brahms y2000 + y2001 @ rhic: s nn =130 gev, and s nn =200 gev

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Sept 4, 2001 Paris, Jens Jørgen Gaardhøje, Niels Bohr Institute 1 Reaction features in 65 AGeV + 65 AGeV and 100 AGeV + 100 AGeV Au-AU collisions EM dissociation dN(ch)/d distribution -4<<4 vs. Collision Centrality Production of charged particles, N(ch)/pr.participant Bjorken limit attained ? Transparency or Stopping p-bar/p vs y, b, p t Strangeness vs y Future BRAHMS Y2000 + Y2001 @ RHIC: s nn =130 GeV, and s nn =200 GeV

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BRAHMS Y2000 + Y2001 @ RHIC: s nn =130 GeV, and s nn =200 GeV. Reaction features in 65 AGeV + 65 AGeV and 100 AGeV + 100 AGeV Au-AU collisions EM dissociation dN(ch)/d  distribution -4

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Page 1: BRAHMS Y2000 + Y2001 @ RHIC:  s nn =130 GeV, and  s nn =200 GeV

Sept 4, 2001 Paris, Jens Jørgen Gaardhøje, Niels Bohr Institute 1

Reaction features in 65 AGeV + 65 AGeV and 100 AGeV + 100 AGeV Au-AU collisions

EM dissociation dN(ch)/d distribution -

4<<4 vs. Collision Centrality

Production of charged particles, N(ch)/pr.participant

Bjorken limit attained ? Transparency or Stopping

p-bar/p vs y, b, pt

Strangeness vs y Future

BRAHMS Y2000 + Y2001 @ RHIC: snn=130 GeV, and snn=200 GeV

Page 2: BRAHMS Y2000 + Y2001 @ RHIC:  s nn =130 GeV, and  s nn =200 GeV

Sept 4, 2001 Paris, Jens Jørgen Gaardhøje, Niels Bohr Institute 2

I.G. Bearden7, D. Beavis1, C. Besliu10, Y. Blyakhman6, J. Bondorf7, J.Brzychczyk4, B. Budick6, H. Bøggild7, C. Chasman1, C. H. Christensen7, P. Christiansen7, J.Cibor4,

R.Debbe1, J. J. Gaardhøje7, K. Grotowski4, K. Hagel8, O. Hansen7, H. Heiselberg7, A. Holm7, A.K. Holme12, H. Ito11, E. Jacobsen7, A. Jipa10, J. I. Jordre10, F. Jundt2, C. E. Jørgensen7, T. Keutgen9, E. J. Kim5, T. Kozik3, T.M.Larsen12, J. H. Lee1, Y. K.Lee5,

G. Løvhøjden2, Z. Majka3, A. Makeev8, B. McBreen1, M. Murray8, J. Natowitz8, B.S.Nielsen7, K. Olchanski1, D. Ouerdane7, R.Planeta4, F. Rami2, D. Roehrich9, B. H.

Samset12, S. J. Sanders11, I. S. Sgura10, R.A.Sheetz1, Z.Sosin3, P. Staszel7, T.S. Tveter12, F.Videbæk1, R. Wada8 and A.Wieloch3.

1Brookhaven National Laboratory, USA 2IReS and Université Louis Pasteur, Strasbourg, France

3Jagiellonian University, Cracow, Poland 4Institute of Nuclear Physics, Cracow, Poland 5Johns Hopkins University, Baltimore, USA

6New York University, USA 7Niels Bohr Institute, Blegdamsvej 17, University of Copenhagen, Denmark 8Texas A&M University, College Station. USA

9University of Bergen, Norway 10University of Bucharest, Romania

11University of Kansas, Lawrence,USA 12 University of Oslo Norway

BRAHMS Intl. collaboration

Page 3: BRAHMS Y2000 + Y2001 @ RHIC:  s nn =130 GeV, and  s nn =200 GeV

Sept 4, 2001 Paris, Jens Jørgen Gaardhøje, Niels Bohr Institute 3

RHIC physicsAugust 2000 & August 2001

2:00 o’clock

4:00 o’clock6:00 o’clock

8:00 o’clock

10:00 o’clock

STARPHENIX

RHIC

AGS

LINACBOOSTER

TANDEMS

9 GeV/uQ = +79

1 MeV/uQ = +32

HEP/NP

g-2

U-lineBAF (NASA)

