Skip to Content.
Sympa Menu

star-fcv-l - Re: [Star-fcv-l] STAR presentation by Ding Chen for NNPSS 2022 submitted for review

star-fcv-l AT lists.bnl.gov

Subject: STAR Flow, Chirality and Vorticity PWG

List archive

Chronological Thread  
  • From: Ding Chen <dchen087 AT ucr.edu>
  • To: subhash <subhash AT rcf.rhic.bnl.gov>
  • Cc: "STAR Flow, Chirality and Vorticity PWG" <star-fcv-l AT lists.bnl.gov>
  • Subject: Re: [Star-fcv-l] STAR presentation by Ding Chen for NNPSS 2022 submitted for review
  • Date: Wed, 22 Jun 2022 09:15:41 -0400

Dear Subhash,

Thank you for your kind sign-off. I've updated with version 3 according to your nice comments! 

By anisotropic flow do you mean v1 or, v2 or, both? You can probably
clarify it in the abstract.
I intend to show v1 only this time. Thank you for the reminder to be more specific.

Title: If you indicate both, then you can consider: Anisotropic flows
--> Directed and elliptic flow of ... or, Directed flow of ...
programs --> program
Done.

line 12: anisotropic flow (v1, v2) of ϕ mesons in Au+Au collisions at
... GeV  from the second phase of RHIC ....
Done.

Thanks again!

Cheers,
Ding 





 
 

On 2022-06-22 12:45 PM, Ding Chen wrote:
> Dear Subhash,
>
> I've updated a  version 2 in the same link according to your nice
> comments:
> https://drupal.star.bnl.gov/STAR/node/60017
>
> Let me know if you have any more questions or comments,
>
> Best regards,
> Ding
>
> On Tue, Jun 21, 2022 at 10:37 PM subhash via Star-fcv-l
> <star-fcv-l AT lists.bnl.gov> wrote:
>
>> Dear Ding,
>>
>> Nice abstract. A few suggestions for your consideration.
>>
>> Title: Anisotropic flow of ϕ mesons.... (here and elsewhere)
>> I think FXT is a part of BES program. So you don't have to separate
>> BES
>> and FXT. Also you can mention the beam energy that you will be
>> reporting
>> here and also in the main text.
>>
>> line 8-9: ... and has a small hadronic interaction cross-section,
>> which
>> reduces the influence of late stage rescattering in heavy-ion
>> collisions.
>>
>> line 10: ... is sensitive to the early stages of the collisions and
>> is
>> an important observable for the study of ....
>>
>> line 16: You already have BES defined in line-13. So BES-I should
>> work
>> here.
>>
>> Thanks and regards,
>> Subhash
>>
>> On 2022-06-22 09:47 AM, webmaster--- via Star-fcv-l wrote:
>>> Dear star-fcv-l AT lists.bnl.gov members,
>>>
>>> Ding Chen (dchen087 AT ucr.edu) has submitted a material for a
>> review,
>>> please
>>> have a look:
>>> https://drupal.star.bnl.gov/STAR/node/60017
>>>
>>> ---
>>> 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