STAR HardProbes PWG

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

Hi Diptanil,

nice abstract.

I have a comment on your physics part: 

L5-6: ...  is suppressed for heavy quarks, such as charm and bottom, at low transverse momenta (pT) - this is not clear to me. Do you mean the dead-cone effect ? Please note that for HF at low pT (here it might be also ambiguous what one calls the low pT) the collisional energy loss is expected to be (even more) important. There is also expected mass ordering in the case of the collisional energy loss, but one shouldn't mix the two effects. And studies of the radial profile, especially at low pT < 5 GeV as we hope to get, can shed more light also on the D meson diffusion (L16).

Cheers,

Barbara

On Sun, Jun 26, 2022 at 6:56 AM Nihar Sahoo via Star-hp-l <star-hp-l AT lists.bnl.gov> wrote:

Hello Diptanil,

Thank you for implementing my suggestions and modifying your abstract
based on our current D^0+jet preliminary results.
Please find additional comments below and with implementing these I sign
off.

Line1: "Partons i.e. quarks and gluons " -> "Parton, i.e, quark and
gluons, …"
Line13:"…radial profile in anti-kT jets from Au+Au collisions …" ->
"…radial profile in jets reconstructed using anti-kT in Au+Au
collisions…"
"…200 GeV at RHIC, collected …" -> "…200 GeV collected…"

Cheers
Nihar


On 2022-06-25 22:43, Diptanil Roy wrote:
> Hi Nihar, thank you for your comments, I have implemented most of them
> in the new version uploaded here.
> https://drupal.star.bnl.gov/STAR/system/files/APS2022_DiptanilRoy_v2.pdf
>
> Please let me know if you have any more comments.
>
> Thank you.
>
> On Sat, Jun 25, 2022 at 12:29 PM Nihar Sahoo <nihar AT rcf.rhic.bnl.gov>
> wrote:
>
>> Hello Diptanil,
>>
>> I would suggest to submit your abstract based on QM2022 preliminary
>> results at DNP without promising a lot. I find your current
>> preliminary
>> results are important and interesting to draw attention of the
>> audience.
>>
>> Besides, please find my comments on your nice abstract.
>>
>> "Mentor: Dr. Sevil Salur" -> you can drop it, not required;
>> line#1 "Partons (quarks/gluons)… " -> "         Partons, i.e.,
>> quarks or
>> gluons, ….
>> Line#5"…quarks (such as charm and bottom) at low …" ->
>> "…quarks, such as
>> charm and bottom, at low …"
>> Line#10 "…mesons at low with high significance, …" -> "…mesons
>> at low
>> $p_{\rm T} with high significance of signal over the background."
>> You could drop "making STAR ideal for similar measurements."; this
>> is
>> not required.
>>
>> On second pare:
>> I would suggest to concentrate only on QM2022 results without
>> promising
>> too much. As we have not seen D^0 lower pT results so far which may
>> need
>> a detailed discussion. So please modify this para based on your
>> QM2022
>> results (D^0 pT > 5 GeV) with existing STAR preliminary.
>>
>> R_CP -> $R_{\rm CP}$  (here "CP" is a label and no value, so is
>> roman)
>>
>> Cheers
>> Nihar
>>
>> On 2022-06-24 01:20, Diptanil Roy via Star-hp-l wrote:
>>> Hi everyone, please find my contribution for DNP 2022 in the link
>>> above. The abstract is more or less similar to the approved one
>> for
>>> Quark Matter 2022, with some changes to reflect the already
>> presented
>>> results. Thank you.
>>>
>>> On Thu, Jun 23, 2022 at 3:48 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/60035
>>>>
>>>> ---
>>>> 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
>>>> https://lists.bnl.gov/mailman/listinfo/star-hp-l
>>>
>>> --
>>>
>>> ~ Neil
>>> _______________________________________________
>>> Star-hp-l mailing list
>>> Star-hp-l AT lists.bnl.gov
>>> https://lists.bnl.gov/mailman/listinfo/star-hp-l
>
> --
>
> ~ Neil
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