The Heavy Flavor Tracker (HFT) The Silicon Vertex Upgrade of RHIC Jaiby Joseph* for the STAR Collaboration * Kent State University, USA Lake Louise.

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Presentation transcript:

The Heavy Flavor Tracker (HFT) The Silicon Vertex Upgrade of RHIC Jaiby Joseph* for the STAR Collaboration * Kent State University, USA Lake Louise Winter Institute Feb th, 2011

Outline The Heavy Flavor physics opportunities in Heavy Ion Collisions The HFT concept and realization Physics performance (simulations)

The Bottom Line Hot and dense (partonic) matter with strong collectivity has been formed in Au+Au collisions at RHIC. Study of the properties of the new form of matter requires more penetrating probes like heavy quarks. o Mechanism for parton energy loss. o Thermalization New micro-vertex detector is needed for STAR experiment. DOE milestone for 2016: “Measure production rates, high pT spectra, and correlations in heavy-ion collisions at √s NN = 200 GeV for identified hadrons with heavy flavor valence quarks to constrain the mechanism for parton energy loss in the quark- gluon plasma.”

STAR Detector TPC & HFT Large acceptance at midrapidity, |η| <1 Full azimuthal coverage, 0 < ϕ < 2π

STAR Physics Program 1)At 200 GeV top energy - Study medium properties, EoS - pQCD in hot and dense medium 2) RHIC beam energy scan - Search for the QCD critical point - Chiral symmetry restoration Spin program - Study proton intrinsic properties Forward program - Study low-x properties, search for CGC - Study elastic (inelastic) processes (pp2pp) - Investigate gluonic exchanges

Heavy Quark Energy Loss Surprising results - - challenge our understanding of the energy loss mechanism - force us to RE-think about the elastic-collisions energy loss - Requires direct measurements of c- and b-hadrons. 1) Non-photonic electrons decayed from - charm and beauty hadrons 2) At p T ≥ 6 GeV/c, R AA (n.p.e.) ~ R AA (h ± )! Contradicts naïve pQCD predictions STAR: Phys. Rew. Lett, 98, (2007).

SSD+ R=22cm IST R=14cm Pixel 1-2 R=2.5, 8cm SSD+ IST PIXEL HFT Technology New beam pipe Low mass Near the event vertex Active pixels Pointing resolution ~25  GeV/c to resolve average decay length ~80  m

200 GeV DATA with old Silicon TPC only Cu+Cu TPC+SVT+SSD Au+Au (Relatively) low significance peaks have already been observed in the DATA but of limited physics reach STAR preliminary

STAR HFT has the capacity to reconstruct the displaced vertex of D 0  K  (B.R 3.8%, c  = 123  m) Λ c   Kp (B. R. 5.0%, c  = 59.9  m) Hadronic reconstruction with HFT

HFT Performance example on the D 0 ➝ Kπ reconstruction Simulation of Hijing events with STAR tracking software including pixel pileup (RHIC-II luminosity) extrapolated to 500 M events (~one RHIC run). Identification done via topological cuts and PID using Time Of Flight

Heavy Quark Production NLO pQCD predictions of charm and bottom for the total p+p hadro-production cross sections. Renormalization scale and factorization scale were chosen to be equal. RHIC: 200, 500 GeV LHC: 900, GeV Ideal energy range for studying pQCD predictions for heavy quark production. Necessary reference for both, heavy ion and spin programs at RHIC. Estimated error bars of measurement comparable to line thickness! RHIC LHC R. Vogt

HFT - Charm Hadron v GeV Au+Au minimum bias collisions (500M events). - Charm collectivity  drag/diffusion constants  medium properties! Charm-quark flow  Thermalization of light-quarks! Charm-quark does not flow  Drag coefficients

HFT - Charm Hadron v GeV Au+Au minimum bias collisions (500M events). - Charm collectivity  drag/diffusion constants  medium properties! Charm-quark flow  Thermalization of light-quarks! Charm-quark does not flow  Drag coefficients

HFT - Charm Hadron R CP - Significant Bottom contributions in HQ decay electrons GeV Au+Au minimum bias collisions (|y|< M events). - Charm R AA  energy loss mechanism! Simulation – D 0 p T, NOT decay electron

Λ C Measurements Λ c (  p + K + π): 1)Lowest mass charm baryon 2)Total yield and Λ c /D 0 ratios can be measured. Λ c /D 0 enhancement? Measuring Λ c yield is important for charmed baryon/meson ratio.

