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  • From: Nihar Sahoo <nihar AT rcf.rhic.bnl.gov>
  • To: Tristan Protzman <tlp220 AT lehigh.edu>, STAR HardProbes PWG <star-hp-l AT lists.bnl.gov>
  • Cc: Yi Yang <yiyang0429 AT gmail.com>, webmaster AT star.bnl.gov
  • Subject: Re: [Star-hp-l] STAR presentation by Tristan Protzman for Hot Quarks 2022 submitted for review
  • Date: Sun, 09 Oct 2022 13:43:59 +0530

Hello Tristan,

Thank you for implementing my comments and your reply.
Please find my further comments and reply to your response.
All my comments on your recent version (v4).
Please don't remove your old version; that can be done after finishing our discussion otherwise it is difficult to follow the slide numbers with new version.

1) Have you updated your remaining sys uncertainty that we were waiting for?

2)Comments on Figures:
Slide18 fig:
1. You don't need to put description of "ALCIE sys bands like correlated and uncorrelated etc" One green circle is enough to represent ALICE results.
2. Please include instead STAR sys box's description in legend

Slide17 fig:
_ Can you include v2 value (with uncertainty) in this figure that you get from the fitting?


3) Additional comment:
I think EPD is used for the first time in jet v2 measurement.
It would be good to include EP resolution plot that you get from this measurement.
For that you can combine slide15-16 to make a story for EPD and EP calculation.


4) Slide18(in vesrion4):
"Suggests that jet modification is path-length dependent, even in medium sized systems!"
Can you please elaborate how we draw the conclusion of " jet modification is path-length dependent" in Isobar ?
We don't have any hard-core jet RAA/RCP measurement in isobar. Do we have?

We can only say so far (from this preliminary study) what you have mentioned in conclusion slide19 (with slight modification "hint…")
"Hint of non-zero v2^ch jet is observed in a medium sized system "

Please bring this statement in slide18


5) Slide19(v4 version)
_"A very different system!" -> "A very different kinematic range and system size"
_"v2ch jet is observed despite the introduced surface bias" -> "v2ch jet is observed despite the possible surface bias"
I would be careful on this statement, as I mentioned we have not done any dijet Aj study in Isobar to support of the surfaced bias jet selection. It could be correct but we have not done any measurement so we should abstain mentioning this.
If you want, then need to do Aj measurement for this hard core jet selection in Isobar.

_"Our picture of jet quenching is not complete - there is still much to discover"
Sounds a vague statement. Please mention 1) what is not completed relating to jet quenching? 2) what do you think that needs to be discovered? Please elaborate this.


Remaining reply can be found inline.

On 2022-10-09 07:56, Tristan Protzman via Star-hp-l wrote:
Hello Nihar,

A new draft has been uploaded to Drupal.

Note: it should be written as $p$+$p$ and $p$+Au, etc, which is
different from the guidance.

Fixed.

Slide:2
_Second bullet seems out of context here. Coupling is large at low Q^2
then why is it relevant for the QGP and your jet anisotropy
measurements? This part is not clear here.
It motivates the need for a perturbative object like jets to probe
what we actually want to study, the QGP. Changed text to clarify.

Still it is not clear and confusing for 1st and 3rd bullets.
If you want to motivate jet (which pQCD calculable) and this is used to probe QGP (which is asymptotic region of coupling); then what is the point to mention "alpha_s ~ O(1) at low Q^2."
I would suggest to rephrase;
"Since running coupling is asymptotically small at high Q^2, pQCD calculable probes are used to study the QGP medium"
Then you don't need 3rd bullet.



_ Give reference to the running coupling plot. And you could replace
with most updated version where LHC measurements (very highQ2 region)
are included if you want to start with it.
Changed.

__GIve a reference or credit for left cartoon._

Figure removed, I felt it did not add to the message.

