Run 17: PID Q/A Update
Updated on Tue, 2025-03-04 08:03 by jiatchisonacu. Originally created by xchu on 2025-02-25 08:20.
Reference
Speaker : Joseph Atchison
Talk time : 09:00, Duration : 00:20
https://bnl.zoomgov.com/j/1616069263?pwd=aHJIMEErQXVDVjczdnFvQ21wY2R2dz09
Updated on Tue, 2025-03-04 09:05 by jaenam. Originally created by xchu on 2025-02-25 08:17.Zoom: https://bnl.zoomgov.com/j/1616069263?pwd=aHJIMEErQXVDVjczdnFvQ21wY2R2dz09
Reference
Talk time : 08:50, Duration : 00:10
Spin/Cold-QCD PWG Session I
Updated on Tue, 2025-02-25 08:25. Originally created by xchu on 2025-02-25 08:17.Time | Talk | Presenter |
---|---|---|
09:00 | Run 17: PID Q/A Update ( 00:20 ) 1 file | Joseph Atchison |
09:20 | Run 17: Normalized Energy-Energy Correlators (NEEC) Statistical Uncertainties Through a Bootstrap Approach ( 00:20 ) 1 file | Manny Rosales (University of Kentucky) |
09:40 | Run 17 diffractive EM-jet A_N ( 00:20 ) 1 file | Xilin Liang (University of Kentucky) |
10:00 | Run 17 W+/W- cross sections and ratio ( 00:20 ) 1 file | Jae Nam (University of Kentucky) |
10:20 | Coffee break ( 00:30 ) | |
10:50 | Run 15: 200 GeV pAu Collins Analysis ( 00:20 ) 1 file | Bassam Aboona (University of Kentucky) |
11:10 | Run 15: Parallel Analysis of Collinear and TMD FJFs in pp at 200 GeV ( 00:20 ) 1 file | Chris Larson (University of Kentucky) |
11:30 | Run 15 AN of pi0 with EEmc using transversely polarised pp ( 00:20 ) 2 files | Ananya Paul (University of Kentucky) |
Run24 production_AuAu
Updated on Mon, 2025-02-24 12:52. Originally created by akio on 2025-02-24 12:52.Agenda
Updated on Mon, 2025-03-03 12:42. Originally created by akio on 2025-02-24 12:50.Run 17: A Study of An Unbiased Triggered Jet Sample
Updated on Mon, 2025-02-24 12:51. Originally created by mrosales2016 on 2025-02-24 12:46.Introduction to a subset sample of our Triggered Data ( Unbiased Triggered Jet Sample ) and provide evidence that this new sample is able recover the Min Bias ( VPDMB30 ) behavior in o
Paper Page of Measurement of Charge Correlator Ratio in pp
Updated on Wed, 2025-03-12 15:21. Originally created by youqi on 2025-02-24 12:38.Title: Measurement of the charge correlator ratio in p+p collisions at STAR
PAs: Youqi Song, Helen Caines, Isaac Mooney
Target journal: PRD or PRC
Figures:
Fig. 1. The angular separation Delta R between the truth-level and detector-level leading (subleading) tracks in jets.
Fig. 3. Fully corrected r_c vs jet p_T, compared to event generator predictions.
Conclusions: In summary, to probe for string-like fragmentation, we measure of r_c as a function of jet p_T in sqrt{s}=200 GeV p+p collisions at STAR. On average, the data show that leading charged particles in jets are more likely to be opposite signs than same sign. (In data, opposite signs occur 65% of the time and same sign 35% of the time. In PYTHIA these fractions are 68% to 32%). Compared with predictions from event generators, the fully corrected data show a weaker correlation between the leading and subleading tracks in jets. The significant difference between HERWIG and PYTHIA in their relative fractions of fragmentation vs. resonance decays might explain why their predictions for r_c are similar despite different approaches to fragmentation.
Preliminary results: page
Public presentations:
HP 24
WWND 24
CFNS npQCD workshop
QM 23 (poster)
Presentations within STAR:
04/13/23
05/11/23
07/13/23
08/10/23
08/17/23
08/22/23: preliminary request
01/17/24
03/05/25: paper proposal
03/14/25: PWGC preview
Measurement of p-phi Correlation Functions in 200 GeV Isobar Collisions
Updated on Wed, 2025-03-05 09:05 by bfu. Originally created by dongx on 2025-02-24 11:41.
