STAR Flow, Chirality and Vorticity PWG

[Prithwish Tribedy <ptribedy AT rcf.rhic.bnl.gov>]

Hello Chenlu (Xionghong),
  Here are my comments on your nice abstract -- with these included I 
sign off.

line 8:
"v1" --> "v_1" everywhere
"have been" --> "has been"

line 9:
"all particle ranging" --> "different particle species"

Why did you choose 5-40%, your earlier studies were done for 0-60%:
https://drupal.star.bnl.gov/STAR/system/files/ChenluHu_Directed_Flow_H3L_H4L_PWG_20200916%282%29.pdf

"This is part of the beam energy scan program carried by
the STAR experiment in 2018."
-->
"This is part of the fixed target program carried by
the STAR experiment in 2018."

"About 2700 and 4200 ^3_\Lamda H from"
-->
"About 2700 and 4200 ^3_\Lamda H candidates from"

"decay and about 5300 ^4_\Lamda H "
-->
"decay respectively, and about 5300 ^4_\Lamda H candidates"

"compared with this of the"
-->
"compared with that of the"

" dv1/dy slope of the "
-->
either say "slope of v_1 with rapidity for the"
or just say "dv1/dy magnitude for the"


Best,
Prithwish



On 2021-02-02 03:03, Xionghong He via Star-fcv-l wrote:
> Dear all,
>
> This is the abstract from Chenlu Hu (huchenlu AT impcas.ac.cn).
> She has problem logining the drupal webpage. Sorry about the confusion.
>
> Best regards,
>
> Xionghong
>
>
> 在 2021/2/2 15:53, webmaster--- via Star-fcv-l 写道:
> > Dear star-fcv-l AT lists.bnl.gov members,
> >
> > Xionghong He (hexh AT impcas.ac.cn) has submitted a material for a 
> > review,
> > please have a look:
> > https://drupal.star.bnl.gov/STAR/node/53562
> >
> > ---
> > If you have any problems with the review process, please contact
> > webmaster AT www.star.bnl.gov
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