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Jaipur, India Feb 4-10 20 08 1 title Recent Results from Recent Results from BRAHMS BRAHMS R. Debbe for the BRAHMS R. Debbe for the BRAHMS Collaboration Collaboration Physics Dept. Brookhaven Physics Dept. Brookhaven National Laboratory National Laboratory

Jaipur, India Feb 4-10 20081 title Recent Results from BRAHMS R. Debbe for the BRAHMS Collaboration Physics Dept. Brookhaven National Laboratory

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Jaipur, India Feb T.Hirano and Y.Nara, Nucl.Phys.A743(2004)305 Energy loss: first order GLV (x,y)=(0,0) E max  Gauss E max =45 GeV/fm 3  flat = 2.0  Gauss = 0.8  0 = 0.6 fm/c We will make use of a 3D+1 hydrodynamic model provided graciously by T. Hirano to guide the description of our results. y=2.95 Parameterization of initial energy density

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Page 1: Jaipur, India Feb 4-10 20081 title Recent Results from BRAHMS R. Debbe for the BRAHMS Collaboration Physics Dept. Brookhaven National Laboratory

Jaipur, India Feb 4-10 2008 1

title

Recent Results from BRAHMSRecent Results from BRAHMS

R. Debbe for the BRAHMS R. Debbe for the BRAHMS CollaborationCollaboration

Physics Dept. Brookhaven National Physics Dept. Brookhaven National LaboratoryLaboratory

Page 2: Jaipur, India Feb 4-10 20081 title Recent Results from BRAHMS R. Debbe for the BRAHMS Collaboration Physics Dept. Brookhaven National Laboratory

Jaipur, India Feb 4-10 2008 2

Extent of sQGP in rapidity space.

Particle production (in rapidity space) as function of energy and system size.

Strangeness production in AuAu collisions at 62.4 GeV

Extracting high-x physics with the p/+ ratio and the RAuAu of protons in Au+Au collisions.

Systematics of baryon transport.

Outline of presentation

Page 3: Jaipur, India Feb 4-10 20081 title Recent Results from BRAHMS R. Debbe for the BRAHMS Collaboration Physics Dept. Brookhaven National Laboratory

Jaipur, India Feb 4-10 2008 3

T.Hirano and Y.Nara, Nucl.Phys.A743(2004)305

Energy loss: first order GLV

(x,y)=(0,0)

Emax

Gauss

• Emax=45 GeV/fm3

• flat = 2.0• Gauss = 0.8

0 = 0.6 fm/c

We will make use of a 3D+1 hydrodynamic model provided graciously by T. Hirano to guide the description of our results.

y=2.95Parameterization of initial energy density

Page 4: Jaipur, India Feb 4-10 20081 title Recent Results from BRAHMS R. Debbe for the BRAHMS Collaboration Physics Dept. Brookhaven National Laboratory

Jaipur, India Feb 4-10 2008 4

The animations show equal energy density contours at four rapidity values in proper time steps of 0.2fm/c

Partons simulated with Pythia are transported through the expanding system, average energy loss changes by ~X2 from y=0 to y=3, but the ratio of pT distributions of partons is insensitive to that change.

y=0 y=1 y=2 y=3

Page 5: Jaipur, India Feb 4-10 20081 title Recent Results from BRAHMS R. Debbe for the BRAHMS Collaboration Physics Dept. Brookhaven National Laboratory

Jaipur, India Feb 4-10 2008 5The RAuAu at high y is consistent with reduced energy loss and leaves room for saturation effects.

Page 6: Jaipur, India Feb 4-10 20081 title Recent Results from BRAHMS R. Debbe for the BRAHMS Collaboration Physics Dept. Brookhaven National Laboratory

Jaipur, India Feb 4-10 2008 6

Consistent with dense medium effects not fully extending to high y, with binary coll. scaling restored at mid-central collisions.

Centrality dependence of RAuAu pi- at 200 GeV

y=0

y=3.1

Page 7: Jaipur, India Feb 4-10 20081 title Recent Results from BRAHMS R. Debbe for the BRAHMS Collaboration Physics Dept. Brookhaven National Laboratory

Jaipur, India Feb 4-10 2008 7

At 62.4 GeV, dense system has shorter lifetime

At high y(>2), effects of dense medium start to disappear. Isospin effects grow stronger

I.G. Bearden 5th Feb.14:00

Au+Au 0-10% centralTop energy density

~20 GeV/fm3

Page 8: Jaipur, India Feb 4-10 20081 title Recent Results from BRAHMS R. Debbe for the BRAHMS Collaboration Physics Dept. Brookhaven National Laboratory

Jaipur, India Feb 4-10 2008 8

Particle production systematics

Positive pion production in p+p collisions at √s=200 and 62.4 GeV.

