STAR HardProbes PWG

["Roy Chowdhury Priyanka (DOKT)" <priyanka.roy_chowdhury.dokt AT pw.edu.pl>]

Hi Qian,

Firstly, apologize for the delay in getting back to you and thanks for providing your thoughtful comments. Please find my updated version here.

https://drupal.star.bnl.gov/STAR/system/files/WPCF24_Priyanka_V1.pdf

Here are the answers of your questions.

1. P4: Yes, the production mechanism means D0 hadronization process
2. P7: The ref. plots calculated for p+p system. In final state, strong interaction doesn't depend on the charge, so we can expect similar outcome (very small scattering length) from D0-charged hadron correlation in Au+Au system
3. P12: As I didn't use the whole dataset from Run 14, I was asked to mention the no. of events in previous times. We think, information in first 3 lines are needed.
4. P14: This question is not very clear to me. If you are referring about the spin states of D0 and hadron, we considered both with same spin states.
5. P15: Here, I mention about D_S0^* (2317) state as it is a bound state of DK channels and in theory prediction, we can see its presence. So, to clarify the fact that in our Data, why we can't see such resonance state, I introduced this point
6. P19: I would like to keep it as "and" instead of "or" because it was suggested to keep the conclusion like this previously. Also, our conclusion holds both points mentioned in bullet no. 2.
   
   
   Please let me know if you have further questions and comments.
   
   

Regards,

Priyanka

---

From: star-hp-l-request AT lists.bnl.gov <star-hp-l-request AT lists.bnl.gov> on behalf of tc88qy <tc88qy AT rcf.rhic.bnl.gov>
Sent: Sunday, October 27, 2024 2:08 PM
To: star-hp-l AT lists.bnl.gov <star-hp-l AT lists.bnl.gov>
Subject: Re: [[Star-hp-l] ] STAR presentation by Priyanka Roy Chowdhury for WPCF 2024 submitted for review

 

Hello Priyanka,

  Please find my comments to your nice slides below :
Page 3, Heavy flavored … in collisions due to their large mass.
Page 4, what is the production mechanism you mentioned here? If I
understand correctly, do you mean the D0 hadronization process ?
Page 6, a reference should for this page.
Page 7, Title: D-hadron femtoscopy in p+p at LHC
             Small values of apiD (scattering length )…, It is in p+p not
heavy-ion collision right ?
             Possibility to …  source size or length of homogeneity in
A+A system.
Page 12: you do not need all dateset information, please remove it
Page 13: remove Good S/B ratio for D0 signal pT>1 GeV/c
Page 14: How did you deal with the pair spin?
Page 15: The mention of D_S0^* (2317) here feels quite abrupt, Is there
any particular reason to bring  up D_S0^* (2317)?
Page 19: the second bullet:  … or large emission source size (~ 5 fm).

Qian Yang

On 2024-10-25 21:51, "Roy Chowdhury Priyanka (DOKT)" wrote:
> Dear Convenors,
>
>  Here's my submission for upcoming WPCF. Talk duration is 25 mins.
>  I have kept one slide with placeholders where I intend to add the
> plots from model fitting. I would like to give an update of these fit
> results at the next week's PWG meeting. Please add me as a speaker in
> advance.
>
>  Regards,
>  Priyanka
>
> -------------------------
>
> From: star-hp-l-request AT lists.bnl.gov
> <star-hp-l-request AT lists.bnl.gov> on behalf of webmaster AT star.bnl.gov
> <webmaster AT star.bnl.gov>
> Sent: Friday, October 25, 2024 3:46 PM
> To: Star-hp-l AT lists.bnl.gov <Star-hp-l AT lists.bnl.gov>
> Subject: [[Star-hp-l] ] STAR presentation by Priyanka Roy Chowdhury
> for WPCF 2024 submitted for review
>
> 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/69682
>
> Deadline: 2024-11-04
> ---
> If you have any problems with the review process, please contact
> webmaster AT www.star.bnl.gov