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star-fcv-l - Re: [Star-fcv-l] STAR presentation by Gavin Wilks for SQM 2022 submitted for review

star-fcv-l AT lists.bnl.gov

Subject: STAR Flow, Chirality and Vorticity PWG

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  • From: Gavin Wilks <gwilks3 AT uic.edu>
  • To: subhash <subhash AT rcf.rhic.bnl.gov>, "STAR Flow, Chirality and Vorticity PWG" <star-fcv-l AT lists.bnl.gov>
  • Subject: Re: [Star-fcv-l] STAR presentation by Gavin Wilks for SQM 2022 submitted for review
  • Date: Thu, 3 Mar 2022 17:04:04 -0600

Upon review, I see that there was ~20M events from 2014 at 14.5 GeV. I will
make this correction.

Best,
Gavin

> On Mar 3, 2022, at 13:58, Gavin Wilks <gwilks3 AT uic.edu> wrote:
>
> Hello Subhash,
>
> Thank you for the comments.
>
> Regarding the BES-I data, I thought there were only data sets for
> 7.7,11.5,19.6,27,39, and 62.4 GeV. This is why I specify 14.6 GeV as a new
> set.
>
> Best,
> Gavin
>
>> On Mar 3, 2022, at 02:28, subhash via Star-fcv-l
>> <star-fcv-l AT lists.bnl.gov> wrote:
>>
>> Dear Gavin,
>>
>> I have a few suggestions for your consideration.
>>
>> Rephrase this line "In heavy-ion collisions, global spin alignment is a
>> preferential alignment of particles’ spin with the large orbital angular
>> momentum produced at the center of these systems".
>>
>> I feel we don't need these parts in the abstract "Finite elliptic flow
>> (v2) could affect global spin alignment by pushing more particles toward
>> the in-plane direction...will help to remove any potential bias in the
>> measurements.".
>>
>> Suggest remove "provides a new data set for Au+Au collisions at √ sNN=14.6
>> GeV" --> We already have 14.5 from BES-I. You can simply mention both 14.6
>> and 19.6 BES-II data would provide better precision.
>>
>> I don't understand what do you mean by "helping to clarify the behavior of
>> this
>> quantity"? You can mention precision measurement will allow more
>> differential studies, e.g. centrality dependence which is not possible for
>> BES-I
>>
>> "Additionally, the elliptic and triangular flow (v3) of ϕ and K∗0 can be
>> determined with higher precision and for a new collision energy." --> I
>> would suggest saying we will report high precision v3 for ϕ and K∗0 ...
>>
>> One suggestion, you can probably mention that the comparison of ϕ and K∗0
>> is interesting because their lifetime differ by factor of ten and the
>> former is less affected by hadronic re-scattering.
>>
>> Thanks and regards,
>> Subhash
>>
>> On 2022-03-03 02:46 AM, webmaster--- via Star-fcv-l wrote:
>>> Dear star-fcv-l AT lists.bnl.gov members,
>>> Gavin Wilks (gwilks3 AT uic.edu) has submitted a material for a review,
>>> please
>>> have a look:
>>> https://urldefense.com/v3/__https://nam04.safelinks.protection.outlook.com/?url=https*3A*2F*2Fdrupal.star.bnl.gov*2FSTAR*2Fnode*2F58623&amp;data=04*7C01*7Cgwilks3*40groute.uic.edu*7C82e9c2ce95054bf9aefe08d9fceffb1a*7Ce202cd477a564baa99e3e3b71a7c77dd*7C0*7C0*7C637818929934510539*7CUnknown*7CTWFpbGZsb3d8eyJWIjoiMC4wLjAwMDAiLCJQIjoiV2luMzIiLCJBTiI6Ik1haWwiLCJXVCI6Mn0*3D*7C3000&amp;sdata=Wqh4rydzTOJ*2Be9KhDUY1zV1ay0w1iFDL*2FvnOYjtuhvw*3D&amp;reserved=0__;JSUlJSUlJSUlJSUlJSUlJSUlJSUl!!P4SdNyxKAPE!U14G6VD0S82qRRFP3gTo5gl1xUwv3PhgvmGFq5BmH_ucen6SYu-xKwg3aOFLZ7JO_PxcAD-c$
>>>
>>> ---
>>> If you have any problems with the review process, please contact
>>> webmaster@https://urldefense.com/v3/__https://nam04.safelinks.protection.outlook.com/?url=http*3A*2F*2Fwww.star.bnl.gov*2F&amp;data=04*7C01*7Cgwilks3*40groute.uic.edu*7C82e9c2ce95054bf9aefe08d9fceffb1a*7Ce202cd477a564baa99e3e3b71a7c77dd*7C0*7C0*7C637818929934510539*7CUnknown*7CTWFpbGZsb3d8eyJWIjoiMC4wLjAwMDAiLCJQIjoiV2luMzIiLCJBTiI6Ik1haWwiLCJXVCI6Mn0*3D*7C3000&amp;sdata=WUb1H0zMuNGKGEyk2MNc1q*2F5fK*2FlERYuuQu*2BFgUUKo8*3D&amp;reserved=0__;JSUlJSUlJSUlJSUlJSUlJSUlJSU!!P4SdNyxKAPE!U14G6VD0S82qRRFP3gTo5gl1xUwv3PhgvmGFq5BmH_ucen6SYu-xKwg3aOFLZ7JO_KbQy499$
>>>
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>





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