Skip to Content.
Sympa Menu

sphenix-physics-l - [Sphenix-physics-l] [minutes] bi-weekly Heavy Flavor Topical Group meeting

sphenix-physics-l AT lists.bnl.gov

Subject: sPHENIX discussion of physics

List archive

Chronological Thread  
  • From: Hideki Okawa <Hideki.Okawa AT cern.ch>
  • To: "sphenix-hf-jets-l AT lists.bnl.gov" <sphenix-hf-jets-l AT lists.bnl.gov>
  • Cc: "sphenix-physics-l AT lists.bnl.gov" <sphenix-physics-l AT lists.bnl.gov>, "sphenix-maps-l AT lists.bnl.gov" <sphenix-maps-l AT lists.bnl.gov>
  • Subject: [Sphenix-physics-l] [minutes] bi-weekly Heavy Flavor Topical Group meeting
  • Date: Tue, 9 Mar 2021 14:59:23 +0000

Heavy Flavor Topical Group Meeting (2021/3/8)
https://indico.bnl.gov/event/10963/


Introduction - Jin (BNL)

Completion of the MDC1 samples!

Wei: Do we plan to make minbias samples?
Jin: Not for MDC1. The target is to check the signal efficiency.
Wei: With minbias, the efficiency will change. So, the point
      is to just see the peak?
Jin: For MDC1, yes. For BG studies, we also need the fastsim.

Zhaozhong: The day light saving time will start soon.
Jin: We will stick to the same time in ET for now.


MDC1 status & updates -  Cameron (LANL)

Added more options in KFParticle.

p.5:
Hideki: We will definitely need jet samples for 2021-2025.
Jin: Tracking is now stable. We are ready to produce jetty
      samples included Hijing embedded ones. We will also
      need to do fake jet studies.
Ming: What is the expected integ. lumi. for pp?
Jin: For the calorimeter trigger case, 62 pb-1.


Vertex performance with ACTS - Dan (Colorado)

Yen-Jie: You should also check the RMS and not just
      a Gaussian fit, since there is a large tail.

Hideki: Which sample are you running over?
Dan: I produced by myself.
Jin: The events are dominated by ccbar.

p.6:
Jin: You need to first check the DCA calculation deeper.
Yen-Jie: The DCA looks asymmetric for the light-jets.
      There must be a bug.
Jin: Which DCA is this?
Dan: The z direction.
Jin: Please also check the r-phi direction. We will follow
      up offline for the details.
Joe: Is the DCA straight out of the Svtx track objects?
Dan: No, I calculate separately.
Jin: The module is old and the code has changed a lot in
      the past 3 years. The DCA calculation in the analysis
      package needs to be revisited.


b-tag calibration - Sebastian (Iowa State)

p.4:
Hideki: Which jet flavor ID is used here? Truth parton or
      hadron?
Sebastian: Truth hadron.
Jin: What is the pt cut of jets?
Sebastian: 20 GeV.
Jin: For low pt, the decays can go out of the jet cone. Are
      all the track DCAs inside the jets? We may want to
      consider variable jet size.
Sebastian: Yes, DCAs are all inside the jets. Varying R
      would be tough for the calibration, etc.
Hideki: We at least have jets with various R. We should
      keep in close touch with the Jet TG, as they should be
      calibrating those jets. We may be able to study the
      R-dependence.

p.9:
Hideki: Are these from ttbar events?
Sebastian: Yes, but even without asking for ttbar, we can
      enhance b-jets by just requiring the leptons.

p.10:
Hideki: What do you calibrate here?
Sebastian: The efficiency, not the variables.

General:
Hideki: For electrons, we may need to develop ID working
      points by ourselves for the b-tag. The Upsilon TG is likely
      to develop only a very loose working point for their
      analysis.
Jin: Yes, but their code will be a good starting point.

Sebastian: Is DCA signed in sPHENIX?
Jin: Yes, but one needs to re-calculate to get the sign.

Jin: This is a very nice summary. We will post it on our twiki
      as a reference.

MDC1 studies - Sebastian (Iowa State)

p.3:
Jin: Large DCA tail in ccbar. Interesting... What is the
      structure seen here?
Cameron: Cuts will bias the distributions. We should
      check. (-> Some plots posted on MatterMost now)
Jin: There must be pre-selections cutting away the prompt
      D0's here.
Sebastian: I will add descriptions on the selections used
      on the slides.
Jin: The DCA distributions should behave as seen in the
      2017 note. Let's check the pre-selections. We should
      also check the HepMC record to make sure that c's
      are not coming from the b's.

p.5:
Jin: Which integrated luminosity?
Sebastian: 6M ccbar events. Mixing bbbar samples.

p.6:
Jin: The plot style looks ok, but there may be tiny tuning
     from Camelia for the Software & Computing Review.
     Please also update the D+ plot with the sPHENIX style.


MDC1 studies: Lambda_c - Sourav (Vanderbilt)

Cameron: Selection looks sensible. This is quite a
     challenging decay. We can see the peak with
     the truth matching (posted on MatterMost).
Jin: We can check whether the cuts are still tight or not.





  • [Sphenix-physics-l] [minutes] bi-weekly Heavy Flavor Topical Group meeting, Hideki Okawa, 03/09/2021

Archive powered by MHonArc 2.6.24.

Top of Page