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star-hp-l - Re: [Star-hp-l] STAR presentation by Priyanka Roy Chowdhury for IS 2023 submitted for review

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  • From: Nihar Sahoo <nihar AT rcf.rhic.bnl.gov>
  • To: "Roy Chowdhury Priyanka (DOKT)" <priyanka.roy_chowdhury.dokt AT pw.edu.pl>
  • Cc: STAR HardProbes PWG <star-hp-l AT lists.bnl.gov>
  • Subject: Re: [Star-hp-l] STAR presentation by Priyanka Roy Chowdhury for IS 2023 submitted for review
  • Date: Mon, 12 Jun 2023 11:19:36 +0530

Hello Priyanka,

Thank you for implementing my comments.

One additional comment on Summary
How should the correlation functions look like in heavy-ion collisions? -> What is the effect of hot-dense QCD medium on D^0-hadron femtoscopic correlations?
Or "What is the D^0-hadron femtoscopic correlations due to the presence of hot-dense QCD medium?"
Or something similar.

With this implementation, I sign off.

Looking forward to seeing your updates on this analysis for QM2023 in coming days.


Cheers
Nihar


On 2023-06-10 22:43, Roy Chowdhury Priyanka (DOKT) wrote:
Hi Nihar,

Thanks for your thoughtful comments. Sorry for the delay. Please
check the updated version with the implementation of all your
feedback.
https://drupal.star.bnl.gov/STAR/system/files/IS2023_poster_V2_Priyanka.pdf
[1]

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: Wednesday, June 7, 2023 3:01 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 IS 2023 submitted for review

Hello Priyanka,

Please find my comments on your nice abstract below.

I. Motivation:

"Charm-hadron __correlation__can " -> can you make some adjustment to
avoid the extra gaps?
Please indicate if these plots are for QGP medium or vacuum.
Introduce QGP here, a short sentence. [or in the abstract mention "the

Quark Gluons Plasma (QGP)."]

II. Methodology
distribution respectively for correlated -> distribution,
respectively,
for correlated
Event mixing technique to calculate k* for uncorrelated pairs -> Event

mixing technique to calculate uncorrelated pairs k* …

III. D-hadron femtoscopy

Data suggest .. -> ALICE preliminary data suggest … or ALICE data
suggest
FIg.4 -> Please include "ALICE preliminary" on this plot indicating
this
is from ALICE preliminary.
strong interaction of c/c with -> Not clear what is "c/c"?

IV. D0 reconstruction at STAR
Figure - 7: D0 decay channel -> Figure - 7: D0 decay topology

V. Analysis & Outcomes
Detector effects corrections: -> TPC detector effects correction:
max. possible no. -> maximum possible number
Fig.10 left -> T_1,2 -> Track_1,2

VI. Summary

How should the correlation functions look like in heavy-ion
collisions?
->

For heavy-ion collisions, QGP and hadronic phase effects on
two-particle
correlations are 
unknown
-> In heavy-ion collisions, the contribution of QGP and hadronic
phase
to D meson+hadron correlation functions is not well understood. (or
well
studied)

First experimental analysis -> First measurement

Model study (ex. Lednický–Lyuboshitz) is on the plan to extract
interaction parameters, like emission source size -> Plan to extract
interaction parameter, like emission source size, using
Lednický–Lyuboshitz model.

input on interactions -> input to the interaction …

Model calculations needed that include -> Theoretical inputs are
needed
that include

Cheers
Nihar

On 2023-06-06 17:59, 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/63885

Deadline: 2023-06-19
---
If you have any problems with the review process, please contact
webmaster AT www.star.bnl.gov
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Links:
------
[1] https://drupal.star.bnl.gov/STAR/system/files/IS2023_poster_V2_Priyanka.pdf




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