Femtoscopy of Protons, Light Nuclei, and Strange hadrons in Au+Au Collisions at the STAR experiment

 

Speaker : Ke Mi ( CCNU )


Talk time : 11:00, Duration : 01:00

STAR Forward Detector System Upgrade Status

 

Speaker : Xu Sun ( UIC )


Talk time : 10:00, Duration : 01:00

Highlights from the STAR experiment

  https://drupal.star.bnl.gov/STAR/system/files/qm2022_star_overview_v0.pdf

Speaker : Prithwish Tribedy ( BNL )


Talk time : 09:00, Duration : 01:00

Plenary I

TimeTalkPresenter
09:00Highlights from the STAR experiment ( 01:00 ) 1 filePrithwish Tribedy (BNL)
10:00STAR Forward Detector System Upgrade Status ( 01:00 ) 1 fileXu Sun (UIC)
11:00Femtoscopy of Protons, Light Nuclei, and Strange hadrons in Au+Au Collisions at the STAR experiment ( 01:00 ) 1 fileKe Mi (CCNU)

2022 Pre-QM meeting

2022-03-22 09:00
2022-04-05 12:00
America/New York
-
from Tuesday, 22 March 2022 to Tuesday, 5 April 2022
Online
Conference organizing committee information :  
Conference duration: 15 days
Format: online
 
Date: Mar. 22nd – Apr. 1st
 
Time: 9 am – 12 pm BNL time
 

Run 22 Cold QCD Offline QA - Days [054 - 060]

Speaker : Bassam Aboona


Talk time : 12:00, Duration : 00:20

 drupal.star.bnl.gov/STAR/blog/bassam/Run-22-Cold-QCD-Offline-QA-Days-054-060

Run 22 Cold QCD Offline QA - Days [054 - 060]

 

Jpsi production in isobar

 

Jpsi production in isobar

 

Jpsi production in isobar

 

HoSanKO_QM2022_v2_1.pdf

 HoSanKO_QM2022_v2_1.pdf

ZDC SMD gain factor vs. time

1.

Isobar 80-100

 

Correlations in UPC?

 

Weekly meeting (March 1, 2022)

 - David: First round of plots to use for FPS and FPOST NIM paper

Refined centrality definition in isobars

 

Updates_on_paper_proposal_II

 

Analysis_Note_Charge_Splitting_of_Directed_Flow_v1

 

Observation_of_the_electromagnetic_effect_via_charge_dependent_directed_flow_in_Au_Au_Ru_Ru_and_Zr_Zr_collisions_at__200_GeV

 

Diffusions and drift velocity garfield++ calculations for P10 and Ar+CH4+CF4 gas mixtures with more detailed steps in CF4 %