D s Reconstruction D s → K + K - π (BR 5.5%) D s →φπ→ K + K - π (BR 2.2%) mass = ± 0.34 MeV decay length ~ 150 μm Work in progress … 200 GeV central Au+Au Ideal PID Power-law spectrum with: n = 11, = 1 GeV/c 0.5B events will work! 200 GeV Central Au+Au Collisions at RHIC

17 No cuts L/  L >6 && pixHits=2 D + -> K  Another charmed meson reconstructed using a full secondary vertex (Kalman) fit The HFT is going to reconstruct ALL major charm-carrying particles –D 0, D S, D +-, D* This is important for ‘bottom’ contribution using the ‘subtraction’ method (next slide)

Strategies for Bottom Measurement (1.a) Displaced vertex electrons (TOF+HFT) +MTD trigger? (1) All Charm states ( D 0,±, D s,  C ) (2) Charm decay electrons (Charm) (1.a) - (2) Bottom decay electrons  Some Bottom states (Statistics limited at RHIC) Measure Charm and Bottom hadron: Cross sections, Spectra and v 2   

B-meson capabilities (in progress) B->e+X approach Rate limited, not resolution

c- and b-decay Electrons - DCA cuts  c- and b-decay electron distributions and R CP GeV Au+Au minimum biased collisions (|y|< M events) H. van Hees et al. Eur. Phys. J. C61, 799(2009). (arXiv: )

Summary Detailed spectra of heavy flavor (c, b) is an invaluable piece of information First generation of detectors needs smart replacements The Heavy Flavor Tracker in STAR is the most advanced answer to this need

Spares

D s Reconstruction D s → K + K - π (BR 5.5%) D s →φπ→ K + K - π (BR 2.2%) mass = ± 0.34 MeV decay length ~ 150 μm Work in progress … 200 GeV central Au+Au Ideal PID Power-law spectrum with: n = 11, = 1 GeV/c 0.5B events will work! 200 GeV Central Au+Au Collisions at RHIC

Λ C Measurements Λ c (  p + K + π): 1)Lowest mass charm baryon 2)Total yield and Λ c /D 0 ratios can be measured. Λ c /D 0 enhancement? Measuring Λ c yield is important for charmed baryon/meson ratio.

SVT+SSD 10 Projection error is a strong function of first-layer distance and thickness

Decay e p T vs. B- and C-hadron p T The correlations between the decayed electrons and heavy flavor hadrons is weak. Key: Directly reconstructed heavy quark hadrons! Pythia calculation Xin Dong, USTC October 2005

D 0 ->K+pi Decay Length in X-Y plane ~1 c  cm counts Used ~1GeV 1 GeV/  =0 D 0 has  Un-boost in Collider ! Mean R-  value ~ 80  m Challenge: e.g. D 0 decay length For a realistic D 0 distribution, at midrapidity and ~ 1GeV/c, the average decay length is ~80μm

SSD SVT SSD+ IST PIXELS 23cm 15cm 11cm ~6.5cm 22cm 14cm 8cm 2.5cm Detector resolutions differ by a factor of two but pointing by a factor of ten. OLD (SVT)NEW (HFT).. SVT:~1.5%X0/layer PXL: %X0/layer

