STAR HardProbes PWG

[Nihar Sahoo <nihar AT rcf.rhic.bnl.gov>]

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
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>  --
>
> Andrew Tamis
> Yale University
> Graduate School of Arts and Sciences
> Department of Physicsandrew.tamis AT yale.edu