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Re: [Star-hp-l] STAR presentation by Tristan Protzman for Hard Probes 2023 submitted for review
- From: Nihar Sahoo <nihar AT rcf.rhic.bnl.gov>
- To: Tristan Protzman <tlp220 AT lehigh.edu>
- Cc: STAR HardProbes PWG <star-hp-l AT lists.bnl.gov>
- Subject: Re: [Star-hp-l] STAR presentation by Tristan Protzman for Hard Probes 2023 submitted for review
- Date: Tue, 21 Mar 2023 22:26:30 +0530
Hello Tristan,
Thank you for addressing my comments.
Can you please point to your Drupal page putting all preliminary plots and preliminary request slides?
Cheers
Nihar
On 2023-03-21 21:34, Tristan Protzman wrote:
Hi Nihar, Barbara,
Thank you for your careful review and comments. I have also received
feedback from the Lehigh group after my practice talk yesterday
afternoon which has been addressed. A new draft has been uploaded,
find my comments below.
Cheers,
Tristan
Nihar's Comments
Slide-2:
1. "The contribution of each process to jet quenching is unknown "->
But
we do know in QGP radiative process dominates over collisional
process.
So this sentence probably needs to rephrase unless you want to say
somethingelse.
_Changed to suggest that measuring v2 can help distinguish between
competing models of jet energy loss_
2. Can you give reference for collisional E_loss's L dependence?
3. For radiative case L^2 dependence comes from BDMPS. So you need to
give reference.
_Both references added_
SLide-3
1. In this plot, increase the X-axis title and label size (also for
Y-axis). Not visible.
_Changed_
2. "Central events show significant hadron suppression at high
momentum"
-> " 0-10% central events show significant hadron suppression at
high
momentum"
_I would like to leave this as central, since all centralities show
suppression and I would like to draw _
3. You need to mention what are <Ncoll> and sigma_inel^NN and their
values used for this result?
_This plot was shown at QM22 by Tong without those values, I will work
with Tong to find what was used and have them ready in backup at a
minimum_
SLide-4
1. "Semi-central collisions produce an approximately elliptical QGP"
->
"Semi-central collision produces a elliptical geometry of the QGP
medium"
_I would like to leave approximately, since it is important to
remember that the higher order fluctuations drive it away from
elliptical_
2. "To use familiar language, we will report this as 𝑣2, despite
jet
quenching being being distinct mechanism from flow" Not sure what you
want to say here.
_Changed to "_Though the language is the same, high 𝑝_T 𝑣_2 is
driven by different effects than low 𝑝_T flow"
3. I think you need to introduce what is v2 as 2nd order anisotropy in
this slide?
_Added._
Slide-6
1. X-axis title: pT^reco -> "pT^trak;
_Changed_
2. X-axis: increase title and label size; put unit
_Changed_
3. Y-axis: increase title and label size
_Changed_
4. You need to mention before or in this slide what is pT?
_Changed first occurrence _
5. "No strong momentum dependence observed " -> "No transverse
momentum
dependence of v_{2} observed at high-p_{T}"
_Changed_
Slide-7
1. "Measuring high 𝑝T charged hadron 𝑣2 gives us a connection to
flow
measurements " Not sure what you want to say? Why only "high-pT
charged
hadron v2 gives connection to flow"? Please rephrase
_Added explicate reference to low pT flow, drawing the connection that
there is going to be a transition from the flow dominated v2 to
quenching dominated flow_
2. "…with resolutions …" -> "…with resolution (R)…" here you
can
introduce jet R.
_Added_
3. Give STAR paper's reference to this upper v2 plot.
_I don't believe this result has been published yet_
Slide-9:
1. "2 GeV" -> "2 GeV/c"
_Added_
2. "The event is clustered into jets with the anti-𝑘T algorithm" ->
You
have mentioned already in the above sentence. Drop this bullet.
_I am making it clear that the event is clustered twice_
3. "Δ𝑅 < R_resolution " you need to find a better way to write
this.
What is R_resolution?
_Clarified with formula for \Delta R_
4. First subbullet of last bullet expression: you need to mention what
are pT^measured, rho(phi), A, etc?
_Added_
SLide-10:
1. Title: "Combinatorial Jet Quenching" sounds awkward. Please
rephrase
this. Something like "Combinatorial jet contribution"
2. Put this slide in backup. If somebody asks then show. Otherwise
you
don't need to speak on this test.
