Skip to Content.
Sympa Menu

star-fcv-l - Re: [Star-fcv-l] STAR presentation by Niseem Magdy Abdelwahab Abdelrahman for CPOD March Meeting 2021 submitted for review

star-fcv-l AT lists.bnl.gov

Subject: STAR Flow, Chirality and Vorticity PWG

List archive

Chronological Thread  
  • From: Niseem <niseemmagdy AT yahoo.com>
  • To: Prithwish Tribedy via Star-fcv-l <star-fcv-l AT lists.bnl.gov>
  • Subject: Re: [Star-fcv-l] STAR presentation by Niseem Magdy Abdelwahab Abdelrahman for CPOD March Meeting 2021 submitted for review
  • Date: Tue, 2 Feb 2021 09:32:19 -0600

Hi Prithwish,

Thanks for the nice comments.

Please find the updated abstract at the same link,

https://drupal.star.bnl.gov/STAR/node/53482

For your comments,

It is not clear what this new observable is C2(Δη,Δφ) does not clearly indicate that you're measuring transverse momentum correlations.
>> It's written that C2(Δη, Δφ) is the “longitudinal two-particle momentum correlations”


Do you think you'll be done with systematics by CPOD
>>The standard systematics i.e. tracks and events variations exist, currently along with others we are working on the systematics associated with the extraction of the \eta/s



I remember you looked at \rho for three energies:
https://drupal.star.bnl.gov/STAR/system/files/Flow_PT_5.pdf
Did you look at all other energies for 200-11.5 GeV, if not do you plan to update soon ? Or I missed it?
>>I’m working on including some of the lower beam energies, however, I rephrased the sentence to reflect the energy range for the different measurements


Thanks,
Niseem


On 2/2/21 7:59 AM, Prithwish Tribedy via Star-fcv-l wrote:
Hi Niseem,
  Looks good, please consider the following suggestions. I'll sign off once these are included.

"The beam-energy of the transverse momentum correlations; Implication for the η/s
extraction"
-->
"The beam-energy dependence of the transverse momentum correlations and implication for the η/s
extraction"

"The ongoing heavy-ion programs’ primary aim is to"
-->
"One of the primary aim of the ongoing heavy-ion programs is to"

Remove "formed in high-energy heavy ion collisions"

"further constraints for more robust extractions of η/s(T)"
-->
"further constraints on the extractions of η/s(T)"

"required for the initial-state and the T"
-->
"required for the uncertainties on the initial-state and the T"

"dependence of η/s.The recent"
-->
"dependence of η/s.(ADD SPACE)The recent"

"correlations, C2(Δη,Δφ)[1,2], and"
-->
"correlations, C2(Δη,Δφ)(ADD SPACE)[1,2], and"


"add an additional constrain"
-->
"add additional constraints"


"are compared with similar studies"
-->
"will be compared to similar measurements"

"to several theoretical calculations"
-->
"to theoretical calculations"

Some general comments/question:

It is not clear what this new observable is C2(Δη,Δφ) does not clearly indicate that you're measuring transverse momentum correlations.

Do you think you'll be done with systematics by CPOD

I remember you looked at \rho for three energies:
https://drupal.star.bnl.gov/STAR/system/files/Flow_PT_5.pdf
Did you look at all other energies for 200-11.5 GeV, if not do you plan to update soon ? Or I missed it?


Best,
Prithwish


On 2021-01-29 10:16, webmaster--- via Star-fcv-l wrote:
Dear star-fcv-l AT lists.bnl.gov members,

Niseem Magdy Abdelwahab Abdelrahman (niseemmagdy AT yahoo.com) has submitted a
material for a review, please have a look:
https://drupal.star.bnl.gov/STAR/node/53482

---
If you have any problems with the review process, please contact
webmaster AT www.star.bnl.gov
_______________________________________________
Star-fcv-l mailing list
Star-fcv-l AT lists.bnl.gov
https://lists.bnl.gov/mailman/listinfo/star-fcv-l
_______________________________________________
Star-fcv-l mailing list
Star-fcv-l AT lists.bnl.gov
https://lists.bnl.gov/mailman/listinfo/star-fcv-l



Archive powered by MHonArc 2.6.24.

Top of Page