STAR HardProbes PWG

[Yi Yang <yiyang0429 AT gmail.com>]

Hi Priyanka,

Thanks a lot for the nice abstract. I don't have any comments on it.

Cheers,

Yi

On Thu, Dec 1, 2022 at 3:55 PM Barbara Trzeciak via Star-hp-l <star-hp-l AT lists.bnl.gov> wrote:

Hi Priyanka, 

the new version looks good, I sign off.

Cheers,

Barbara 

On Wed, 30 Nov 2022, 20:47 Sooraj Radhakrishnan via Star-hp-l, <star-hp-l AT lists.bnl.gov> wrote:

Hi Priyanka,

   Thanks for the updated version. I sign off

Sooraj

On Wed, Nov 30, 2022 at 6:53 AM Roy Chowdhury Priyanka (DOKT) <priyanka.roy_chowdhury.dokt AT pw.edu.pl> wrote:

Hi Sooraj, all, 

Thanks for your feedback. I have implemented your comments and uploaded the updated version here https://drupal.star.bnl.gov/STAR/system/files/HP2023_abstract_Priyanka.pdf

I agree with your suggestion that we need some suitable model calculation to check the sensitivity of interaction strength with these femtoscopic correlations. Unfortunately, there's no such existing model. We can look into this in the future. 

Regards,

Priyanka

---

From: Sooraj Radhakrishnan <skradhakrishnan AT lbl.gov>
Sent: Tuesday, November 29, 2022 9:14 PM
To: Roy Chowdhury Priyanka (DOKT) <priyanka.roy_chowdhury.dokt AT pw.edu.pl>; STAR HardProbes PWG <star-hp-l AT lists.bnl.gov>
Cc: Nihar Sahoo <nihar AT rcf.rhic.bnl.gov>; webmaster AT star.bnl.gov <webmaster AT star.bnl.gov>
Subject: Re: [Star-hp-l] STAR presentation by Priyanka Roy Chowdhury for Hard Probes 2023 submitted for review

 

Hi Priyanka,

   Thanks for preparing the nice abstract and the updates. The abstract reads good to me.  

A few minor comments

Is the font size different for part of first line?

L8: in Au+Au collisions

L8: using data taken

Regarding the above discussion, with the sensitivity to the emission region or the region of homogeneity, its not clear how non-identified correlations with D0 where the mass is much different is helpful. On the other hand, these femtoscopic correlations should be sensitive to the interaction strengths between D0-hadrons and potentially charm and light partons. The sensitivity to screening length is also plausible then. It would be good if there are some model calculations that look into sensitivity to the interaction strengths with these femtoscopic correlations. If there are such studies existing, could be referenced in the abstract

thanks

Sooraj

On Tue, Nov 29, 2022 at 5:30 AM Roy Chowdhury Priyanka (DOKT) via Star-hp-l <star-hp-l AT lists.bnl.gov> wrote:

Hello Nihar, Barbara, all

I have modified my abstract to incorporate your suggestions. You can find the modified version here https://drupal.star.bnl.gov/STAR/system/files/HP2023_abstract_Priyanka.pdf

Regards,

Priyanka

---

From: Nihar Sahoo <nihar AT rcf.rhic.bnl.gov>
Sent: Tuesday, November 29, 2022 12:22 PM
To: Roy Chowdhury Priyanka (DOKT) <priyanka.roy_chowdhury.dokt AT pw.edu.pl>
Cc: webmaster AT star.bnl.gov <webmaster AT star.bnl.gov>; STAR HardProbes PWG <star-hp-l AT lists.bnl.gov>; Barbara Trzeciak <barbara.trzeciak AT gmail.com>
Subject: Re: [Star-hp-l] STAR presentation by Priyanka Roy Chowdhury for Hard Probes 2023 submitted for review

 

Hello Priyanka,

Thank you for implementing my comments and correcting me.

Please upload your new version here (do not send in the attachment)
https://drupal.star.bnl.gov/STAR/node/61809

> of " low relative momentum": For femtoscopic correlation, 'relative
> momentum' (k*) is from the reference of relative momentum between two
> particles for which pair we calculate correlation function C(k*).

Yes, you are correct. Never mind to that.

I have a few additional comment on your updated abstract. With
implementing these I sign off.


