Dear ShinIchi,
I have uploaded a new version of my poster with your suggestions, thank you for your comments.
https://drupal.star.bnl.gov/STAR/system/files/Quark_Matter_Poster_Updated_v3.pdf
Best regards,
Jonathan Ball
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Today's Topics:
1. Re: QM22 poster from Jonathan Ball (ShinIchi Esumi)
2. Re: STAR presentation by Ke Mi for Quark Matter 2022
submitted for review (Ke Mi)
----------------------------------------------------------------------
Message: 1
Date: Thu, 31 Mar 2022 23:06:29 +0900
From: ShinIchi Esumi <esumi.shinichi.gn AT u.tsukuba.ac.jp>
To: STAR Correlations and Fluctuations PWG <star-cf-l AT lists.bnl.gov>
Cc: "Ball Cap, Jonathan Gonzalo" <jballcap AT Central.UH.EDU>
Subject: Re: [Star-cf-l] QM22 poster from Jonathan Ball
Message-ID: <003F6BBC-E3C1-4078-A093-E9EE921E0C91 AT u.tsukuba.ac.jp>
Content-Type: text/plain; charset="utf-8"
Dear Jonathan, I forgot to mention the following reason for the comparison between
your net-lambda and submitted net-proton fluctuation at the same energy with the
same dataset. From the comparison, the basic trend is quite similar (although the quite
different magnitude) with respect to the net-proton results, so that you might be able to
say the dominant mechanism would be similar including the baryon-conservation etc
and could also would give an additional confidence of both results...
Best regards, ShinIchi
> On Mar 31, 2022, at 22:51, ShinIchi Esumi via Star-cf-l <star-cf-l AT lists.bnl.gov> wrote:
>
> Dear Jonathan
> Thank you for the nice study and result for your poster.
> I find your poster very good and send you a few comments for a possible improvement.
> In future, you could also try to apply a new purity correction that is proposed by Toshihiro,
> as you might know from :
https://urldefense.com/v3/__https://arxiv.org/abs/2202.06953__;!!P4SdNyxKAPE!Uzd0_XmVrEIKX_25Wjnk_VxFh_w7JwHsywjistBOyDvXPWwHN0ZVMU6VVIxtAUeYdQSoKV0$ <https://urldefense.com/v3/__https://arxiv.org/abs/2202.06953__;!!P4SdNyxKAPE!SFqGw7PyrxVsqb-6avyIl3dVIRiyx4WLiVzKL1D0rTtajR5PospHazcOKss7strL4iOtL8E$>
> Best regards, ShinIchi
>
> P4: I would include a small inset panel in each of all 7 panels in this page, in order to
> compare the trend with the net-proton data from submitted 3GeV FXT paper that will
> also be shown in Yu Zhang?s talk, where the magnitude is quite different, so that we
> can not overlay the points in your plot, therefore I?m suggesting to add a small inset panel
> in each of 7 plots showing c1~c4 and 3 ratios vs Npart, that can be taken from Yu?s slide
> p12 in his talk. Within this inset panel, you could overlay your points, if you like to.
>
> P5: Please increase the symbol size especially for the experimental data points as well as
> for the ones from UrQMD at 3GeV. The yellowish (or gold color) is not really visible, maybe
> just because of the size and line width, but I would guess you can not change with line width,
> if it indicates the systematic/statistical errors in the model. (Please also indicate the meaning
> of the line width in the plot.) At least, all the point size can be enlarged, but I would also
> choose some other color like red or dark-red/dark-green etc for UrQMD.
>
>> On Mar 30, 2022, at 15:45, Ball Cap, Jonathan Gonzalo <jballcap AT Central.UH.EDU <mailto:jballcap AT Central.UH.EDU>> wrote:
>>
>> Dear ShinIchi,
>>
>> You can find my updated poster in the following link:
>>
https://urldefense.com/v3/__https://drupal.star.bnl.gov/STAR/node/58753__;!!LkSTlj0I!A8u8IJT35HnKL_bEqdaZVW5snFbWiYcAuoJ3c6y4xIN1AGH7pVyE3lqE0gvyw_XEqQAlz1ve4UD8UEPG5hODqXOK6Piu0QBUHj4DGQ0$ <https://urldefense.com/v3/__https://drupal.star.bnl.gov/STAR/node/58753__;!!LkSTlj0I!A8u8IJT35HnKL_bEqdaZVW5snFbWiYcAuoJ3c6y4xIN1AGH7pVyE3lqE0gvyw_XEqQAlz1ve4UD8UEPG5hODqXOK6Piu0QBUHj4DGQ0$
>
>>
>> Best regards,
>> Jonathan Ball
>> From: ShinIchi Esumi <esumi.shinichi.gn AT u.tsukuba.ac.jp <mailto:esumi.shinichi.gn AT u.tsukuba.ac.jp>>
>> Sent: Sunday, March 27, 2022 9:05 AM
>> To: Ball Cap, Jonathan Gonzalo <jballcap AT Central.UH.EDU <mailto:jballcap AT Central.UH.EDU>>
>> Cc: ShinIchi Esumi <esumi.shinichi.gn AT u.tsukuba.ac.jp <mailto:esumi.shinichi.gn AT u.tsukuba.ac.jp>>
>> Subject: QM22 poster
>>
>> Dear Jonathan
>> I has been assigned to review your poster for QM22 by
>> the STAR management, but I might have missed your E-mail
>> to CF or to STAR mailing list, so please remind me the web
>> location of your poster for QM22? Thank you and I?m looking
>> tor seeing your nice results.
