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

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Subject: STAR HardProbes PWG

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  • From: Nihar Sahoo <nihar AT rcf.rhic.bnl.gov>
  • 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 Hard Probes 2023 submitted for review
  • Date: Wed, 30 Nov 2022 12:35:39 +0530

Hi Andrew,

Thank you for addressing my additional comment. I sign off.

Cheers
Nihar

On 2022-11-30 16:06, Andrew Tamis via Star-hp-l wrote:
Hi Sooraj,

Thank you for the comments.
L22: Done
L23: I removed the kinematic range
L25: Removed ", a monte carlo event generator"
L27: I removed the kinematic range, and rephrased the last sentence to
"..., which will provide information about how the quark-gluon plasma
interacts with the jet differently across the angular scales covered
by the EEC." Please let me know if this sounds better.

Best,
Andrew

On Tue, Nov 29, 2022 at 8:26 PM Sooraj Radhakrishnan
<skradhakrishnan AT lbl.gov> wrote:

Hi Andrew,
Thanks for preparing this nice abstract. Please find a few
comments from me below

L22: in p+p collisions --> p+p collisions
L23: GeV/c (not as a fraction). Do you want to specify the kinematic
range in the abstract?
L25: I dont think you need to define PYTHIA6 for HP abstract
L27: scale dependence of the QGP doesnt read right, what do you
refer to here? Modification from QGP at different length/angular
scales? Should rephrase if so

thanks
Sooraj

On Tue, Nov 29, 2022 at 12:00 AM Nihar Sahoo via Star-hp-l
<star-hp-l AT lists.bnl.gov> wrote:

Hello Andrew,

Thank you for implementing my comments.
I have a few additional comments below.

L6: "Other time information" Not clear what is other time besides
"split
formation time" ?
L23: "The response of the EEC to selections on jet pT …. 15
GeV/c to 50
GeV/c" ->" The EEC of full jet pT will be shown in a kinematic
range
from 15 to 50 GeV/$\it c$ using the STAR barrel calorimeter
detectors
and time projection chamber. "
L25: "… PYTHIA 6, a Monte Carlo event generator." -> "…
PYTHIA-6." (If
it is STAR tune, then mention it please)

Cheers
Nihar

On 2022-11-29 01:14, Andrew Tamis wrote:
Hello Barbara and Nihar

Thank you for the comments! I have implemented both of your
suggestions. I included split formation time as an example of
time
information that soft drop and the lund plane extract. I have
also
listed PYTHIA 6 as the monte carlo generator I am using for
comparisons.

Please let me know if you have any more comments

Best,
Andrew

On Sun, Nov 27, 2022 at 6:07 AM Nihar Sahoo via Star-hp-l
<star-hp-l AT lists.bnl.gov> wrote:

Hello Andrew,

Please find my comment on your nice abstract.

L6: "extract time information " -> please mention what time
information.
Do you mean "formation time of parton shower" ?
L12:"… jet evolution .." -> the jet evolution
L14: "infrared and collinear " -> "infrared-and-collinear "
L21: "data from" -> "the data from"; "in p+p collisions"
L22: for the detector effect;
"a Monte Carlo event generator " -> better to mention what are
those
generators or models?

Please give some information how do you select jet in pp and
what
kinematic range you plan to present.

Cheers
Nihar

On 2022-11-21 10:58, 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/61793

Deadline: 2022-12-05
---
If you have any problems with the review process, please
contact
webmaster AT www.star.bnl.gov
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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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