Reference
Speaker : Boyang Fu
Talk time : 10:00, Duration : 00:20
FST Meeting on 02/24/2025
Updated on Mon, 2025-02-24 08:59. Originally created by sunxuhit on 2025-02-23 00:51.Start: 2025-02-25 9:00 am
update on dielectron production in Au+Au collisions at 17.3 GeV
Updated on Mon, 2025-02-24 10:25 by zli1. Originally created by xgn1992 on 2025-02-21 00:16.STAR PWGC meeting
Updated on Thu, 2025-02-20 14:20 by rksooraj. Originally created by marr on 2025-02-20 14:20.https://lbnl.zoom.us/j/99981267001?pwd=Q05nbjc3ZlgvR21TTzFpK2Jod2pJdz09, at 14:00 (GMT), duration : 00:00
STAR PWGC meeting
Updated on Thu, 2025-02-20 14:20 by rksooraj. Originally created by marr on 2025-02-20 14:20.https://lbnl.zoom.us/j/99981267001?pwd=Q05nbjc3ZlgvR21TTzFpK2Jod2pJdz09, at 14:00 (GMT), duration : 00:00
STAR PWGC meeting
Updated on Thu, 2025-02-20 14:20 by rksooraj. Originally created by marr on 2025-02-20 14:20.https://lbnl.zoom.us/j/99981267001?pwd=Q05nbjc3ZlgvR21TTzFpK2Jod2pJdz09, at 14:00 (GMT), duration : 00:00
STAR PWGC meeting
Updated on Thu, 2025-02-20 14:20 by rksooraj. Originally created by marr on 2025-02-20 14:20.https://lbnl.zoom.us/j/99981267001?pwd=Q05nbjc3ZlgvR21TTzFpK2Jod2pJdz09, at 14:00 (GMT), duration : 00:00
STAR PWGC meeting
Updated on Thu, 2025-03-27 23:05 by rksooraj. Originally created by marr on 2025-02-20 14:20.https://lbnl.zoom.us/j/99981267001?pwd=Q05nbjc3ZlgvR21TTzFpK2Jod2pJdz09, at 14:00 (GMT), duration : 00:00
- LIST of talks and posters from STAR
2) Run 22 production
- Get involved with using FWD data. PicoDsts (without tracking alignment) produced /gpfs01/star/pwg_tasks/
- Check picoDsts, see if all required information are there
3) 32 bit vs 64 bit
- Simulation study by Jason LINK.
- No major differences seen. Would like to have a physics evaluation (part of task force?)
4) GEANT4STAR task force volunteers
STAR PWGC meeting
Updated on Thu, 2025-02-20 14:20 by rksooraj. Originally created by marr on 2025-02-20 14:20.https://lbnl.zoom.us/j/99981267001?pwd=Q05nbjc3ZlgvR21TTzFpK2Jod2pJdz09, at 14:00 (GMT), duration : 00:00
STAR PWGC meeting
Updated on Thu, 2025-03-13 12:50 by rksooraj. Originally created by marr on 2025-02-20 14:20.https://lbnl.zoom.us/j/99981267001?pwd=Q05nbjc3ZlgvR21TTzFpK2Jod2pJdz09, at 14:00 (GMT), duration : 00:00
- Brief introduction from the PWG conveners (5’) [QIan Yang]
2) QM analysis status
- LIST of talks and posters from STAR
STAR PWGC meeting
Updated on Thu, 2025-02-20 14:20 by rksooraj. Originally created by marr on 2025-02-20 14:20.https://lbnl.zoom.us/j/99981267001?pwd=Q05nbjc3ZlgvR21TTzFpK2Jod2pJdz09, at 15:00 (GMT), duration : 00:00
STAR PWGC meeting
Updated on Fri, 2025-02-28 10:26 by rksooraj. Originally created by marr on 2025-02-20 14:20.https://lbnl.zoom.us/j/99981267001?pwd=Q05nbjc3ZlgvR21TTzFpK2Jod2pJdz09, at 15:00 (GMT), duration : 00:00
- Brief introduction from the PWG conveners (5’) []
2) Embedding Status
- Presentation by Xianglei Zhu
3) QM Preliminary with Run21 3 GeV
- For analyses that we are not releasing final results, could show preliminary results with SL24a production
4) Convener Managment Meeting at CM
- Scheduled for Thursday, March 6
- Let us know if you have anything to bring up for discussion