1) "Due to large mass, the charm quarks are produced early in the
relativistic heavy-ion reactions…"
It doesn't sound good. (because Charm quarks are produced early in the
collision "not" because they are heavy but they come mainly from hard
scattering)

"The heavy quarks—-like charm quarks—-are produced early in the
relativistic heavy-ion collisions…"
How about this?

2) "…in the high-statistics Au-Au collision (run 2014) at √sNN =200 GeV
at the STAR experiment." -> "...in Au-Au collisions at sqrt(sNN)=200 GeV
data taken in the year 2014." (high-statistics not required.)

3) "reconstructed at via the K--π+ decays using topological
reconstruction enabled by the excellent…
" -> "reconstructed via the K^{-}- π+ decay channel using topological
criteria enabled by the excellent…"
(Just to avoid "reconstructed" and "reconstruction" in the same
sentence)

4) "Hadrons are selected and identified…" -> "Hadrons are
identified…using Time-of-Flight and time projection chamber detectors."


Cheers
Nihar


On 2022-11-28 20:31, Roy Chowdhury Priyanka (DOKT) wrote:
> Hello Barbara and Nihar,
>
>  Thanks for your comments and feedback.
>
>  Here's a clarification regarding the motivation of the analysis
> (asked by Barbara).
>
>  Explanation: Two-particle femtoscopic correlation is a useful method
> to study the Debye screening length of c/cquarks within the QGP
> medium. By fitting the analytical result into the suitable model (ex.
> Lednicky & Lyuboshitz), source size can be calculated. For strong
> correlation, the source size is expected lower than the size of the
> fireball and vice-versa.
>
>  If required, I can add this explanation to my abstract.
>
>  Regarding the suggestion by Nihar, " relatively low momentum" instead
> of " low relative momentum": For femtoscopic correlation, 'relative
> momentum' (k*) is from the reference of relative momentum between two
> particles for which pair we calculate correlation function C(k*).
>
>  I tried to address all your suggestions. Please check my modified
> abstract attached here.
>
>  Regards,
>
>  Priyanka
>
> -------------------------
>
> From: Star-hp-l <star-hp-l-bounces AT lists.bnl.gov> on behalf of Nihar
> Sahoo via Star-hp-l <star-hp-l AT lists.bnl.gov>
> Sent: Sunday, November 27, 2022 12:16 PM
> To: webmaster AT star.bnl.gov <webmaster AT star.bnl.gov>; STAR HardProbes
> PWG <star-hp-l AT lists.bnl.gov>
> Subject: Re: [Star-hp-l] STAR presentation by Priyanka Roy Chowdhury
> for Hard Probes 2023 submitted for review
>
> Hello Priyanka,
>
> Please find my comment on your nice abstract.
>
> Title: drop "registered"
>
> "Due to their large mass, charm quarks.." -> "Due to large mass, the
> charm quarks…"
> "…the created system, including…" -> "the created medium— the
> Quark
> Gluon Plasma."
> "at low relative momentum…" -> " …at relatively low momentum…"
>
> Please mention about the kinematic range of D-meson and hadrons; what
> centrality, analysis details, etc.
>
> Cheers
> Nihar
>
> On 2022-11-21 20:01, webmaster--- via Star-hp-l wrote:
>> Dear Star-hp-l AT lists.bnl.gov members,
>>
>> Priyanka Roy Chowdhury (priyanka.roy_chowdhury.dokt AT pw.edu.pl) has
>> submitted
>> a material for a review, please have a look:
>> https://drupal.star.bnl.gov/STAR/node/61809
>>
>> Deadline: 2022-12-05
>> ---
>> If you have any problems with the review process, please contact
>> webmaster AT www.star.bnl.gov
>> _______________________________________________
>> Star-hp-l mailing list
>> Star-hp-l AT lists.bnl.gov
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--

Sooraj Radhakrishnan

Research Scientist,

Department of Physics

Kent State University

Kent, OH 44243

Physicist Postdoctoral Affiliate

Nuclear Science Division
Lawrence Berkeley National Lab
MS70R0319, One Cyclotron Road

Berkeley, CA 94720

Ph: 510-495-2473

Email: skradhakrishnan AT lbl.gov

--

Sooraj Radhakrishnan

Research Scientist,

Department of Physics

Kent State University

Kent, OH 44243

Physicist Postdoctoral Affiliate

Nuclear Science Division
Lawrence Berkeley National Lab
MS70R0319, One Cyclotron Road

Berkeley, CA 94720

Ph: 510-495-2473

Email: skradhakrishnan AT lbl.gov

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