STAR Flow, Chirality and Vorticity PWG

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

Dear conveners, and all,

Thank you for your nice comments. Here is the link for the updated 
abstract.

https://drupal.star.bnl.gov/STAR/system/files/QM2022_HaojieXuv2.pdf

with best regards,
Haojie

On 2021-11-22 14:34, ShinIchi Esumi via Star-fcv-l wrote:
> Dear Haojie
>
> The followings are comments on your talk abstract from conveners.
> Best regards, Jiangyong, Prithwish and ShinIchi
>
> ---------------------------------------
>
> Jiangyong
> L2 -->dense nuclear matter in neutron stars and heavy ion collisions.
> L5 by the aforementioned strong interaction means-->in hadronic
> collisions
> L6 remove "completely apart"
> L7 traditional low-energy scatterings-->traditional method
> L12 world-wide data -->World data
> L12 effect-->implication
> Prithwish
> "by smashing isobar nuclei" -->"by colliding isobar nucleai
> "mean transverse momentum" -->"mean transverse momenta"
> "world-wide data" --> "global data"
> It's not clear what is meant by "and the recent PREX-II tension" -- do
> you mean "tension with PREX-II data" ?
> ShinIchi
> Should we mention some relations to the deformation study/talk from
> Chunjian/Jiangyong?
> This might be asked to merge later on by QM organizers. I’m fine to
> sign-off.
>
> ---------------------------------------
>
> > On Nov 16, 2021, at 13:17, webmaster--- via Star-fcv-l
> > <star-fcv-l AT lists.bnl.gov> wrote:
> >
> > Dear star-fcv-l AT lists.bnl.gov members,
> >
> > Haojie Xu (haojiexu AT zjhu.edu.cn) has submitted a material for a
> > review,
> > please have a look:
> > https://drupal.star.bnl.gov/STAR/node/57251
> >
> > ---
> > If you have any problems with the review process, please contact
> > webmaster AT www.star.bnl.gov
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