Slide:4
_3rd bullet: "Leads to path length…" this is not the only effect;
it
could be various other contributions like color factor, Temp of QGP,
initial gluon density, etc. But you need to mention Your motivation is
to study "path length dependence".
__ same comment for 4th bullet_
I have adjusted this section to clarify that the aspect of jet
modification I am trying to study is the path length dependent nature
of jet energy loss

Slide4 (current v4)
_ "We are interested in understanding the path-length dependence of these processes" -> "We are interested in understanding the path-length dependence of jet quenching"

_"Both collisional and radiative" -> "Both collisional and radiative energy loss" or "Parton energy loss via both collisional and radiative processes"


_ 5th Bullet ("Both collisional and radiative") you need to provide
reference to the theory calculation for this L/L^2 dependence. These
are
model calculations.

Slide4 (current v4)
_"Both collisional and radiative" -> "Both collisional and radiative energy loss" or "Parton energy loss via both collisional and radiative processes"



Removed L/L^2 statements as I am not comparing to any models in this
presentation

_ This slide only focus on jet and jet quenching, but it doesn't
motivate your measurement like why jet anisotropy measurement is
required? Need to include some text on it.
I suggest you need to motivate jet anisotropy before you go to any jet
analysis details like in Slide5 underlying event discussion

The way I have structured my talk is to first motivate that we have
observed jet quenching. I am using the dijet analysis to this end. I
then want to contrast that with azimuthal anisotropy, which is not a
dissimilar measurement in that it probes jet modification, but it does
so in a new way. Therefore, I think it makes sense to talk about jet
measurements and then the dijet measurement before introducing the
idea of anisotropy and motivating how that can get us towards the
missing path length dependence of a dijet analysis.

SLide:5
_Not clear, what is that right side plot? Is this data or MC
simulation.
What is pT, of track or jet? What is Delta phi?
I agree, this plot was not particularly clear. I have removed it.
__"Soft processes produce a fluctuating background" what is that_
_background? Is it track or _combinatoric_ jet background?_
I'm not quite sure I understand what you are asking, it is the tracks
from soft processes which produce the combinatorial jet background, so
I suppose both?
Then it would good to mention, "Soft processes produce a fluctuating uncorrelated background for jet measurement in heavy-ion collisions"
Here "uncorrelated" is important.

Slide5 (current v4), right figure is from STAR data or any model? No description mentioned there.

__3rd _bulltet_ (Estimated…) it should _be sub-bullet_ of 2nd bullet
(Soft_
_process…)_
Changed.
__ what is kT?_
The k_T jet finding algorithm, clarified.
__ Jet area -> Jet area(A)_

Changed.

Slide6:
_Not clear, what is that right side plot? Is this data or MC
simulation?
What is pT, eta, and phi?
This is the total track momentum for eta/phi bins for a collision.
__"A jet finder… had scattering and other processes" ->" had
scattering_
_and combinatorial background in heavy-ion collisions"_
_2nd bullet is not required if you mention above.

_ _I have merged this with slide 5 and changed this wording

SLide:7
I would suggest to use jet pT as $p_{\rm T, jet}$ throughout your
presentation.
Changed.
__Used in other STAR analysis -> Proved references_
__Provide _referecen_ to ALICE measurement_

Done.

Slide:8
_Move this slide or Isobar jet pT distribution after your slide14
where
you discuss about Isobar dataset. It seems the left side plot just
pop-up. This plot should be part of you results discussion even if it
is
a STAR performance plot.
Figure removed
__"Statistically unlikely for soft processes…" Please rephrase
this… not_
_clear._
Changed to clarify that it is unlikely for soft processes to produce
high pt hadrons which look like jets
__"May bias jet selection towards surface" Not sure the motivation of_
_this bullet. _why it is_ important? You are not doing jet RAA/RCP
study_
_and you do not study trigger jet v2 then why it is important if this
jet_
_is trigger biased or not. These jets should be treated as inclusive
_jet_._

Is it not important to understand the biases we introduce into our
measurements? By requiring the high pT hadrons the selected jets are
biased towards the surface of the QGP. This is the motivation for one
of the items we would like to explore next in this analysis, the
variation of the hard core threshold.

