusive

measurements of hadron production at the SPS energy range.

SPS has the potential to address many of these issues: wide energy range and choice of beams to narrow down the ‘model space’

Page 15: Future prospects for NA61 heavy ions: rare observables

15M. van Leeuwen, Future prospects for NA61: rare probes

EXChALIBUR

Dipol Magnetic Field (1 Tesla)

B-ImCalo

B-ImCalo

F-PhT

B-PhT

B-PhT

B-Si-Box

F-S

i-Box

B-Si-Box

B-ImCaloACT

Conceptual lay-out of a possible new 4 detector system

Page 16: Future prospects for NA61 heavy ions: rare observables

16M. van Leeuwen, Future prospects for NA61: rare probes

DIAMOND-TPC

Ohmic contact

Pixel readout

Vdrift = 5 micron/s 1 GHz sampling : 1 micron resolution

IDEAL case: no limit on money and progress of CVD technology

1 cm

1 million10*10 pixels on 1cm*1cm Active

Carbon

Target

E

Carbon target, with full measurement of recoils

Page 17: Future prospects for NA61 heavy ions: rare observables

17M. van Leeuwen, Future prospects for NA61: rare probes

Si-Box

Barrel

Front

ACT 5 SDD layers

Low-momentum and vertex tracking

Page 18: Future prospects for NA61 heavy ions: rare observables

18M. van Leeuwen, Future prospects for NA61: rare probes

PhotonTracker

Standard TPC with W-strips in 1Tesla magnetic field

25 cm cells with 0.8mm = 0.25 Xo W-converters where interaction length=30Xo

20 cells : total 5 Xo and only 0.17 interaction length, NOEFFECT for p, K,

Top view

p, K ,

e+

e-

Unchanged dE/dx for hadrons

Gradually developing EM shower

0.25 Xo, 0.008 PhT

Page 19: Future prospects for NA61 heavy ions: rare observables

19M. van Leeuwen, Future prospects for NA61: rare probes

Impact Calorimeter

p

n

20cm 20cm 20cm 20cm 20cm20cm 20cm 20cm

20 cm Polyethylene: 0.47 Xo and 0.25 interaction length16 periods gives total length 6.4 m with 4 interaction length

TPC pad readout pattern is optimized for local vertex reconstruction

Showers from charged hadrons can be used for calibration.

ImCalo

TPC with polyethylene hadron interaction volumes

Page 20: Future prospects for NA61 heavy ions: rare observables

20M. van Leeuwen, Future prospects for NA61: rare probes

DAQ

Beam intensity: 105 - 106 particle/s , spot size sigma = 2 mm

Interaction rate: 100 – 1000 ev/s

Each channel is continuously read out by a token ring.

Parallel processing by SIMD farm

Each hit has LOCALITY (XY) + TIME(t) + AMPLITUDE(Energy) Recorded.

DATA DRIVEN System: Single hits are looking for association with others relying on locality and time.

Successfull associations create OBJECTs. Simpler objects are building up higher classes….

Unbiased sampling with trigger-less read out

Page 21: Future prospects for NA61 heavy ions: rare observables

21M. van Leeuwen, Future prospects for NA61: rare probes

Due to the fact that in this region the multiplicities are still relatively modest one have more chance to identify characteristic features.Bohr was using the spectral lines of Hydrogen and not the ones of Lead.

In short: We should find "the Lyman and Balmer series" for QCD. Due to the fact that QCD is so many times more complicated than QED we need EXA-Bytes instead of the few Bytes of Bohr.

The complication is mainly arising from the fact that the hadrons areextended objects in space in contrast to point-like leptons. In thissituation one should grab any possibility to collect new information whichcan provide insight into the space-time evolution of this complex system.

The aim of this proposal calls for not an immediate concrete action, butto initiate the discussion for a longer range project which could lead todefinite design of a dedicated exclusive experiment in 5 years from now.

It is clear, that exclusive experiments have more information than the inclusive ones, what is not clear, is this information enough for a breakthrough.

Pessimists can say: There is no such information.But I ask: Please prove it without trying to measure it!

If you are interested in more scientific and technical details. please contact: [email protected]

Page 22: Future prospects for NA61 heavy ions: rare observables

22M. van Leeuwen, Future prospects for NA61: rare probes

Extra slides

Page 23: Future prospects for NA61 heavy ions: rare observables

23M. van Leeuwen, Future prospects for NA61: rare probes

Charm production at RHIC

PHENIX, PRL 98 (2007) 172301

Total cross section scales with Ncoll

-- as expected

J. Dunlop, QM09

pQ

CD

ex

pe

cta

tion

p+p Au+Au

cc/

Nco

ll [m

b]

Remove!

Page 24: Future prospects for NA61 heavy ions: rare observables

24M. van Leeuwen, Future prospects for NA61: rare probes

Lowering pT: gluon fragments/bulk response

3 < pt,trigger < 4 GeVpt,assoc. > 2 GeV

Au+Au 0-10%STAR preliminaryassociated

trigger

Jet-like peak

`Ridge’: associated yield at large dN/d approx. independent of

Strong - asymmetry suggests effect of longitudinal flow or underlying event

Long. flow Long. flow

J. Putschke, M. van Leeuwen, et al

d+Au, 200 GeV

Page 25: Future prospects for NA61 heavy ions: rare observables

25M. van Leeuwen, Future prospects for NA61: rare probes

Trigger particle

More medium effects: away-side3.0 < p

Ttrig < 4.0 GeV/c

1.3 < pT

assoc < 1.8 GeV/c

Mach Cone/Shock wave

T. Renk, J. Ruppert

Stöcker, Casseldery-Solana et al

A. Polosa, C. Salgado

Gluon radiation+Sudakov

Au+Au 0-10%

d+Au

Near side:Enhanced yield in Au+Au consistent with ridge-effect Away-side:

Strong broadening in central Au+Au‘Dip’ at =

Medium response (shock wave)or gluon radiation with kinematic constraints?

(other proposals exist as well: kT-type effect or

Cherenkov radiation)

M. Horner, M. van Leeuwen, et al

Note also: not shown is large background – something non-trivial may be hiding there?

Page 26: Future prospects for NA61 heavy ions: rare observables

26M. van Leeuwen, Future prospects for NA61: rare probes

-correlations from NA49M

. Szu

ba

, QM

09

Page 27: Future prospects for NA61 heavy ions: rare observables

27M. van Leeuwen, Future prospects for NA61: rare probes

Characterizing the shapes

PHENIX M. S

zub

a, Q

M0

9

Page 28: Future prospects for NA61 heavy ions: rare observables

28M. van Leeuwen, Future prospects for NA61: rare probes

Summary of correlation shapes

Away-side shape: no (large) energy dependence

Near-side shape: change from ‘dip’ to peak

M. S

zub

a, Q

M0

9