BRAHMS: Lpeak = 3.3 1025 cm-2 s-1

Lave = 1.7 1025 cm-2 s-1

Rcoll= 350 HzPHOBOS

6 b-1

2 wks

August 2000 and 2001

Page 4: BRAHMS Y2000 + Y2001 @ RHIC:  s nn =130 GeV, and  s nn =200 GeV

Sept 4, 2001 Paris, Jens Jørgen Gaardhøje, Niels Bohr Institute 4

BRAHMS in the 2’ hall

… in 1998

Page 5: BRAHMS Y2000 + Y2001 @ RHIC:  s nn =130 GeV, and  s nn =200 GeV

Sept 4, 2001 Paris, Jens Jørgen Gaardhøje, Niels Bohr Institute 5

Forward & Midrapidity spectrometers

FS: 2 TPC, 2 TOF, C1-threshold, 3 Drift Ch. Mod., RICH, 4 Dipoles

2.5 - 30 deg. = 1.5 - 4

MRS: 2 TPC, 1 Dipole, 1TOF

30 - 90 deg. = 0 - 1.5

Page 6: BRAHMS Y2000 + Y2001 @ RHIC:  s nn =130 GeV, and  s nn =200 GeV

Sept 4, 2001 Paris, Jens Jørgen Gaardhøje, Niels Bohr Institute 6

First BRAHMS collision at 100 AGeV+100AGeV

T1

MTPC1

T2

MTPC2

MRS: 90 deg

6.5 msr

FS: 6 deg

0.8 msr

Page 7: BRAHMS Y2000 + Y2001 @ RHIC:  s nn =130 GeV, and  s nn =200 GeV

Sept 4, 2001 Paris, Jens Jørgen Gaardhøje, Niels Bohr Institute 7

BRAHMS acceptanceAugust 2000 & 2001

Page 8: BRAHMS Y2000 + Y2001 @ RHIC:  s nn =130 GeV, and  s nn =200 GeV

Sept 4, 2001 Paris, Jens Jørgen Gaardhøje, Niels Bohr Institute 8

Global detectorsSiMA, TMA, BB

SiMA (-2.0< <2.0) PTMA (-2.2< <2.2) Beam-Beam (3 < | | < 4)

97% (geom)

Page 9: BRAHMS Y2000 + Y2001 @ RHIC:  s nn =130 GeV, and  s nn =200 GeV

Sept 4, 2001 Paris, Jens Jørgen Gaardhøje, Niels Bohr Institute 9

Centrality determinationVertex distribution

1m

Page 10: BRAHMS Y2000 + Y2001 @ RHIC:  s nn =130 GeV, and  s nn =200 GeV

Sept 4, 2001 Paris, Jens Jørgen Gaardhøje, Niels Bohr Institute 10

Electromagnetic nuclear dissociation

LO+NLO Mutual EM

•Mutual Electromagnetic dissociation

•(Spectrum of virtual photons) * (absorption cross section) = WW

•Multiphonon GDR excitation, abs

•EM vs Nuclear coll.

•=> neutron (L*R) coincidences

•RELDIS. Pshenichnov, JPB, IM, et al.

EM dissociation selected by ZDC coincidences

and TMA Veto in BRAHMS

n

n n

2n

1n

LO

NLO

Page 11: BRAHMS Y2000 + Y2001 @ RHIC:  s nn =130 GeV, and  s nn =200 GeV

Sept 4, 2001 Paris, Jens Jørgen Gaardhøje, Niels Bohr Institute 11

Neutral Energy correlations (ZDC)

C2(EL,ER)=P(EL,ER)/(P(EL)*P(ER))

Page 12: BRAHMS Y2000 + Y2001 @ RHIC:  s nn =130 GeV, and  s nn =200 GeV

Sept 4, 2001 Paris, Jens Jørgen Gaardhøje, Niels Bohr Institute 12

dNch/d @ snn= 130 GeVSiMA, TMA, BB, TPC

N=dE /<dE> P(0)/P(n1) Background corr.due

to secondaries (37-50%)

Consistency between 4 independent detector systems

65 AGeV+ 65 AGeV: N(ch)d= 4050±300 Central 0-5% dN(ch)/d (=0) =550 FWHM of distribution

= 7.6 0.7

0-5%

10-20%

20-30%

30-40%

40-50%

5-10%

600

BRAHMS Subm. Phys. Lett. B 7/2001.

