STAR HardProbes PWG

[Sooraj Radhakrishnan <skradhakrishnan AT lbl.gov>]

Hi Barbara,

   Thanks for the update. I dont have further comments and sign off

Sooraj

On Wed, Jun 22, 2022 at 9:39 AM Yi Yang via Star-hp-l <star-hp-l AT lists.bnl.gov> wrote:

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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--

Sooraj Radhakrishnan

Research Scientist,

Department of Physics

Kent State University

Kent, OH 44243

Physicist Postdoctoral Affiliate

Nuclear Science Division
Lawrence Berkeley National Lab
MS70R0319, One Cyclotron Road

Berkeley, CA 94720

Ph: 510-495-2473

Email: skradhakrishnan AT lbl.gov