Systematic errors shown with gray boxes are mainly driven by extrapolations of pT distributions.

Measurements normalized to total inelastic cross section (41mb 200GeV and 36mb at 62.4 GeV)

Page 9: Jaipur, India Feb 4-10 20081 title Recent Results from BRAHMS R. Debbe for the BRAHMS Collaboration Physics Dept. Brookhaven National Laboratory

Jaipur, India Feb 4-10 2008 9

Positive pion production in d+Au at 200 GeV

The centrality dependence shows the presence of the Au “target” source at negative rapidity, as well as the projectile d at high rapidity. The distribution becomes similar to p+p in the most peripheral sample.

H. Yang 9th Feb. 14:00

Page 10: Jaipur, India Feb 4-10 20081 title Recent Results from BRAHMS R. Debbe for the BRAHMS Collaboration Physics Dept. Brookhaven National Laboratory

Jaipur, India Feb 4-10 2008 10

Positive pion produced in central (0-10%) Au+Au coll. at 62.4 GeV

Fit to single gaussian yields width consistent with Landau’s model: 2=ln(√s/2mp)

Landau= 1.87

Positive pion production in Au + Au at √sNN = 62.4 GeV

Page 11: Jaipur, India Feb 4-10 20081 title Recent Results from BRAHMS R. Debbe for the BRAHMS Collaboration Physics Dept. Brookhaven National Laboratory

Jaipur, India Feb 4-10 2008 11

Positive pion production in Au+Au at 200 GeV

To first order, all distributions are described with a single gaussian. Width of central events consistent with Landau’s value:

Landau= 2.16

meas.= 2.23±0.06

Page 12: Jaipur, India Feb 4-10 20081 title Recent Results from BRAHMS R. Debbe for the BRAHMS Collaboration Physics Dept. Brookhaven National Laboratory

Jaipur, India Feb 4-10 2008 12

Evolution of the multiplicity dist. Shapes with centrality

Central collisions, (up to 40%) scale with Npart. The tails of the peripheral distributions deviate from that scaling. (This has been attributed to pion emission from spectators. PHOBOS PRL91 052303)

Au+Au collisions at 200 GeV

Page 13: Jaipur, India Feb 4-10 20081 title Recent Results from BRAHMS R. Debbe for the BRAHMS Collaboration Physics Dept. Brookhaven National Laboratory

Jaipur, India Feb 4-10 2008 13

One can tune the baryo- chemical potential using the pbar/p values measured at different rapidities.

The high y K/pi+ ratios at RHIC (62.4 GeV) are very similar to the SPS results from the high energy slope of the “MarekHorn”. (At same pbar/p ratio and thus driven by the baryo-chemical potential.)

I.C. Arsene 5th Feb. 15:00

Poster by M. Murray

Page 14: Jaipur, India Feb 4-10 20081 title Recent Results from BRAHMS R. Debbe for the BRAHMS Collaboration Physics Dept. Brookhaven National Laboratory

Jaipur, India Feb 4-10 2008 14

High-x physics accessible with the p/+ ratio

The puzzling abundance of protons with respect to pions has been attributed to recombination effects that do reproduce the data at mid-rapidity for pt values that range up to ~6 GeV/c.

Our results at high y indicate that this ratio may rather be driven by beam fragmentation.

Page 15: Jaipur, India Feb 4-10 20081 title Recent Results from BRAHMS R. Debbe for the BRAHMS Collaboration Physics Dept. Brookhaven National Laboratory

Jaipur, India Feb 4-10 2008 15

Comparison of the p/+ in p+p and Au+Au systems at 62.4 GeV

The overall difference between the ratio measured in pp and AuAu is consistent with the favored interpretation based on coalescence in Au+AuThe similarity of the ratio in both systems may be driven by incoherent proton fragmentation. Large p+p value of ratio may be driven by proximity to beam rapidity.

Poster by N. Katrynska‘

p+p Au+Au

Page 16: Jaipur, India Feb 4-10 20081 title Recent Results from BRAHMS R. Debbe for the BRAHMS Collaboration Physics Dept. Brookhaven National Laboratory

Jaipur, India Feb 4-10 2008 16

Comparison of the p/+ in p+p and Au+Au systems at 200 GeV

At mid-rapidity the difference between pp and AuAu system can be related to re-combination which favors proton production.

A much pronounced effect at higher rapidity may be an interplay between fragmentation effects, parton coalescence and baryon transport.

