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Craig Ogilvie, Iowa State University On behalf of the PHENIX Collaboration Heavy flavor systematics from PHENIX Sep 27, 2013 1 Complexity of interpreting data from HI collisions Use systematics: spectra, elliptic flow,… Present d+Au, Cu+Cu, excitation function,… [email protected]
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Craig Ogilvie, Iowa State University On behalf of the PHENIX Collaboration Heavy flavor systematics…

Jan 20, 2018

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CNM I: d+Au heavy-flavor at 200 GeV Sep 27, Non-photonic e, from heavy-flavor decays Phys. Rev. Lett. 109, (2012), Phys. Rev. Lett. 109, (2012) Significant enhancement at moderate p T
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Page 1: Craig Ogilvie, Iowa State University On behalf of the PHENIX Collaboration Heavy flavor systematics…

[email protected]

Craig Ogilvie, Iowa State UniversityOn behalf of the PHENIX Collaboration

Heavy flavor systematics from PHENIX

Sep 27, 20131

• Complexity of interpreting data from HI collisions• Use systematics: spectra, elliptic flow,…• Present d+Au, Cu+Cu, excitation function,…

• Which leads to the complexity of interpreting d+Au…

Page 2: Craig Ogilvie, Iowa State University On behalf of the PHENIX Collaboration Heavy flavor systematics…

[email protected]

Complexity of d(p)+A collisions

Sep 27, 20132

Nuclear structure functionsShadowing, saturation at low-xAnti-shadowing at moderate, high-x

Initial state scatteringOften modeled as increase in effective kTLikely largest impact at RHIC where spectra are softer

Possible collective effectsBarbara Jacak’s talk on Wed

Final state energy-loss, absorption,….Centrality classification

Page 3: Craig Ogilvie, Iowa State University On behalf of the PHENIX Collaboration Heavy flavor systematics…

[email protected]

CNM I: d+Au heavy-flavor at 200 GeV

Sep 27, 20133

Non-photonic e, from heavy-flavor decays Phys. Rev. Lett. 109, 242301 (2012) , Significant enhancement

at moderate pT

Page 4: Craig Ogilvie, Iowa State University On behalf of the PHENIX Collaboration Heavy flavor systematics…

[email protected]

CNM II: d+Au heavy-flavor at 200 GeV

Sep 27, 20134

Non-photonic e, from heavy-flavor decays

Phys. Rev. Lett. 109, 242301 (2012)

Enhancement present in min-biasEffect not caused by challenges of centrality definition

RdA

PT (GeV/c)

Page 5: Craig Ogilvie, Iowa State University On behalf of the PHENIX Collaboration Heavy flavor systematics…

[email protected]

CNM IV: Forward, backward m from HF decay

Sep 27, 20135

m me

Forward rapidity suppressedLikely shadowing at low-x in Au

Backward rapidity enhancedanti-shadowing at higher x in Au?or increase in <kT> due to initial scattering?

Page 6: Craig Ogilvie, Iowa State University On behalf of the PHENIX Collaboration Heavy flavor systematics…

[email protected]

CNM III: Identified hadron spectra in dA

Sep 27, 20136

Phys. Rev. C 88, 024906 (2013)

Cronin peak: proton ~ > HFe

Why?

Page 7: Craig Ogilvie, Iowa State University On behalf of the PHENIX Collaboration Heavy flavor systematics…

[email protected]

RdA

PT (GeV/c)

CNM II: d+Au heavy-flavor at 200 GeV

Sep 27, 20137

Phys. Rev. Lett. 109, 242301 (2012)

Does <kT> increase have larger impact when p+p spectrum is soft?spectra = convolution of scattering + fragmentation

Or recombination effects in hadronization? Or collective? Or…Opportunity for theory impact

Page 8: Craig Ogilvie, Iowa State University On behalf of the PHENIX Collaboration Heavy flavor systematics…

[email protected]

Example with p0 RdA

Sep 27, 20138

p0 calc from I. VitevReasonable reproduction of p0

Nuclear structure functionCronin

Large initial state multiple-scattering

Final state Eloss Need calculations for heavy-

flavor RdA

Vitev et al., PRD 74 (2006)Phys.Lett. B718 (2012) 482-487

Page 9: Craig Ogilvie, Iowa State University On behalf of the PHENIX Collaboration Heavy flavor systematics…

J/y CNM

Sep 27, 20139 y

EPS09 nuclear structure functions plus breakupReasonable reproduction, misses centrality dependence

BUT, charm is enhanced at moderate pT

(non-photonic electrons RdA>1)

1) Do these calculations reproduce open charm RdA >1 ?

2) If not, then more effective suppression needed for J/y

PRL 107, 142301 (2011)

Page 10: Craig Ogilvie, Iowa State University On behalf of the PHENIX Collaboration Heavy flavor systematics…

Normalize J/y by HF?

