Blast-Wave inspired fit of light nuclei spectra in FXT Au+Au collisions at 3 GeV and comparied to BES-I
Updated on Mon, 2021-06-07 07:11. Originally created by huiliu on 2021-06-07 05:36.Lambda dN/dy Comparison of BES-I and UrQMD at √s = 27 GeV
Updated on Mon, 2021-06-07 04:10. Originally created by harasty on 2021-06-07 04:10.Reference
Speaker : Matthew Harasty
Talk time : 10:00, Duration : 00:20
Follow-up on action items
Updated on Sun, 2021-06-13 18:53. Originally created by yezhenyu on 2021-06-06 13:52.Speaker : all
Talk time : 08:30, Duration : 00:10
************* From June 7 *************
Production Status:
1) Completed:
Pre-installation Testing
Updated on Mon, 2021-06-14 07:36 by sunxuhit. Originally created by yezhenyu on 2021-06-06 13:52.Speaker : Xu Sun, Gavin Wilks, Yu Hu ( UIC, Fudan )
Talk time : 09:10, Duration : 00:10
Production module assembly
Updated on Mon, 2021-06-14 04:06 by shenghui. Originally created by yezhenyu on 2021-06-06 13:52.Speaker : Shenghui Zhang, Gavin Wilks ( UIC )
Talk time : 09:00, Duration : 00:10
Inner and Outer Signal Cables
Updated on Sun, 2021-06-06 13:52. Originally created by yezhenyu on 2021-06-06 13:52.Speaker : Michael Capotosto ( BNL )
Talk time : 08:50, Duration : 00:10
Integration and Cooling System
Updated on Sun, 2021-06-06 13:52. Originally created by yezhenyu on 2021-06-06 13:52.Speaker : Rahul Sharma, Felix Archampong ( BNL )
Talk time : 08:40, Duration : 00:10
STAR Forward Silicon Tracker Meeting
Updated on Sun, 2021-06-06 13:52. Originally created by yezhenyu on 2021-06-06 13:52. 2021-06-14 08:30
America/New York
Monday, 14 June 2021
Zoom meeting ID: 87904302955 Passcode: fSTAR2021, at 12:30 (GMT), duration : 00:00
Zoom meeting ID: 87904302955 Passcode: fSTAR2021, at 12:30 (GMT), duration : 00:00
| Time | Talk | Presenter |
|---|---|---|
| 08:30 | Follow-up on action items ( 00:10 ) 0 files | all |
| 08:40 | Integration and Cooling System ( 00:10 ) 0 files | Rahul Sharma, Felix Archampong (BNL) |
| 08:50 | Inner and Outer Signal Cables ( 00:10 ) 0 files | Michael Capotosto (BNL) |
| 09:00 | Production module assembly ( 00:10 ) 2 files | Shenghui Zhang, Gavin Wilks (UIC) |
| 09:10 | Pre-installation Testing ( 00:10 ) 1 file | Xu Sun, Gavin Wilks, Yu Hu (UIC, Fudan) |
Follow-up on action items
Updated on Sun, 2021-06-06 14:02. Originally created by yezhenyu on 2021-06-06 13:52.Speaker : all
Talk time : 08:30, Duration : 00:10
************* From May 24 *************
Production Status:
1) Completed:
Integration and Cooling System
Updated on Sun, 2021-06-06 13:52. Originally created by yezhenyu on 2021-06-06 13:52.Speaker : Rahul Sharma, Felix Archampong ( BNL )
Talk time : 08:40, Duration : 00:10
Inner and Outer Signal Cables
Updated on Sun, 2021-06-06 13:52. Originally created by yezhenyu on 2021-06-06 13:52.Speaker : Michael Capotosto ( BNL )
Talk time : 08:50, Duration : 00:10
Production module assembly
Updated on Sun, 2021-06-06 20:09 by shenghui. Originally created by yezhenyu on 2021-06-06 13:52.Speaker : Shenghui Zhang ( UIC )
Talk time : 09:00, Duration : 00:10
Pre-installation Testing
Updated on Mon, 2021-06-07 08:22 by huyu. Originally created by yezhenyu on 2021-06-06 13:51.Speaker : Xu Sun, Yu Hu, Gavin Wilks ( UIC, Fudan )
Talk time : 09:10, Duration : 00:10
STAR Forward Silicon Tracker Meeting
Updated on Sun, 2021-06-06 13:51. Originally created by yezhenyu on 2021-06-06 13:51. 2021-06-07 08:30
America/New York
Monday, 7 June 2021
Zoom meeting ID: 87904302955 Passcode: fSTAR2021, at 12:30 (GMT), duration : 00:00
Zoom meeting ID: 87904302955 Passcode: fSTAR2021, at 12:30 (GMT), duration : 00:00
| Time | Talk | Presenter |
|---|---|---|
| 08:30 | Follow-up on action items ( 00:10 ) 0 files | all |
| 08:40 | Integration and Cooling System ( 00:10 ) 0 files | Rahul Sharma, Felix Archampong (BNL) |
| 08:50 | Inner and Outer Signal Cables ( 00:10 ) 0 files | Michael Capotosto (BNL) |
| 09:00 | Production module assembly ( 00:10 ) 1 file | Shenghui Zhang (UIC) |
| 09:10 | Pre-installation Testing ( 00:10 ) 2 files | Xu Sun, Yu Hu, Gavin Wilks (UIC, Fudan) |
matter and antimatter asymmetry
Updated on Sun, 2021-06-06 10:18. Originally created by yiyang on 2021-06-06 10:07.We show that the matter-antimatter asymmetry in the present-day universe is mainly due to the highly suppressed detection probability of antimatter, which is a direct result of the Dirac-Feynman
JetCorr PWG QA
Updated on Fri, 2021-06-04 11:49. Originally created by tongliu on 2021-06-04 11:49.JetCorr PWG QA
Updated on Fri, 2021-06-04 11:49. Originally created by tongliu on 2021-06-04 11:49.JetCorr PWG QA
Updated on Fri, 2021-06-04 11:49. Originally created by tongliu on 2021-06-04 11:49.Bulkcorr_QA_Au17p3_O200
Updated on Fri, 2021-06-04 11:00. Originally created by apandav on 2021-06-04 11:00.Reference
Speaker : Ashish Pandav
Talk time : 12:50, Duration : 00:20