STAR Flow, Chirality and Vorticity PWG

["Junyi Han" <jyhan AT mails.ccnu.edu.cn>]

Dear Conveners,

I would like to ask there are any further suggestions? Thanks!

Best regards,

Junyi

 

 

------------------ Original ------------------

From:  "STAR Flow, Chirality and Vortici"<star-fcv-l AT lists.bnl.gov>;

Date:  Wed, Dec 18, 2024 04:22 PM

To:  "STAR Flow, Chirality and Vortici"<star-fcv-l AT lists.bnl.gov>;

Cc:  "nxu"<nxu AT lbl.gov>;

Subject:  Re: [[Star-fcv-l] ] STAR presentation by Junyi Han for INPC 2025 got commented by Subhash Singha

 

Dear Nu, Subhash, All,

Thanks for the discussion and good suggestions! I have updated it in this link: https://drupal.star.bnl.gov/STAR/system/files/INPC_2025_abstract_v4.pdf.

Thanks and best regards,

Junyi

 

 

------------------ Original ------------------

From:  "subhash"<subhash AT rcf.rhic.bnl.gov>;

Date:  Wed, Dec 18, 2024 11:00 AM

To:  "STAR Flow, Chirality and Vortici"<star-fcv-l AT lists.bnl.gov>;

Cc:  "nxu"<nxu AT lbl.gov>;

Subject:  Re: [[Star-fcv-l] ] STAR presentation by Junyi Han for INPC 2025 got commented by Subhash Singha

 

Dear Nu, Junyi, All,

Thanks, I get it now and I am fine with it if we are focussing on 3 GeV.
Then can we tweak that would imply that with high statistics 3 GeV allow
more differential measurements in y, pt space, and possibility of v2 of
hyper-nuclei species. In present version, it is not evident what is new
we are offering at these energies. Here is my attempt for line#6-9:

In this presentation, we report on the directed flow (v1) and elliptic
flow (v2) of hyper-nuclei, including lambda, H3L, H4L, and He4L, using
approximately 2 billion minimum-bias events from Au+Au collisions at sNN
= 3.0 GeV, collected by the STAR experiment in the fixed-target mode
during BES-II. The large event statistics will enable detailed
differential flow measurements of hyper-nuclei in rapidity (y) and
transverse momentum (pt), and extend v2 measurements to H3L, H4L, and
He4L.

Thanks and regards,
Subhash

On 2024-12-18 02:32 PM, Nu Xu wrote:
> Hi Subhash,
>
> I would suggest we stay with 3GeV for the time being as the statistics
> is the best from the energy. It is important for hyper-nuclei results
> on collectivity.
> For example, the statistics will be very poor for v2 measurements of
> hyper-nuclei.
>
> Thanks,
> Nu
>
>> On Dec 17, 2024, at 10:28 PM, subhash <subhash AT rcf.rhic.bnl.gov>
>> wrote:
>>
>> Dear Junyi,
>>
>> Then I would suggest modifying the abstract (and title) including
>> other FXT energies as well.
>>
>> Thanks and regards,
>> Subhash
>>
>> On 2024-12-18 01:41 PM, "Junyi Han" wrote:
>>> Dear Subhash,
>>> Thank you for your nice suggestions! I have update the abstract based
>>> on your suggestions, and it can be found in this link:
>>> https://drupal.star.bnl.gov/STAR/system/files/INPC_2025_abstract_v3.pdf.
>>> For hyper-nuclei v2, we don't make sure if we have enough statistics
>>> in other FXT energies to measure them. But for v1, I think we can
>>> include other FXT energies results. Thanks!
>>> Best regards,
>>> Junyi
>>> ------------------ Original ------------------
>>> From:  "webmaster"<webmaster AT star.bnl.gov>;
>>> Date:  Wed, Dec 18, 2024 03:16 AM
>>> To:  "STAR Flow, Chirality and Vortici"<star-fcv-l AT lists.bnl.gov>;
>>> Subject:  [[Star-fcv-l] ] STAR presentation by Junyi Han for INPC
>>> 2025
>>> got commented by Subhash Singha
>>> Dear star-fcv-l AT lists.bnl.gov members,
>>> Subhash Singha ( connectsubhash AT gmail.com ) has commented on a
>>> material
>>> originally submitted by Junyi Han ( jyhan AT mails.ccnu.edu.cn ) at
>>> https://drupal.star.bnl.gov/STAR/presentations/INPC-2025/Flow-measurements-hyper-and-light-nuclei-AuAu-collisions-30-GeV-RHIC-1
>>> Comment:
>>> Dear Junyi, Nice abstract. I have following comments:
>>> l#7: About 2 billion minimum bias ....
>>> l#10: p, d, t, 3He and 4He
>>> Why do you want to focus on only 3 GeV, do you plan to include flow
>>> results
>>> from other FXT energies as well?
>>> ---
>>> If you have any problems with the review process, please contact
>>> webmaster AT www.star.bnl.gov