Sep 27, 201310

J/y at mid-y suppressed @low-pt

Charm is enhanced at moderate pt (non-photonic electrons RdA>1)

Alternative: use dA HF spectra as baseline?

• Question, what axis? pT ?RdA

PT (GeV/c)

J/y

Phys. Rev. C 87, 034904 (2013)

Au-going, high-x

d-going, low-x

Page 11: Craig Ogilvie, Iowa State University On behalf of the PHENIX Collaboration Heavy flavor systematics…

[email protected]

Connect d+Au to A+A

Sep 27, 201311

Phys. Rev. Lett. 109, 242301 (2012) ,

1) Enhancement in d+Au + energy-loss suppression in A+A2) Models must attempt to reproduce both d+A and A+A

Min-bias collisions

Page 12: Craig Ogilvie, Iowa State University On behalf of the PHENIX Collaboration Heavy flavor systematics…

[email protected]

One method to organize results

Sep 27, 201312

Phys. Rev. Lett. 109, 242301 (2012) , Matt Durham

Common suppression pattern when normalized by square of RdA

Does this take into account impact of initial state increase of <kT>?

Page 13: Craig Ogilvie, Iowa State University On behalf of the PHENIX Collaboration Heavy flavor systematics…

[email protected]

Intermediate Cu+Cu: links d+A and Au+Au

Sep 27, 201313

Peripheral Cu+Cu (yellow)Enhancement ~ central d+Au (blue)

Page 14: Craig Ogilvie, Iowa State University On behalf of the PHENIX Collaboration Heavy flavor systematics…

[email protected]

d+Au to Cu+Cu to Au+Au

Sep 27, 201314

Interplay of two effectsCNM increases yield, competes with energy-loss suppression

Page 15: Craig Ogilvie, Iowa State University On behalf of the PHENIX Collaboration Heavy flavor systematics…

[email protected]

d+Au to Cu+Cu to Au+Au

Sep 27, 201315

Higher pTCNM increases yield, stronger energy-loss suppression

Page 16: Craig Ogilvie, Iowa State University On behalf of the PHENIX Collaboration Heavy flavor systematics…

[email protected]

dAu

Cu+Cu heavy-flavor, forward rapidity

Sep 27, 201316

Large uncertainties: Forward y in central d+Au ~ peripheral Cu+Cu

Cu+Cu forward y, Au+Au mid-rapidity

Page 17: Craig Ogilvie, Iowa State University On behalf of the PHENIX Collaboration Heavy flavor systematics…

Additional lever arm: beam energy

Sep 27, 201317

Dominant energy-loss at high s Transitions to stronger Cronin effect at lower s

pT (GeV/c)

charged hadrons from Au+Aup0 Phys. Rev. Lett. 109, 152301 (2012)

Page 18: Craig Ogilvie, Iowa State University On behalf of the PHENIX Collaboration Heavy flavor systematics…

[email protected]

Need RdA at lower-beam energy

Sep 27, 201318

Not in current RHIC running plan :(How does RdA change from 200 GeV to 62 GeV Three beam energies (62, 200 GeV, LHC) constrains interplay

of structure function, initial state scatteringRdA calculations at 62 GeV

p RdA ~ 2 at 62 GeV p RdA ~ 1.2 at 200 GeV

A. Accardi Eur. Phys. J. C 43, 121–125 (2005)

Page 19: Craig Ogilvie, Iowa State University On behalf of the PHENIX Collaboration Heavy flavor systematics…

Non-photonic electrons Au+Au 62 GeV

Sep 27, 201319

Lower beam energy changes interplay of two effectsStronger CNM competing with weaker energy-loss

Forthcoming PHENIX publicationspectra with smaller systematicscomparison with p+p, RAA etc.

If your model reproduces 200 GeV and 2.76 TeV heavy flavor RAA

Final call for 62 GeV HF RAA prediction

Page 20: Craig Ogilvie, Iowa State University On behalf of the PHENIX Collaboration Heavy flavor systematics…

[email protected]

HF v2 at lower beam energy

Sep 27, 201320

HF flow is > 0 at 62 GeV, but uncertainties large

Page 21: Craig Ogilvie, Iowa State University On behalf of the PHENIX Collaboration Heavy flavor systematics…

[email protected]

V2 2nd constraint on e-loss Au+Au 200 GeV

Sep 27, 201321

Low-pt Charm v2, extent of thermalization of HFChallenge for theory to reproduce both RAA, v2

Many calculations, theory updates past few years

Page 22: Craig Ogilvie, Iowa State University On behalf of the PHENIX Collaboration Heavy flavor systematics…

[email protected]

One example, P.B. Gossiaux SQM 2013

Sep 27, 201322

Elastic + radiative energy lossWith running coupling a

Page 23: Craig Ogilvie, Iowa State University On behalf of the PHENIX Collaboration Heavy flavor systematics…

[email protected]

Is dpT/pT what we should be plotting for HF?

