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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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Subject: STAR HardProbes PWG

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  • From: Nihar Sahoo <nihar AT rcf.rhic.bnl.gov>
  • To: 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
  • Date: Wed, 07 Jun 2023 18:31:32 +0530

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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