STAR HardProbes PWG

[Yi Yang <yiyang0429 AT gmail.com>]

Hi Barbara,

Thanks a lot for the nice abstract. 

I don't have any comments or suggestions.

Cheers,

Yi

On Tue, Jun 21, 2022 at 6:03 PM Nihar Sahoo via Star-hp-l <star-hp-l AT lists.bnl.gov> wrote:

Hello Barbara,

Thank you for implementing my comments. I sign off your nice abstract.

Regards
Nihar

On 2022-06-21 14:43, Barbara Trzeciak wrote:
> Hi Nihar, Sooraj,
> thanks for additional comments.
> I've updated the abstract.
>
> Cheers,
> Barbara
>
> On Mon, Jun 20, 2022 at 5:03 PM Sooraj Radhakrishnan
> <skradhakrishnan AT lbl.gov> wrote:
>
>> Hi Barbara,
>> Thanks for preparing this nice abstract. Please find some
>> comments from me below.
>>
>> L4: I think at this point we can state, 'Ultra relativistic
>> heavy-ion collisions create a dense and ...'
>> L8: A suggestion, may be the open heavy flavor part on L13 goes
>> better immediately after 'probing the whole medium evolution'.
>> Quarkonia probing the color screening and thermodynamic properties
>> could come after as a separate point.
>> L10: effect --> mechanism, which causes the quarkonia bound states
>> to dissociate in the QGP,
>> L19: J/Psi production --> J/Psi suppression?
>>
>> L21: results on --> measurements of?
>>
>> L23: the part staring 'that conclude ...' can be removed
>> L27: D0 tagged jets and their radial profiles
>> L29: by STAR will be discussed
>>
>> thanks
>> Sooraj
>>
>> On Mon, Jun 20, 2022 at 9:47 AM Nihar Sahoo via Star-hp-l
>> <star-hp-l AT lists.bnl.gov> wrote:
>>
>>> Hello Barbara,
>>>
>>> Thank you for implementing my last comments.
>>> Please find my additional comments below.
>>>
>>> LIne#4: "In ultra-relativistic heavy-ion collisions creation a
>>> dense and
>>> hot medium  … is expected." -> "In ultra-relativistic heavy-ion
>>> collisions, a dense and hot medium… is created."
>>>
>>> Line#5: "…a dense and hot medium with partonic degrees of
>>> freedom,
>>> called the Quark-Gluon Plasma (QGP),…" -> "…a dense and hot
>>> Quantum
>>> Chromodynamics medium with the color degrees of freedom, called
>>> the
>>> Quark-Gluon Plasma (QGP), …" (Here "dense and hot medium" is the
>>> QCD
>>> medium; you mean "color degrees of freedom" here).
>>>
>>> Line#12: "…not only…, but help…,respectively." -> The syntax
>>> of this
>>> sentence needs a bit of improvement. Suggestion: use "and" with
>>> ",respectively." in this sentence. Otherwise, use "not
>>> only…but…"
>>> without "respectively" here.
>>>
>>> Regards,
>>> Nihar
>>>
>>> On 2022-06-20 02:11, Barbara Trzeciak wrote:
>>>> Hi Nihar,
>>>>
>>>> thank you for your useful comments.
>>>> I've updated the abstract.
>>>> And sorry for multiple posts, the current version is under:
>>>>
>>>
>>
> https://drupal.star.bnl.gov/STAR/presentations/ICNFP-2022/Recent-heavy-flavor-results-STAR
>>>>
>>>> Cheers,
>>>> Barbara
>>>>
>>>> On Sun, Jun 19, 2022 at 4:59 PM Nihar Sahoo via Star-hp-l
>>>> <star-hp-l AT lists.bnl.gov> wrote:
>>>>
>>>>> Hello Barbara,
>>>>>
>>>>> Please find my comments on your nice abstract on HF
>>> measurements.
>>>>>
>>>>> 1_ "…the early stage of heavy-ion ultra-relativistic
>>> heavy-ion
>>>>> collisions…" -> "the early stage of ultra-relativistic
>>> heavy-ion
>>>>> collisions…"