_Changed and moved to backup_
SLide-11,12,13:
1. Please follow the same suggestion on this fig from Slide-6
_Changed_
2. "Small, non-zero R=0.2 anti-𝑘T jet 𝑣2 in isobar
collisions at STAR "
-> "Non-zero jet v_{2} is observed for R=0.2 in isobar collisions"
(same
for SLide12)
_Changed_
3. "Like charged particle …" -> "Like inclusive charged
particle…"
_Changed_
4. "No obvious R dependence!" -> "No jet R dependence of v_{2}
is
observed" (Not sure why it is "Obvious"?)
_I would like to keep this as there is no obvious effect looking at
the plot, and on the next slide we quantify this_
Slide-14:
1. Please follow the same suggestion on this fig from Slide-6
_Done_
2. "To remove correlations by comparing the same partons, the
numerator
and denominator are separate sets of events"
Can you please rephrase this sentence to make it more clear?
_Removed, and I will spend time explaining this clearly in the talk _
Barbara's Comments
- s2: add references related to the coll. and radiative processes
_Added_
- s3: the last bullet - please follow the status of Isaac's poster
_Will do!_
- s4: define v2. I would rephrase the last bullet. The mechanisms
causing v2 are different at low and high pT, but it's still v2
observable. Maybe something along the line: "non-zero v2 at high pT
due to jet quenching"
_Rephrased to "_Though the language is the same, high 𝑝_T 𝑣_2 is
driven by different effects than low 𝑝_T flow"
- s5: change title of the slide, e.g. Event Plane Reconstruction
_Done_
- s5: before run 18 -> before 2018
_Changed_
- s5: since you don't show STAR or don't have more details on the used
detector for the jet reconstruction, I suggest to add at least
information that we have the full azimuthal coverage.
_Changed, showing STAR as well now. I couldn't make a graphic I liked
demonstrating the EPD usage_
- s6: No strong momentum -> No strong p_T
_Changed_
- s8: you can remove "Effect demonstrated with a toy model", this
information is below.
_Removed_
- s11-13: as you go from slide 11 to 13, add: R=0.2 then R=0.2 and 0.4
then R=0.2, 0.4 and 0.6, to your first bullet
_ADded_
- s12: "No obvious R dependence!" - make it bold or in colour
_Bolded_
- s13: Elrage x and y-axis title size and the text font size of the
plot.
_Changed_
- s15: appears consistent -> consistent. You can add "in overlapping
p_T region"
_Added_
- s15: you should be a bit careful here. You compare v2 to ALICE 2.76
TeV results. Then you show R_AA from ALICE for 5.02 TeV for charged
jets, and compare it to our isobar single particle R_AA, with
different pT coverages. The discussion may look a bit messy and
far-fetched. I think it's fine that we ask questions, maybe I would
remove "Maybe – Both systems show similar 𝑅AA for mid-central
even". Please try to think a bit on this, how you can make a smooth
but brief story from slides 15-17 and reduce material you're showing
there. Some suggestions below.
_I removed that line, and found a more accurate comparison from ALICE
to use instead. I also removed the claim of similar RAA, since that
wasn't accurate looking at the correct comparison _
- s16: I would suggest removing this or partially merge it with the
next slide. You already have many slides, and it would be good to
focus more on presenting our results.
_Agreed, removed_
- s18-19: I would remove it - you advertise Isaac's poster and if he
shows one then anyway we won't have physics results yet. It's fine to
mention it in the conclusions, as you have now. And your talk is
15min so it might not fit time wise.
_Removed for now, I'm following Isaac's status as well. I had a
little extra time in my practice talk so I'll keep track of what
happens._
- Add the STAR logo on your slides.
_Added_
On Fri, Mar 17, 2023 at 12:06 PM Barbara Trzeciak
<barbara.trzeciak AT gmail.com> wrote:
Hi Tristan,
please find below my comments to your nice slides.
- s2: add references related to the coll. and radiative processes
- s3: the last bullet - please follow the status of Isaac's poster
- s4: define v2. I would rephrase the last bullet. The mechanisms
causing v2 are different at low and high pT, but it's still v2
observable. Maybe something along the line: "non-zero v2 at high pT
due to jet quenching"
- s5: change title of the slide, e.g. Event Plane Reconstruction
- s5: before run 18 -> before 2018
- s5: since you don't show STAR or don't have more details on the
used detector for the jet reconstruction, I suggest to add at least
information that we have the full azimuthal coverage.
- s6: No strong momentum -> No strong p_T
- s8: you can remove "Effect demonstrated with a toy model", this
information is below.