Partonic Energy Loss at RHIC Central Au+Au collisions: light quark hadrons and the away-side jet in back-to- back ‘jets’ are suppressed. Different for p+p and d+Au collisions. Energy density at RHIC:  > 5 GeV/fm 3 ~ 30  0 Explore pQCD in hot/dense medium R AA (c,b) measurements are needed! STAR: Nucl. Phys. A757, 102(2005).

nuclei hadron gas CSC quark-gluon plasma TETE Baryon Chemical Potential Critical Point? Temperature Early Universe T E RHIC, FAIR 1 T ini, T C LHC, RHIC 3 Phase boundary RHIC, FAIR, NICA The QCD Phase Diagram and High-Energy Nuclear Collisions The nature of thermalization at the top energy:  Heavy quarks  Di-lepton The nature of thermalization at the top energy:  Heavy quarks  Di-lepton

Quark Masses - Higgs mass: electro-weak symmetry breaking (current quark mass). - QCD mass: Chiral symmetry breaking (constituent quark mass). éStrong interactions do not affect heavy-quark mass. éNew scale compare to the excitation of the system. éStudy properties of the hot and dense medium at the foremost early stage of heavy-ion collisions. éExplore pQCD at RHIC. Total quark mass (MeV) X. Zhu, et al, Phys. Lett. B647, 366(2007).

MeasurementsRequirements Heavy Ion heavy-quark hadron v 2 - the heavy-quark collectivity - Low material budget for high reconstruction efficiency - p T coverage ≥ 0.5 GeV/c - mid-rapidity - High counting rate heavy-quark hadron R AA - the heavy-quark energy loss - High p T coverage ~ 10 GeV/c p+p energy and spin dependence of the heavy-quark production - p T coverage ≥ 0.5 GeV/c gluon distribution with heavy quarks - wide rapidity and p T coverage Requirement for the HFT

Low p T (≤ 2 GeV/c): hydrodynamic mass ordering High p T (> 2 GeV/c): number of quarks ordering s-quark hadron: smaller interaction strength in hadronic medium light- and s-quark hadrons: similar v 2 pattern => Collectivity developed at partonic stage! Partonic Collectivity at RHIC STAR: QM2009 STAR: preliminary

 -meson Flow: Partonic Flow “  -mesons (and other hadrons) are produced via coalescence of seemingly thermalized quarks in central Au+Au collisions. This observation implies hot and dense matter with partonic collectivity has been formed at RHIC” In order to test early thermalization: v 2 (p T ) of c- and b-hadrons data are needed! STAR: Phys. Rev. Lett. 99, (2007).

Charm Cross Sections at RHIC 1)Large systematic uncertainties in the measurements 2)New displaced, topologically reconstructed measurements for c- and b-hadrons are needed  Upgrade

SVT+SSD D0-vertex resolution (simulation) Left : correlation between reconstructed path length and MC Right : Decay length resolution Reco - MC [cm] MC [cm] Reco vs. MC [cm] MC [cm] Mean of the difference reconstructed -MC Rms of the difference reconstructed -MC There is no systematic shift in reconstructed quantities. The standard deviation of the distribution is flat at ~ 250  m, which is of the order of the resolution of (SSD+SVT).

Charm Baryon/Meson Ratios Y. Oh, C.M. Ko, S.H. Lee, S. Yasui, Phys. Rev. C79, (2009). S.H. Lee, K.Ohnishi, S. Yasui, I-K.Yoo, C.M. Ko, Phys. Rev. Lett. 100, (2008). QGP medium  C  pK -  + D 0  K -  -+ 2-body collisions by c and ud 3-body collisions by c, u and d

The di-Lepton Program at STAR TOF + TPC + HFT (1) σ (2) v 2 (3) R AA Mass (GeV/c 2 ) p T (GeV/c) ρ ϕ J/ψ DY, charm Bk Direct radiation from the Hot/Dense Medium Chiral symmetry Restoration  A robust di- lepton physics program extending STAR scientific reach PHENIX: