STAR HardProbes PWG

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

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
> > > > > _______________________________________________
> > > > > Star-hp-l mailing list
> > > > > Star-hp-l AT lists.bnl.gov
> > > > > https://lists.bnl.gov/mailman/listinfo/star-hp-l
> > > _______________________________________________
> > > Star-hp-l mailing list
> > > Star-hp-l AT lists.bnl.gov
> > > https://lists.bnl.gov/mailman/listinfo/star-hp-l
> >
> > --
> >
> > 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