- s11-13: as you go from slide 11 to 13, add: R=0.2 then R=0.2 and
0.4 then R=0.2, 0.4 and 0.6, to your first bullet
- s12: "No obvious R dependence!" - make it bold or in colour
- s13: Elrage x and y-axis title size and the text font size of the
plot.
- s15: appears consistent -> consistent. You can add "in overlapping
p_T region"
- s15: you should be a bit careful here. You compare v2 to ALICE
2.76 TeV results. Then you show R_AA from ALICE for 5.02 TeV for
charged jets, and compare it to our isobar single particle R_AA,
with different pT coverages. The discussion may look a bit messy and
far-fetched. I think it's fine that we ask questions, maybe I would
remove "Maybe – Both systems show similar 𝑅AA for mid-central
even". Please try to think a bit on this, how you can make a smooth
but brief story from slides 15-17 and reduce material you're showing
there. Some suggestions below.
- s16: I would suggest removing this or partially merge it with the
next slide. You already have many slides, and it would be good to
focus more on presenting our results.
- s18-19: I would remove it - you advertise Isaac's poster and if he
shows one then anyway we won't have physics results yet. It's fine
to mention it in the conclusions, as you have now. And your talk is
15min so it might not fit time wise.
- Add the STAR logo on your slides.
Cheers,
Barbara
On Fri, Mar 17, 2023 at 12:48 PM Nihar Sahoo via Star-hp-l
<star-hp-l AT lists.bnl.gov> wrote:
Hello Tristan,
Please find my comments on your nice presentation slides.
_________
General comment/suggestion to all HP2023 and DIS2023 presenters:
1. Please make a Drupal page for all your preliminary plots and
provide
us the link.
If you have already done that, please send us the link.
2. While preparing your analysis plots for "STAR preliminary"
request,
please follow the guidance 1-7:
https://drupal.star.bnl.gov/STAR/pwg/common/Preliminary-figures
It saves our time.
_________
Please increase your slide number font size and use different
color. It
is invisible.
Slide-2:
1. "The contribution of each process to jet quenching is unknown
"-> But
we do know in QGP radiative process dominates over collisional
process.
So this sentence probably needs to rephrase unless you want to say
somethingelse.
2. Can you give reference for collisional E_loss's L dependence?
3. For radiative case L^2 dependence comes from BDMPS. So you need
to
give reference.
SLide-3
1. In this plot, increase the X-axis title and label size (also
for
Y-axis). Not visible.
2. "Central events show significant hadron suppression at high
momentum"
-> " 0-10% central events show significant hadron suppression
at high
momentum"
3. You need to mention what are <Ncoll> and sigma_inel^NN and
their
values used for this result?
SLide-4
1. "Semi-central collisions produce an approximately elliptical
QGP" ->
"Semi-central collision produces a elliptical geometry of the QGP
medium"
2. "To use familiar language, we will report this as 𝑣2,
despite jet
quenching being being distinct mechanism from flow" Not sure what
you
want to say here.
3. I think you need to introduce what is v2 as 2nd order
anisotropy in
this slide?
Slide-6
1. X-axis title: pT^reco -> "pT^trak;
2. X-axis: increase title and label size; put unit
3. Y-axis: increase title and label size
4. You need to mention before or in this slide what is pT?
5. "No strong momentum dependence observed " -> "No transverse
momentum
dependence of v_{2} observed at high-p_{T}"
Slide-7
1. "Measuring high 𝑝T charged hadron 𝑣2 gives us a
connection to flow
measurements " Not sure what you want to say? Why only "high-pT
charged
hadron v2 gives connection to flow"? Please rephrase
2. "…with resolutions …" -> "…with resolution (R)…" here
you can
introduce jet R.
3. Give STAR paper's reference to this upper v2 plot.
Slide-9:
1. "2 GeV" -> "2 GeV/c"
2. "The event is clustered into jets with the anti-𝑘T
algorithm" -> You
have mentioned already in the above sentence. Drop this bullet.
3. "Δ𝑅 < R_resolution " you need to find a better way to
write this.
What is R_resolution?
4. First subbullet of last bullet expression: you need to mention
what
are pT^measured, rho(phi), A, etc?
SLide-10:
1. Title: "Combinatorial Jet Quenching" sounds awkward. Please
rephrase
this. Something like "Combinatorial jet contribution"
2. Put this slide in backup. If somebody asks then show.
Otherwise you
don't need to speak on this test.