Page 13: BRAHMS Y2000 + Y2001 @ RHIC:  s nn =130 GeV, and  s nn =200 GeV

Sept 4, 2001 Paris, Jens Jørgen Gaardhøje, Niels Bohr Institute 13

TPC tracks, Vertex reconstruction, Charged particle track density

MTPC1

z

y

Page 14: BRAHMS Y2000 + Y2001 @ RHIC:  s nn =130 GeV, and  s nn =200 GeV

Sept 4, 2001 Paris, Jens Jørgen Gaardhøje, Niels Bohr Institute 14

Charged Particle Mult.snn=130 GeV

BRAHMS. Subm. to Phys Lett. B. 2001

SPS

Page 15: BRAHMS Y2000 + Y2001 @ RHIC:  s nn =130 GeV, and  s nn =200 GeV

Sept 4, 2001 Paris, Jens Jørgen Gaardhøje, Niels Bohr Institute 15

NCharged vs. number of participant nucleon pairs. snn=130AGeV

dN/d 3 (=0) pr.part pair. Cf. HIJING, FRITIOF No saturation effects

observed

Claus Ekman Jørgensen.

Thesis NBI 2001

FRITIOF

HIJING

MTPC1 CEJ

EKRT

Page 16: BRAHMS Y2000 + Y2001 @ RHIC:  s nn =130 GeV, and  s nn =200 GeV

Sept 4, 2001 Paris, Jens Jørgen Gaardhøje, Niels Bohr Institute 16

RHIC: 200 AGeVWill this happen?

Page 17: BRAHMS Y2000 + Y2001 @ RHIC:  s nn =130 GeV, and  s nn =200 GeV

Sept 4, 2001 Paris, Jens Jørgen Gaardhøje, Niels Bohr Institute 17

dNch/d for100 AGeV + 100 AGeV

100 AGeV + 100 AGeV Au+Au

N(ch)d= 5100±300 Central 0-6% dN(ch)/d (=0) =61050 FWHM of distribution

= 7.9 1.0

BRAHMS 200AGEV

Page 18: BRAHMS Y2000 + Y2001 @ RHIC:  s nn =130 GeV, and  s nn =200 GeV

Sept 4, 2001 Paris, Jens Jørgen Gaardhøje, Niels Bohr Institute 18

Hard and Soft vs.High Density QCD @ 200 AGeV

Kharzeev and Levin (nucl-th/0108006)

Soft-Hard: dN/d=(1-X) npp <Npart>/2

+ X npp <Ncoll>

<Ncoll>=1049, <Npart>=339, npp=2.43 =>dN/d=668 (with X=0.9)

High Density QCD-saturation: dN/dy = f( Npart, Qs

2, ,QCD,s,y)

with =0.3 from HERA data => dN/d=620 (using dN/d=549 at

s=130GeV)

Page 19: BRAHMS Y2000 + Y2001 @ RHIC:  s nn =130 GeV, and  s nn =200 GeV

Sept 4, 2001 Paris, Jens Jørgen Gaardhøje, Niels Bohr Institute 19

Total production of Charged particles

130 AGeV 4000 charged part. observed Nch 23.5 pr. part. pair cf. Nch 17 in p+p at s=130GeV 35-40% increase over p+p

Syst

?BRAHMS

200 AGeV 130AGeV

200 AGeV 5100 charged part. observed Nch 30 pr. part. pair cf. Nch 20 in p+p at

s=200GeV 50% increase over p+p

Page 20: BRAHMS Y2000 + Y2001 @ RHIC:  s nn =130 GeV, and  s nn =200 GeV

Sept 4, 2001 Paris, Jens Jørgen Gaardhøje, Niels Bohr Institute 20

Hadron identification MRS (90, 40 deg)

m2=p2( t2 / L2 -1)

p-bar

K p

=0

=3

p

K

0

p, pbar

Page 21: BRAHMS Y2000 + Y2001 @ RHIC:  s nn =130 GeV, and  s nn =200 GeV

Sept 4, 2001 Paris, Jens Jørgen Gaardhøje, Niels Bohr Institute 21

Hadron IdentificationFS (4 deg & 130AGeV)

p-bar

=3

C1,H1,T2

+

p

m2=p2( t2 / L2 -1)