Slide:9
This slide is not relevant. You could put in Backup. (A distraction)

I disagree, the story I am hoping to tell with this talk is that we
saw signs of jet quenching with measurements like dijet imbalance, but
that it doesn't tell the complete story. We can continue our
understanding of jet quenching from dijet measurements to jet v2
measurements.

slide8(in v4)
_ we are doing inclusive hard-core jet v2 measurement here. Is not it?
_I am not convinced to motivate with dijet measurement here. Are we going to do any dijet measurement in isobar?
_Selecting a hard-core jet may not imply you select surface biased jet. For that you need to show the same dijet Aj measurement in isobar like in Au+Au. If you have any result to demonstrate that you are selecting surfaced bias jet in Isobar, please show those results.
I think we have not done that study.


Slide:10
_ 1st bullet: Why it is important for Dijet imbalance discussion here?
You are doing inclusive jet v_n measurement. Not clear to me.

See above.

Please see above my concerns.


SLide12
_"A jet in plane interacts with less medium than one out of plane" ->
"A
jet interacts less with medium in plan than out of plane"
Changed.
__"Since jet production is isotropic, differences in yields are a
result_
_of medium interactions" Not sure, _what you_ want to say here?
Please_
reprhase_._
Changed.
__" like flow" Remove this._
I included this to help give context for the measurement to an
audience who may be familiar with flow studies, but not jet anisotropy
studies. If you feel this is misleading I will remove it.
__ you do not discuss what is v_{2}^{jet} is?_
Changed equation to remove \Delta\phi -> \Psi_2 - \Phi_jet
__"Not a flow effect though!" Can you elaborate this?_

I am stating that although it may be described using the same
framework as flow measurements, jet v2 is a different process.

I would suggest to give a clear idea what could be that different process, For example...?
Otherwise do not create unnecessary doubt or make statement just for a buzz?



SLide13
_RHIC produces a different, cooler QGP -> "RHIC produces a cooler QGP
medium than the LHC"
Changed.
__"Down to 10 _GeV"_ -> But you are not going to show down to 10 GeV.
So_
_just remove this extra quantifier _subbullet. Main bullet is fine.

I do show down to 10 Gev though, my first point is 10-12.5 GeV/c jets.

Slide15:
- Jet trigger -> You don't use any jet trigger and BEMC info in your
measurement. If yes, just remove.
I do use the barrel high tower trigger in my analysis, as detailed in
the preliminary figure request. I have clarified this as high tower
trigger rather than jet trigger.
_- Right side STAR detector, please indicate where is TPC, BEMC, EPD_
_- Mention kinematic acceptance of these detectors_

See updated slides, Yi mentioned this as well

Slide16:
_you did not discuss what is Delta_phi?
I did not, but I am not sure I need to on this slide. I will discuss
it on the next slide.
__right side plot, _make title_/_lable_ of x-, y-axis bigger so that
it will_
_be visible. And also legends _in side_ the plot._
Changed, made entire plot larger as well

Slide18
Move this slide after Slide15

Changed.

Slide19
_INside fig, mention "red line" is fit fun.
Added.
__ inside fig, p_T^reco -> p_{\rm T, jet}^{reco} ; 12.5 -> 12.5 GeV/c_
Changed.
__ you did not mention anywhere before what is "R"? And what jet _R
you
are_ going to _do measurement_?_
It is labeled on the plot, and I will discuss it further on the
following slide.
__ what is v_{2}^ch? Need to mention _it charged_ jet v2. I would
suggest_
to use $v_{2}^{\rm ch, jet}$; And the same about v_{2}^ch,abs

Changed.