SLide-11,12,13:
1. Please follow the same suggestion on this fig from
Slide-6
2. "Small, non-zero R=0.2 anti-𝑘T jet 𝑣2 in isobar
collisions at STAR "
-> "Non-zero jet v_{2} is observed for R=0.2 in isobar collisions"
(same
for SLide12)
3. "Like charged particle …" -> "Like inclusive charged
particle…"
4. "No obvious R dependence!" -> "No jet R dependence of
v_{2} is
observed" (Not sure why it is "Obvious"?)
Slide-14:
1. Please follow the same suggestion on this fig from Slide-6
2. "To remove correlations by comparing the same partons, the
numerator
and denominator are separate sets of events"
Can you please rephrase this sentence to make it more
clear?
Cheers
Nihar
On 2023-03-17 10:45, Tristan Protzman via Star-hp-l wrote:
Hi All,marked
There are still a few supporting figures I am remaking, clearly
as such. These should be done in the next day or two at thelatest,
and I will share when I have updated them. The text and messageof
those slides however is complete.for a
Cheers,
Tristan
On Fri, Mar 17, 2023 at 1:13 AM webmaster--- via Star-hp-l
<star-hp-l AT lists.bnl.gov> wrote:
Dear Star-hp-l AT lists.bnl.gov members,
Tristan Protzman (tlp220 AT lehigh.edu) has submitted a material
contactreview,
please have a look:
https://drupal.star.bnl.gov/STAR/node/63006
Deadline: 2023-03-26
---
If you have any problems with the review process, please
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[Star-hp-l] STAR presentation by Tristan Protzman for Hard Probes 2023 submitted for review,
webmaster, 03/17/2023
-
Re: [Star-hp-l] STAR presentation by Tristan Protzman for Hard Probes 2023 submitted for review,
Tristan Protzman, 03/17/2023
-
Re: [Star-hp-l] STAR presentation by Tristan Protzman for Hard Probes 2023 submitted for review,
Nihar Sahoo, 03/17/2023
-
Re: [Star-hp-l] STAR presentation by Tristan Protzman for Hard Probes 2023 submitted for review,
Barbara Trzeciak, 03/17/2023
-
Re: [Star-hp-l] STAR presentation by Tristan Protzman for Hard Probes 2023 submitted for review,
Tristan Protzman, 03/21/2023
-
Re: [Star-hp-l] STAR presentation by Tristan Protzman for Hard Probes 2023 submitted for review,
Nihar Sahoo, 03/21/2023
-
Re: [Star-hp-l] STAR presentation by Tristan Protzman for Hard Probes 2023 submitted for review,
Tristan Protzman, 03/21/2023
- Re: [Star-hp-l] STAR presentation by Tristan Protzman for Hard Probes 2023 submitted for review, Barbara Trzeciak, 03/22/2023
- Re: [Star-hp-l] STAR presentation by Tristan Protzman for Hard Probes 2023 submitted for review, Yi Yang, 03/22/2023
- Re: [Star-hp-l] STAR presentation by Tristan Protzman for Hard Probes 2023 submitted for review, Tristan Protzman, 03/22/2023
- Re: [Star-hp-l] STAR presentation by Tristan Protzman for Hard Probes 2023 submitted for review, Barbara Trzeciak, 03/23/2023
- Re: [Star-hp-l] STAR presentation by Tristan Protzman for Hard Probes 2023 submitted for review, Tristan Protzman, 03/23/2023
- Re: [Star-hp-l] STAR presentation by Tristan Protzman for Hard Probes 2023 submitted for review, Barbara Trzeciak, 03/23/2023
-
Re: [Star-hp-l] STAR presentation by Tristan Protzman for Hard Probes 2023 submitted for review,
Tristan Protzman, 03/21/2023
- Re: [Star-hp-l] STAR presentation by Tristan Protzman for Hard Probes 2023 submitted for review, Yi Yang, 03/23/2023
-
Re: [Star-hp-l] STAR presentation by Tristan Protzman for Hard Probes 2023 submitted for review,
Nihar Sahoo, 03/21/2023
-
Re: [Star-hp-l] STAR presentation by Tristan Protzman for Hard Probes 2023 submitted for review,
Tristan Protzman, 03/21/2023
-
Re: [Star-hp-l] STAR presentation by Tristan Protzman for Hard Probes 2023 submitted for review,
Barbara Trzeciak, 03/17/2023
-
Re: [Star-hp-l] STAR presentation by Tristan Protzman for Hard Probes 2023 submitted for review,
Nihar Sahoo, 03/17/2023
-
Re: [Star-hp-l] STAR presentation by Tristan Protzman for Hard Probes 2023 submitted for review,
Tristan Protzman, 03/17/2023
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