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Question from S&T committee Are there any simulations/estimates from STAR concerning the ability to use prior HFT-collected data to do subtraction of open-heavy flavor decays for intermediate dileptons? A: YES, we are actively working on analyses and assessment; Not really the simulation, but using dielectron yields between with and without HFT rejection of decays What was the cost/benefit analysis used to decide that there would be no new runs with the HFT in place? A: Repurpose HFT components/additional material/structure incompatibility/Slow readout

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Page 1: Question from S&T committee · Question from S&T committee •Are there any simulations/estimates from STAR concerning the ability to use prior HFT-collected data to do subtraction

Question from S&T committee• Are there any simulations/estimates from STAR concerning the ability

to use prior HFT-collected data to do subtraction of open-heavy flavor decays for intermediate dileptons? A: YES, we are actively working on analyses and assessment;Not really the simulation, but using dielectron yields between with and without HFT rejection of decays

• What was the cost/benefit analysis used to decide that there would be no new runs with the HFT in place?A: Repurpose HFT components/additional material/structure incompatibility/Slow readout

Page 2: Question from S&T committee · Question from S&T committee •Are there any simulations/estimates from STAR concerning the ability to use prior HFT-collected data to do subtraction

Mid-rapidity e+e- measurement at µB~0:Ø Connection to chiral symmetry restorationØ Thermal radiation from QGP

Low-mass di-lepton emission:T, total baryon density, and life time; more importantly dynamics of approaching Chiral Symmetry

The slope T in IMR: the true average temperature T of the medium.(no blue shift by flow)

Improvement: Factor 2 smaller systematic uncertaintiesFactor 5.5 more statistics

Tue Jun 13 10:42:27 2017

/GeV

)2

dN/d

M (c

4−10

1−10

210

+ 4 billion eventswith iTPC upgrade

= 200 GeV (MinBias)NNsAu + Au |<1ee|<1,|yeη>0.1 GeV/c, |e

Tp

Cocktail

, DYb’, bψ, ψJ/φ, ω’, η, η, 0π

PYTHIAc c

c de-correlated c

)2 (GeV/ceeM0 1 2 3 4

Dat

a/C

ockt

ai

0

1

2

Thermal Dilepton at Low and Intermediate Mass

2

iTPC upgrade essential

Page 3: Question from S&T committee · Question from S&T committee •Are there any simulations/estimates from STAR concerning the ability to use prior HFT-collected data to do subtraction

Dielectron analyses from existing HFT data

Possible study in the future on Thermal dielectron + charm-bkg with tighter cuts:

With HFT: reduces fraction of charm-bkg pairsW/o HFT: inclusive

Additional ONE run with HFT will increase the statistics by 50%

Page 4: Question from S&T committee · Question from S&T committee •Are there any simulations/estimates from STAR concerning the ability to use prior HFT-collected data to do subtraction

Significant ghost hits in low and high ptFIG. 10. HFT matching efficiency ε match HFT (a) and DCAXY (c) distributions of inclusive charged pions from real data and MC simulation in 0–10% Au+Aucollisions. The ratios between real data and GEANT simulation are shown in the bottom panels. The blue histogram depicts the true matches for which the reconstructed tracks pick up the correct MC hits in the HFT detector induced by the associated MC tracks in the GEANT simulation.

https://arxiv.org/pdf/1812.10224.pdf

Page 5: Question from S&T committee · Question from S&T committee •Are there any simulations/estimates from STAR concerning the ability to use prior HFT-collected data to do subtraction

Issues with re-installation of HFT in future runs

• HFT support structure not compatible with the current Forward upgrade• Need to change the support cone• External cables removed for eTOF (space)• PXL cooling unit has been reused for TPC cooling• Need to setup clean room for test before installation• DAQ rate is x2 slower than current TPC• IST cables/electronics/cooling reused for forward silicon tracking• Should use a faster version of the PXL sensors• Add quite some material: create background e+e- and Bremsstrahlung

radiation

Page 6: Question from S&T committee · Question from S&T committee •Are there any simulations/estimates from STAR concerning the ability to use prior HFT-collected data to do subtraction

STAR Collaboration 693 members

Difficult to define URMin other categories in an international collaboration with 15 different countries