>> Best regards, ShinIchi
>
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Message: 2
Date: Thu, 31 Mar 2022 16:33:51 +0200
From: Ke Mi <mike1996 AT mails.ccnu.edu.cn>
To: Xiaofeng Luo <xfluo.star AT hotmail.com>, STAR Correlations and
Fluctuations PWG <star-cf-l AT lists.bnl.gov>
Subject: Re: [Star-cf-l] STAR presentation by Ke Mi for Quark Matter
2022 submitted for review
Message-ID: <40EA0892-9442-4092-A098-ABB1389BDAD5 AT mails.ccnu.edu.cn>
Content-Type: text/plain; charset="utf-8"
Dear Xiaofeng,
Thank you so much for the suggestions and sign-off. I?ve implemented them all.
Please check the update version through same link:https://urldefense.com/v3/__https://drupal.star.bnl.gov/STAR/node/58953__;!!LkSTlj0I!A8u8IJT35HnKL_bEqdaZVW5snFbWiYcAuoJ3c6y4xIN1AGH7pVyE3lqE0gvyw_XEqQAlz1ve4UD8UEPG5hODqXOK6Piu0QBUhxDKTtI$ <https://urldefense.com/v3/__https://drupal.star.bnl.gov/STAR/node/58953__;!!LkSTlj0I!A8u8IJT35HnKL_bEqdaZVW5snFbWiYcAuoJ3c6y4xIN1AGH7pVyE3lqE0gvyw_XEqQAlz1ve4UD8UEPG5hODqXOK6Piu0QBUhxDKTtI$
>
For the pXi result, yes, it?s consistent with Yingjie?s latest result.
Thank you.
Best regards,
Ke
> On 31. Mar 2022, at 12:43, Xiaofeng Luo via Star-cf-l <star-cf-l AT lists.bnl.gov> wrote:
>
> Hi Ke,
>
> Nice presentation.
> Please find my comments/suggestions below :
>
> 1. slide 3, you may add some reference for this slide.
> 2. slide 7, please put the text TPC PID and TOF PID to the empty place in this page, not covering the figures.
>
> 3. slide 11, please make sure the results shown here is consistent with Yingjie's final p-Xi results.
>
> 4. slide 2, please modify the 3rd part to :
> Two-particle femtoscopy :
> 1) Meson-Meson (ks-ks)
> 2) Baryon-Baryon (p-p, p-Xi)
> 3) Light Nuclei (p-d, d-d)
>
> 5. slide 6, the resolution of right figure is not good, please use the one in Yu Zhang's talk with better resolution.
>
> 6. In slide 13 and 14, the legend L-L model is confusion if people only see the Figure, please spell it out as : Lednicky Model
>
> 7. In the bottom of slide 16, add "Stay tuned for the RHIC BES-II"
>
> 8. Summary: d-d has larger source size -> d-d has larger emission source size
>
> With those implemented, I sign off.
>
> Thank you,
> Best Regards,
> Xiaofeng
>
> On 2022/3/21 5:32 PM, webmaster--- via Star-cf-l wrote:
>> Dear star-cf-l AT lists.bnl.gov members,
>>
>> Ke Mi (mike1996 AT mails.ccnu.edu.cn) has submitted a material for a review,
>> please have a look:
>>
https://urldefense.com/v3/__https://drupal.star.bnl.gov/STAR/node/58953__;!!LkSTlj0I!A8u8IJT35HnKL_bEqdaZVW5snFbWiYcAuoJ3c6y4xIN1AGH7pVyE3lqE0gvyw_XEqQAlz1ve4UD8UEPG5hODqXOK6Piu0QBUhxDKTtI$
>>
>> ---
>> If you have any problems with the review process, please contact
>> webmaster AT www.star.bnl.gov
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>
> --
> Xiaofeng Luo
> Professor of Physics
> College of Physical Science and Technology
> Central China Normal University
> Luoyu Road 152, Wuhan China
> Office Phone #: +86-27-67867500
>
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