Page 17: Jaipur, India Feb 4-10 20081 title Recent Results from BRAHMS R. Debbe for the BRAHMS Collaboration Physics Dept. Brookhaven National Laboratory

Jaipur, India Feb 4-10 2008 17

Nuclear modification factor for protons as function of y in AuAu 0-10% 200 GeV

As already seen with the p/+ ratio, baryons do not behave as mesons; this RAuAu shows the increased proton production at high y. Strong enhancement of pbars at y~3 is not understood, yet.

protons anti-proton

Page 18: Jaipur, India Feb 4-10 20081 title Recent Results from BRAHMS R. Debbe for the BRAHMS Collaboration Physics Dept. Brookhaven National Laboratory

Jaipur, India Feb 4-10 2008 18

RAuAu of (p+pbar)/2 as function of centrality in AuAu 200 GeV

Remarkable enhancement of proton prod. In peripheral coll.

y=0

y=3

Consistent with interplay of energy loss and multiple scattering effects. As well as radial flow.

Page 19: Jaipur, India Feb 4-10 20081 title Recent Results from BRAHMS R. Debbe for the BRAHMS Collaboration Physics Dept. Brookhaven National Laboratory

Jaipur, India Feb 4-10 2008 19

Baryon transport studies

BRAHMS experimental program will deliver a wealth of information on baryon transport with results that range from p+p collisions at 62.4 and 200 GeV to bigger systems like Cu+Cu and Au+Au at both energies an different centralities

p+p collisions at 200 GeV

Poster by H.H. Dalsgaard

Page 20: Jaipur, India Feb 4-10 20081 title Recent Results from BRAHMS R. Debbe for the BRAHMS Collaboration Physics Dept. Brookhaven National Laboratory

Jaipur, India Feb 4-10 2008 20

Centrality dependent net-proton distributions AuAu 200 GeV

Npart scaling in semi-central to central coll. (below 40%). Similar scaling appears to extend to ~high rapidity. Shape changes are evident at the “rapidity shifted” peak.

Poster by C. Nygaard

Hijing-B v1.1

AMPT

Page 21: Jaipur, India Feb 4-10 20081 title Recent Results from BRAHMS R. Debbe for the BRAHMS Collaboration Physics Dept. Brookhaven National Laboratory

Jaipur, India Feb 4-10 2008 21

Summary and outlook• Using some guidance from 3D+1 hydro dynamical expansion calculation, we find that, the fact that nuclear modification factors remain constant as function of y, is an indication that other factors besides energy loss do contribute to the overall small measured value. The strength of these effects would grow with y.

• We have described ongoing analysis of particle production in all the measured systems. In particular, a comparison to SPS indicates that the K/pi+ ratio is driven by the B potential.

• We have reported interesting effects related to protons at moderate pT at high rapidity.

• We presented results on baryon transport, with special focus on the AuAu system.

• We need to balance the need to bring analyses to publication and new focus for each member institution.

Page 22: Jaipur, India Feb 4-10 20081 title Recent Results from BRAHMS R. Debbe for the BRAHMS Collaboration Physics Dept. Brookhaven National Laboratory

Jaipur, India Feb 4-10 2008 22

BRAHMS CollaborationI. C. Arsene12, I. G. Bearden7, D. Beavis1, S. Bekele12, C. Besliu10, B. Budick6,

H. Bøggild7, C. Chasman1, C. H. Christensen7, P. Christiansen7, H.Dahlsgaard7, R. Debbe1, J. J. Gaardhøje7, K. Hagel8, H. Ito1, A. Jipa10, E.B.Johnson11, J. I. Jørdre9,

C. E. Jørgensen7, R. Karabowicz5, N. Katrynska5 ,E. J. Kim11, T. M. Larsen7, J. H. Lee1, Y. K. Lee4,S. Lindahl12, G. Løvhøiden12, Z. Majka5, M. J. Murray11,J. Natowitz8, C.Nygaard7

B. S. Nielsen7, D. Ouerdane7, D.Pal12, F. Rami3, C. Ristea8, O. Ristea11, D. Röhrich9, B. H. Samset12, S. J. Sanders11, R. A. Scheetz1, P. Staszel5,

T. S. Tveter12, F. Videbæk1, R. Wada8, H. Yang9, Z. Yin9, I. S. Zgura2 A. Qviller7

1. Brookhaven National Laboratory, Upton, New York, USA2. Institute of Space Science, Bucharest - Magurele, Romania3. Institut Pluridisciplinaire Hubert Curien et Université Louis Pasteur, Strasbourg, France4. Johns Hopkins University, Baltimore, USA5. M. Smoluchkowski Institute of Physics, Jagiellonian University, Krakow, Poland6. New York University, New York, USA7. Niels Bohr Institute, University of Copenhagen, Copenhagen, Denmark8. Texas A&M University, College Station, Texas, USA9. University of Bergen, Department of Physics and Technology, Bergen, Norway10. University of Bucharest, Romania11. University of Kansas, Lawrence, Kansas, USA12. University of Oslo, Department of Physics, Oslo, Norway