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Subject: STAR Flow, Chirality and Vorticity PWG
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Re: [Star-fcv-l] STAR presentation by Shengli Huang for Quark Matter 2023 submitted for review
- From: Shengli Huang <shengli.huang AT stonybrook.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 Shengli Huang for Quark Matter 2023 submitted for review
- Date: Wed, 6 Dec 2023 20:16:04 -0500
Dear Subhash,
Thanks for comments. The update proceeding can be found :
https://drupal.star.bnl.gov/STAR/presentations/Quark-Matter-2023/Measurements-azimuthal-anisotropies-16O16O-and-γAu-collisions-STAR
Thanks
Shengli
On Wed, Dec 6, 2023 at 1:56 AM subhash <subhash AT rcf.rhic.bnl.gov> wrote:
Dear Shengli,
Thanks for the updated version. I have a few suggestions below for your
consideration:
l#6: In these proceedings,
l#7: in 200 GeV in 16^O+16^O collisions ...
L#12-3: How about? Furthermore, the measurements of anisotropies in γ+Au
collisions are also discussed.
l#28: covers the pseudo-rapidity range around |η| <= 1.5
l#32: in different centralities.
l#46-47: The methods differ from each other in terms of how the scale
factor f is estimated
l#48: Systematic uncertainties account for the variations among the four
methods.
l#54-55: "As shown in panel (a) ... is smaller than that from
l#56: However, the values of v3(pT) shown in panel (b) are similar among
the three small systems.
l$56-57: It is consistent with the initial geometry predicted by Glauber
model calculations, which include sub-nucleon fluctuations. In such a
model, ...
l#61: Protons and neutrons can organize themselves into sub-group ....
l#64: forming an alpha cluster
l#74: 74 K \times v2{4}
l#90: in 0-10% 16^O+16^O collisions at sNN = 200 GeV ...
I sign off with these addressed.
Thanks and regards,
Subhash
On 2023-12-05 10:18 PM, Shengli Huang wrote:
> Dear Subhash,
> It is four pages now.
>
> Thanks!
> Shengli
>
> On Mon, Dec 4, 2023 at 9:14 PM subhash <subhash AT rcf.rhic.bnl.gov>
> wrote:
>
>> Dear Shengli,
>>
>> Thanks for posting your proceedings. Could you please shorten it to
>> fit
>> 4 page limit including references.
>>
>> With regards,
>> Subhash
>>
>> On 2023-12-04 11:30 PM, webmaster--- via Star-fcv-l wrote:
>>> Dear star-fcv-l AT lists.bnl.gov members,
>>>
>>> Shengli Huang (shengli.huang AT stonybrook.edu) has submitted a
>> material
>>> for a
>>> review, please have a look:
>>> https://drupal.star.bnl.gov/STAR/node/66153
>>>
>>> ---
>>> 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
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[Star-fcv-l] STAR presentation by Shengli Huang for Quark Matter 2023 submitted for review,
webmaster, 12/04/2023
-
Re: [Star-fcv-l] STAR presentation by Shengli Huang for Quark Matter 2023 submitted for review,
subhash, 12/04/2023
-
Re: [Star-fcv-l] STAR presentation by Shengli Huang for Quark Matter 2023 submitted for review,
Shengli Huang, 12/05/2023
-
Re: [Star-fcv-l] STAR presentation by Shengli Huang for Quark Matter 2023 submitted for review,
subhash, 12/06/2023
- Re: [Star-fcv-l] STAR presentation by Shengli Huang for Quark Matter 2023 submitted for review, Shengli Huang, 12/06/2023
-
Re: [Star-fcv-l] STAR presentation by Shengli Huang for Quark Matter 2023 submitted for review,
subhash, 12/06/2023
-
Re: [Star-fcv-l] STAR presentation by Shengli Huang for Quark Matter 2023 submitted for review,
Shengli Huang, 12/05/2023
-
Re: [Star-fcv-l] STAR presentation by Shengli Huang for Quark Matter 2023 submitted for review,
subhash, 12/04/2023
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