+

p

K+

Page 22: BRAHMS Y2000 + Y2001 @ RHIC:  s nn =130 GeV, and  s nn =200 GeV

Sept 4, 2001 Paris, Jens Jørgen Gaardhøje, Niels Bohr Institute 22

N(pbar)/N(p) @ 130 AGeV Centrality and Pt dependence

Antiproton absorbtion correction to pbar/p ratio:

5 % for FS at 4 deg 2 % for MRS at 90, 40 deg 10% corr. (low pt) p from Be-

tube Applied to data

Most pbar and p from Hyperon decays fall into spectrometer acceptance.

Correction factor depends on H/B, H-bar/B-bar and TB/TH

For H/B < 0.5 systematic correction is < 5% on ratio

Model dependent not applied to data

Page 23: BRAHMS Y2000 + Y2001 @ RHIC:  s nn =130 GeV, and  s nn =200 GeV

Sept 4, 2001 Paris, Jens Jørgen Gaardhøje, Niels Bohr Institute 23

Bjorken limit reached for Au+Au snn= 130GeV?

ISR R803

s=23

s=63

BRAHMS

PRL sept. 2001

Page 24: BRAHMS Y2000 + Y2001 @ RHIC:  s nn =130 GeV, and  s nn =200 GeV

Sept 4, 2001 Paris, Jens Jørgen Gaardhøje, Niels Bohr Institute 24

FS Hadron identificationfor snn = 200 GeV Au+Au

TOF and Cherenkov veto in FFS

Page 25: BRAHMS Y2000 + Y2001 @ RHIC:  s nn =130 GeV, and  s nn =200 GeV

Sept 4, 2001 Paris, Jens Jørgen Gaardhøje, Niels Bohr Institute 25

Particle ratios snn = 200 GeV (y=2)

Y=2 : p-bar/p = 0.48 0.08 -/+= 0.98 0.04

BRAHMS: Preliminary Integrated over centrality and

pt rangeK- p-

K+ p

Page 26: BRAHMS Y2000 + Y2001 @ RHIC:  s nn =130 GeV, and  s nn =200 GeV

Sept 4, 2001 Paris, Jens Jørgen Gaardhøje, Niels Bohr Institute 26

N(p-bar)/N(p) systematics vs CM energy

Page 27: BRAHMS Y2000 + Y2001 @ RHIC:  s nn =130 GeV, and  s nn =200 GeV

Sept 4, 2001 Paris, Jens Jørgen Gaardhøje, Niels Bohr Institute 27

StrangenessK-/K+ vs y @ snn= 130GeV

BRAHMS Preliminary

CERN-SPS

Page 28: BRAHMS Y2000 + Y2001 @ RHIC:  s nn =130 GeV, and  s nn =200 GeV

Sept 4, 2001 Paris, Jens Jørgen Gaardhøje, Niels Bohr Institute 28

How consistent are the models @ snn= 130GeV?

Page 29: BRAHMS Y2000 + Y2001 @ RHIC:  s nn =130 GeV, and  s nn =200 GeV

Sept 4, 2001 Paris, Jens Jørgen Gaardhøje, Niels Bohr Institute 29

Summary: First Au+Au snn=130 & 200 GeV

RESULTS: 100+100 Nch (0-5%) 5100 dN/d (y=0) 625. FWHM 7.8 N(ch) 30 pr. participant-pair dN/d (y=0) 3.6 pr. part. Pair

p-bar/p = 0.48 (y=2) Moderate growth in baryon

poor ’plateau’. Total mult. Increases by 25%, Central mult increases by 14% Pbar/p increases by 17% (y=2)

Large y and pt coverage to come

RESULTS: 65+65 Nch (0-5%) 4000 dN/d (y=0) 550. FWHM 7.6 N(ch) 23 pr. participant-pair dN/d (y=0) 3 pr. part. Pair

AntiMeson/Meson close to unity

p-bar/ p vs y shows increased but still incomplete transparency

Midrapidity Plateau? y =0,0.7,2 : pbar/p 0.64, 0.66,

0.41 (±0.05 ± 0.06) Weak pt and centrality

dependence Bjorken limit not reached Models inconsistent with data