STAR Flow, Chirality and Vorticity PWG

[subhash <subhash AT rcf.rhic.bnl.gov>]

Dear Junyi,

Since there are no further comments from anyone, I have pushed it to 
star-talks.

Thanks and regards
Subhash

On 2024-12-20 06:48 PM, "Junyi Han" wrote:
> 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