Sep 27, 201323

PRC 87, 034911 (2013)

Suggestion in spirit of workshop, This is being worked on for HF, but no results available yet

Page 24: Craig Ogilvie, Iowa State University On behalf of the PHENIX Collaboration Heavy flavor systematics…

[email protected]

VTX Upgrade @ PHENIXTwo layers of silicon pixel detectorsTwo layers of silicon strip detectorsFour layers in endcapsTracks extrapolate back to collision vertexDisplaced vertices charm (D), beauty (B)Requires ~ 50 mm precision

De+X Au

e

Au

X

B e+X

Xp0 e+e- ee

Sep 27, 201324

Installed 2010-12

Page 25: Craig Ogilvie, Iowa State University On behalf of the PHENIX Collaboration Heavy flavor systematics…

[email protected]

VTX p+p results

Sep 27, 201325 2012/10/23

charm/bottom assumes PYTHIA spectra

DCA data are fit by expected DCA shapes of • Signal components : c e and b e (right column)• Background components (left column)

Fit range : 0.2<|DCA|<1.5(mm)

b/(b+c)=0.22+-0.06

Page 26: Craig Ogilvie, Iowa State University On behalf of the PHENIX Collaboration Heavy flavor systematics…

[email protected]

VTX p+p results

Sep 27, 201326 2012/10/23

FONLL consistent with b/(b+c) data

Page 27: Craig Ogilvie, Iowa State University On behalf of the PHENIX Collaboration Heavy flavor systematics…

[email protected]

Physics Goal

Sep 27, 201327

Energy-loss heavy-flavor understand nature of sQGPProgress on understanding many detailsIf a model reproduces a broad range of data

Can we infer any characteristics of QGP?Either direct via a parameter of model

Diffusion parameterOr run same dynamical model in a “box”, e.g. radiation +

collision Eloss

Infer effective transport parametersWhich characteristics of sQGP are accessible this way and can we

communicate this to our fellow physicists?Maybe too many unsettled aspects yet

Page 28: Craig Ogilvie, Iowa State University On behalf of the PHENIX Collaboration Heavy flavor systematics…

[email protected]

Summary

Sep 27, 201328

Complexity of interpreting d+AuLevers: centrality, A, y, s, change impact of

Structure function, initial state scattering, e-loss,…HF RdA enhancement up to factor of 1.5

Call for model calculationsIs dAu HF a better baseline for RAA HF and dAu J/y

production?? Complexity of interpreting data from HI collisions

Cu+Cu HF yields smoothly connects dAu to Au+AuCompetition between enhancement + suppression

Change this competitionAu+Au HF data @ 62 GeV, need dAu running at 62 GeV

Page 29: Craig Ogilvie, Iowa State University On behalf of the PHENIX Collaboration Heavy flavor systematics…

[email protected]

Backup slides

Sep 27, 201329

Page 30: Craig Ogilvie, Iowa State University On behalf of the PHENIX Collaboration Heavy flavor systematics…

[email protected]

X-ranges

Sep 27, 201330

SPSPb+Pb17 GeV

RHIC Au+Au200 GeV

LHC Pb+Pb5.5 TeV

c-cbar X~10-1 X~10-2 X~10-3 to 10 -4

Eskola et al. JHEP 0904 (2009) 065

Page 31: Craig Ogilvie, Iowa State University On behalf of the PHENIX Collaboration Heavy flavor systematics…

[email protected]

RAA of heavy-flavor: from RHIC to LHC

Sep 27, 201331

Note to Craig add citations

Page 32: Craig Ogilvie, Iowa State University On behalf of the PHENIX Collaboration Heavy flavor systematics…

[email protected] Sep 27, 201332

Page 33: Craig Ogilvie, Iowa State University On behalf of the PHENIX Collaboration Heavy flavor systematics…

[email protected]

Charm production at 62 GeV reproduced by FONLL

Sep 27, 201333

Page 34: Craig Ogilvie, Iowa State University On behalf of the PHENIX Collaboration Heavy flavor systematics…

[email protected] Sep 27, 201334

Page 35: Craig Ogilvie, Iowa State University On behalf of the PHENIX Collaboration Heavy flavor systematics…

[email protected] Sep 27, 201335

Page 36: Craig Ogilvie, Iowa State University On behalf of the PHENIX Collaboration Heavy flavor systematics…

[email protected]

Less bound charmonia in dAu collisions

Sep 27, 201336

arXiv:1305.5516

All three systems consistent within uncertainties

Page 37: Craig Ogilvie, Iowa State University On behalf of the PHENIX Collaboration Heavy flavor systematics…

[email protected]

Less bound charmonia in dAu collisions

Sep 27, 201337

arXiv:1305.5516

y’ suppression stronger than J/y for more central dAu collisionsStronger effective breakup cross-section?

Page 38: Craig Ogilvie, Iowa State University On behalf of the PHENIX Collaboration Heavy flavor systematics…

[email protected]

Photon in dA

Sep 27, 201338

Phys.Lett. B718 (2012) 482-487