STAR Flow, Chirality and Vorticity PWG

[Zhiwan Xu <zhiwanxu AT physics.ucla.edu>]

Hi Subhash,
 Thank you for the comments. I have implemented them and please have a look: 
    https://drupal.star.bnl.gov/STAR/node/60079
Regarding the "larger background", we mean that for the same collision 
energy, isobar collisions are smaller systems than Au+Au, and could have a 
larger background, especially nonflow background portion in the observed 
signal.

Best,
Zhiwan

----- Original Message -----
From: "subhash" <subhash AT rcf.rhic.bnl.gov>
To: "Zhiwan Xu" <zhiwanxu AT physics.ucla.edu>, "STAR Flow, Chirality and 
Vorticity PWG" <star-fcv-l AT lists.bnl.gov>
Sent: Monday, June 27, 2022 6:03:11 PM
Subject: Re: [Star-fcv-l] STAR presentation by Zhiwan Xu for DNP 2022 
submitted for review

Dear Zhiwan,

Nice abstract. I sign off with following suggestions:

"We present new STAR data of Au+Au collision from the Beam Energy Scan 
II, ..." --> We present new measurements from STAR in Au+Au collisions 
from the Beam Energy Scan II, where the magnetic field may last longer, 
and ...

"However, owing to the weaker magnetic field and the larger background 
in isobar collisions, these results cannot rule out a possible CME 
signal in Au+Au collisions" --> However, these results cannot rule out a 
possible CME signal in Au+Au collisions owing to the weaker magnetic 
field, and the larger background in isobar collisions.
BTW, when you say larger background, do you mean low energy Au+Au 
collisions?

" ... to investigate the sensitivity on the CME signal in ..." --> ... 
to investigate the sensitivity of the CME signal in ...

Thanks and regards,
Subhash

On 2022-06-28 04:47 AM, Zhiwan Xu via Star-fcv-l wrote:
> Dear Conveners,
>  Thank you for the comments. I have modified the abstract according to
> the suggestions, please have a look:
> https://drupal.star.bnl.gov/STAR/node/60079
> 
> Best,
> Zhiwan
> 
> ----- Original Message -----
> From: "Prithwish Tribedy via Star-fcv-l" <star-fcv-l AT lists.bnl.gov>
> To: "STAR Flow, Chirality and Vorticity PWG" <star-fcv-l AT lists.bnl.gov>
> Sent: Monday, June 27, 2022 10:55:36 AM
> Subject: Re: [Star-fcv-l] STAR presentation by Zhiwan Xu for DNP 2022
> submitted for review
> 
> Dear Zhiwan,
>    Here are my comment on your abstract. With these included I 
> sign-off.
> 
> "quark-gluon plasma drops" --> "quark-gluon plasma medium"
> 
> "which undergo the chiral magnetic effect  (CME)" --> "which can lead 
> to
> the chiral magnetic effect  (CME)"
> 
> "pre-defined  CME  signal  to  be  much smaller  than  previously
> expected" --> "pre-defined  CME  signatures to be absent"
> 
> "insufficient to rule out a possible CME signal in Au+Au collisions
> through extrapolation"
> -->
> "cannot rule out a possible CME signal in Au+Au collisions"
> 
> "with various event-shape handles" -- this sentence is not clear?
> 
> Best,
> Prithwish
> 
> On 2022-06-27 13:22, webmaster--- via Star-fcv-l wrote:
>> Dear star-fcv-l AT lists.bnl.gov members,
>> 
>> Zhiwan Xu (zhiwanxu AT physics.ucla.edu) has submitted a material for a
>> review,
>> please have a look:
>> https://drupal.star.bnl.gov/STAR/node/60079
>> 
>> ---
>> If you have any problems with the review process, please contact
>> webmaster AT www.star.bnl.gov
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