STAR HardProbes PWG

[Barbara Trzeciak <barbara.trzeciak AT gmail.com>]

Hi Neil,

I would just add on s13:  suppression for D0-tagged jets ->  suppression for D0-tagged jets at low pT,jet 

Otherwise the presentation looks good to me and I sign off.

Cheers,

Barbara

On Fri, Oct 21, 2022 at 10:03 PM Diptanil Roy via Star-hp-l <star-hp-l AT lists.bnl.gov> wrote:

Hi everyone, thank you for your comments. I have uploaded a new version here (https://drupal.star.bnl.gov/STAR/system/files/DNP_DiptanilRoy_v2.pdf), where all the comments have been addressed.

Please find some comments inline.

Barbara's comments:

I wouldn't say they are so similar (rather the trend is), we should also keep in mind R_AA vs R_CP, different R and D jet pT requirements.

I agree. I made it a point to mention it during my Hot Quarks talk but I changed the punchline as well. Please let me know if the new version looks better.

Yi's comments:

I would think the STAR detector slide from your Hot Quark (p7) should be added back

I have added it for now. It might push the time right to the edge of 10 minutes, but I can work with it.

Sooraj's commens:

Given the error bars, the conclusion that no significant diffusion for D0 seen from STAR measurement is not fair.

I agree, given that our measurements can be overlaid with the CCNU model as well. I just wanted parity between the statements for CMS and STAR. I have changed it a little now. Please let me know if the new version looks better.

Thank you so much.

On Fri, Oct 21, 2022 at 6:18 AM Nihar Sahoo via Star-hp-l <star-hp-l AT lists.bnl.gov> wrote:

Hello Diptanil,

I agree with Barbara and Sooraj's comment on your slides.
Please address their comments.
I have a minor comment on your slide14

"Slight diffusion observed for D0 mesons..."
-> "Hint of diffusion observed for D0 bensons..."

With that I sign off.

Cheers
Nihar

On 2022-10-21 15:36, Sooraj Radhakrishnan via Star-hp-l wrote:
> Hi Diptanil,
>    As this is very similar to your slides for Hot Quarks, I dont have
> many comments. I sign off with one comment on S14. Given the error
> bars, the conclusion that no significant diffusion for D0 seen from
> STAR measurement is not fair. Why not have the same bullet as from the
> conclusion slide?
>
> thanks
> Sooraj
>
> On Thu, Oct 20, 2022 at 11:35 PM Yi Yang via Star-hp-l
> <star-hp-l AT lists.bnl.gov> wrote:
>
>> Hi Diptanil,
>>
>> Thanks a lot for the nice slides. Since it is similar to your Hot
>> Quarks presentation, I don't have any further comments/suggestions,
>> except I would think the STAR detector slide from your Hot Quark
>> (p7) should be added back. But it really depends on whether you can
>> finish your talk in time.
>>
>> Cheers,
>> Yi
>>
>> On Thu, Oct 20, 2022 at 1:10 AM Diptanil Roy via Star-hp-l
>> <star-hp-l AT lists.bnl.gov> wrote:
>>
>> Hi everyone, please find my contribution below for DNP 2022. It's
>> similar to the Hot Quarks approved talk, but certain slides have
>> been shortened to fit the talk in 10 minutes. Please let me know if
>> you have any comments/questions on the slides.
>>
>> Thank you.
>>
>> On Wed, Oct 19, 2022 at 1:03 PM webmaster--- via Star-hp-l
>> <star-hp-l AT lists.bnl.gov> wrote:
>> Dear Star-hp-l AT lists.bnl.gov members,
>>
>> Diptanil Roy (roydiptanil AT gmail.com) has submitted a material for a
>> review,
>> please have a look:
>> https://drupal.star.bnl.gov/STAR/node/61409
>>
>> Deadline: 2022-10-27
>> ---
>> If you have any problems with the review process, please contact
>> webmaster AT www.star.bnl.gov
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>> --
>>
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> --
>
> Sooraj Radhakrishnan
>
> Research Scientist,
> Department of Physics
>
> Kent State University
>  Kent, OH 44243
>
> Physicist Postdoctoral AffiliateNuclear Science Division
> Lawrence Berkeley National Lab
> MS70R0319, One Cyclotron Road
> Berkeley, CA 94720
> Ph: 510-495-2473 [1]
>
> Email: skradhakrishnan AT lbl.gov
>
>
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