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star-hp-l - Re: [Star-hp-l] STAR presentation by Andrew Tamis for Quark Matter 2023 submitted for review

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Subject: STAR HardProbes PWG

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  • From: Barbara Trzeciak <barbara.trzeciak AT gmail.com>
  • To: Andrew Tamis <andrew.tamis AT yale.edu>, STAR HardProbes PWG <star-hp-l AT lists.bnl.gov>
  • Subject: Re: [Star-hp-l] STAR presentation by Andrew Tamis for Quark Matter 2023 submitted for review
  • Date: Fri, 21 Apr 2023 23:24:13 +0200

Hi Andrew,

I sign off your abstract.

Cheers,
Barbara

On Fri, Apr 21, 2023 at 4:13 PM Andrew Tamis via Star-hp-l <star-hp-l AT lists.bnl.gov> wrote:
Hello Nihar,

I have uploaded the new version

thank you,
Andrew

On Fri, Apr 21, 2023 at 7:45 AM Nihar Sahoo <nihar AT rcf.rhic.bnl.gov> wrote:
Hello Andrew,

Thank you for addressing my comments.
Please make sure to implement these two comments.
>>> _ Title: 200GeV -> 200 GeV
>>> _infrared- and collinear-safe, -> infrared-collinear safe,

with these implemented, I sign off.

Cheers
Nihar

On 2023-04-20 21:14, Andrew Tamis wrote:
> Hello Nihar and Barbara,
>
> Thank you very much for the comments! I have updated the abstract
>
> Best,
> Andrew
>
> On Thu, Apr 20, 2023 at 7:14 AM Barbara Trzeciak via Star-hp-l
> <star-hp-l AT lists.bnl.gov> wrote:
>
>> Hi Andrew,
>>
>> nice abstract. Please find below my minor comments.
>>
>> energy-energy Correlator (EEC) -> Energy-Energy Correlator (EEC)
>>
>> using the data taken from √s = 200 GeV pp collisions measured by
>> the STAR experiment -> using pp collision data at √s = 200 GeV
>> collected by the STAR experiment
>> The EEC will be shown differentially -> The EEC is shown
>> differentially
>>
>> a next-to-leading-logarithmic calculation ->
>> next-to-leading-logarithmic pQCD calculations
>>
>> Cheers,
>> Barbara
>>
>> On Thu, Apr 20, 2023 at 7:57 AM Nihar Sahoo via Star-hp-l
>> <star-hp-l AT lists.bnl.gov> wrote:
>>
>>> Hello Andrew,
>>>
>>> Please find my comments on your nice abstract.
>>>
>>> _ Title: 200GeV -> 200 GeV
>>> _ hadronization, resulting -> hadronization resulting
>>> _ One observable that utilizes the substructure of these jets to
>>> study
>>> the information encoded within, describing the time evolution of
>>> the
>>> parton shower is the energy-energy Correlator (EEC).
>>> -> "The energy-energy correlator (EEC) observable utilizes the
>>> substructure of jets to study the time evolution of the parton
>>> shower."
>>> _ non-perturbative and perturbative effects -> the  perturbative
>>> and
>>> non-perturbative QCD effects
>>> _ rejection of constituents. -> rejection of soft constituents.
>>> _ these two distinct regimes: -> the two distinct regimes:
>>> _ effects originating from free hadrons at small opening angles
>>> and from
>>> perturbative fragmentation of quarks and gluons at large opening
>>> angles.
>>> -> i) from the free hadrons phase at small opening angles, and ii)
>>> from
>>> the perturbative fragmentation of quarks and gluons at large
>>> opening
>>> angles.
>>> _presented, using the data -> presented using the data
>>> _infrared- and collinear-safe, -> infrared-collinear safe,
>>> _systems, which -> systems which
>>>
>>> Cheers
>>> Nihar
>>>
>>> On 2023-04-18 05:38, webmaster--- via Star-hp-l wrote:
>>>> Dear Star-hp-l AT lists.bnl.gov members,
>>>>
>>>> Andrew Tamis (andrew.tamis AT yale.edu) has submitted a material
>>> for a
>>>> review,
>>>> please have a look:
>>>> https://drupal.star.bnl.gov/STAR/node/63424
>>>>
>>>> Deadline: 2023-09-03
>>>> ---
>>>> If you have any problems with the review process, please contact
>>>> webmaster AT www.star.bnl.gov
>>>> _______________________________________________
>>>> Star-hp-l mailing list
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>>>> https://lists.bnl.gov/mailman/listinfo/star-hp-l
>>> _______________________________________________
>>> Star-hp-l mailing list
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>> _______________________________________________
>> Star-hp-l mailing list
>> Star-hp-l AT lists.bnl.gov
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>  --
>
> Andrew Tamis
> Yale University
> Graduate School of Arts and Sciences
> Department of Physicsandrew.tamis AT yale.edu
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