>>>>> (Here "ultra" is optional you may consider to drop it)
>>>>> 2_ "..the whole medium evolution" -> AT this point you have not
>>>>> introduced yet what is this medium (that is QGP). Hence you may
>>> need
>>>>> to
>>>>> introduce the QGP medium before.
>>>>> 3_ "Therefore, …the properties of the Quark-Gluon Plasma
>>> (QGP)
>>>>> produced
>>>>> in these collisions. Please try to introduce QGP before and
>>> then 2_
>>>>> should come next.
>>>>> 4_ "Quarkonium studies in p + p and p+Au collisions provide us
>>> not
>>>>> only
>>>>> with the necessary baseline for Au+Au collisions, but help to
>>>>> understand
>>>>> the quarkonium production mechanisms and the cold nuclear
>>> matter
>>>>> effects, respectively.
>>>>> " -> "On the other hand, the quarkonium measurements in p + p
>>> and
>>>>> p+Au
>>>>> collisions not only help to understand their production
>>> mechanisms
>>>>> and
>>>>> the cold nuclear matter effects but also set the necessary
>>> baseline
>>>>> for
>>>>> Au+Au collisions.
>>>>> 5_ "…production provide us information on transport
>>> properties…"
>>>>> ->
>>>>> "…production provide information on the transport
>>> properties…"
>>>>> 6_"… degree of the heavy quark thermalization and the
>>>>> hadronization
>>>>> mechanism." -> "the degree of the heavy quark thermalization,
>>> and
>>>>> the
>>>>> hadronization mechanism."
>>>>> 7_ "We will show measurements of the J/ψ suppression and
>>> elliptic
>>>>> flow
>>>>> in isobar (Ru+Ru and Zr+Zr) collisions at √sNN = 200 GeV and
>>>>> studies of
>>>>> system size and energy dependence of the J/ψ production." -> I
>>>>> would
>>>>> prefer  to rephrase the sentence something like "The system
>>> size and
>>>>>
>>>>> energy dependence of the J/ψ production, and its suppression
>>> and
>>>>> elliptic flow in isobar (Ru+Ru and Zr+Zr) collisions at √sNN
>>> = 200
>>>>> GeV
>>>>> will be discussed."
>>>>> (Just to avoid "we will" again)
>>>>> 8_ "…D_S and Λ_C…" -> " …D_S, and Λ_C…"
>>>>> 9_ cross section -> cross-section
>>>>> 10_ "…will be also reported." -> "…will also be reported."
>>>>> 11_"We will also present the first measurements of…" -> "The
>>> first
>>>>>
>>>>> measurements of…200 GeV will be presented."
>>>>> 12_ At the end you may consider to include STAR's plan for
>>>>> heavy-flavor
>>>>> measurement in upcoming (Run23-25) data taking. something like
>>>>> "Finally, I plan to shed light on the future data-taking plan
>>> for
>>>>> precision and their kinematic coverage of heavy flavor
>>> measurements
>>>>> in
>>>>> the STAR experiment."
>>>>>
>>>>> Regards,
>>>>> Nihar
>>>>>
>>>>> On 2022-06-19 13:09, webmaster--- via Star-hp-l wrote:
>>>>>> Dear Star-hp-l AT lists.bnl.gov members,
>>>>>>
>>>>>> Barbara Trzeciak (barbara.trzeciak AT gmail.com) has submitted a
>>>>> material
>>>>>> for a
>>>>>> review, please have a look:
>>>>>> https://drupal.star.bnl.gov/STAR/node/59970
>>>>>>
>>>>>> ---
>>>>>> 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
>>>>> _______________________________________________
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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
>
>
> Links:
> ------
> [1] tel:%28510%29%20495-2473
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