Slide20:
Before slide20, you need to discuss different jet v2 (all, hard core,
matched jet) and their spectra showing side-by-side

I'm not sure I understand why? I think that was a good check to make
and certainly worth having in the backup, but the measurement being
presented is jet v2 using the hard core matching criteria, the need
for which is motivated earlier in the talk.

Slie21:
_ "Jet v2 is a exciting measurement for determining the path-length
dependence of jet quenching" -> This statement is fine to motivate.
But
for your conclusion this may not be relevant. Because we don't have
jet
v2 measurement for different path length/system size with the same
kinematic coverage. And you did not discuss what is the strategy for
your measurement unless you plan to do the same in AU+AU.

_"Jets which are in plane interact with a different amount of the QGP
than those out of plane" Not sure how do you get this conclusion from
your measurement.

I have updated my conclusions to better reflect the points I wish to
make and where I will go next with this analysis.




Thank you
Nihar
On Thu, Oct 6, 2022 at 1:34 PM Yi Yang <yiyang0429 AT gmail.com> wrote:

Dear Tristan,

Thanks a lot for the reply and the updated version.
They look very good to me.
Let's wait for your study and the decision on the preliminary
results!

Cheers,
Yi

On Thu, Oct 6, 2022 at 3:26 AM Tristan Protzman <tlp220 AT lehigh.edu>
wrote:

Hi Yi,

Thank you for the feedback! I have uploaded an updated version and
addressed your comments below.

- p4: Are the sub-bullet for the 3rd bullet and the 4th bullet the
same?

Yes, I have removed that redundancy.

- p6: toy mode --> toy model

Fixed.

- p9: Just for my own education, could you please tell me why A_j
can be less than 0 (I am assuming pT^1 and pT^2 are leading and
subleading jet pT, respectively, is it correct)?

Yes, (pT^1, pT^2) is the (leading, subleading) jet pT. The red
points are the measurement of A_j using only hard cores. This is
where leading and subleading are determined, thus no points below 0.
However, after matching is done, leading and subleading are not
recalculate, so it is possible for the subleading hard core to match
to a jet with more momentum than the leading hard core does,
resulting in negative A_j. There are a few ways this could happen.
The subleading jet could contain a larger soft component than the
leading jet, thus when added to the hard core the magnitudes flip.
Additionally, because of the fluctuating background the leading jet
could be over subtracted and the subleading jet under subtracted,
again flipping the relative magnitude. This would not affect the
hard core since background subtraction is not done on that
collection.

- p15: It would be good if you can provide more information for the
subdetectors, for example eta and phi coverage...

I added more information about each system and labeled the picture.

- p18: Jet v2 not feasible --> Jet v2 is not feasible

Changed to Jet v2 was not feasible

Cheers,
Tristan

On Wed, Oct 5, 2022 at 1:59 PM Yi Yang <yiyang0429 AT gmail.com> wrote:

Hi Tristan,

Thanks a lot for the nice slide. I have some suggestions/comments
for your consideration.
- p4: Are the sub-bullet for the 3rd bullet and the 4th bullet the
same?
- p6: toy mode --> toy model
- p8: Title: Hardcore --> Hard core
- p9: Just for my own education, could you please tell me why A_j
can be less than 0 (I am assuming pT^1 and pT^2 are leading and
subleading jet pT, respectively, is it correct)?
- p15: It would be good if you can provide more information for the
subdetectors, for example eta and phi coverage...
- p18: Jet v2 not feasible --> Jet v2 is not feasible
- Since we are not settled with your preliminary results yet, I
will comment on p20 and p21 later. :-)

Cheers,
Yi

On Thu, Oct 6, 2022 at 12:36 AM Tristan Protzman via Star-hp-l
<star-hp-l AT lists.bnl.gov> wrote:

Hi All,

I submitted this material for review last week, but it seems to have
been lost somehow, so I am resending it.

Cheers,
Tristan

On Wed, Oct 5, 2022 at 12:33 PM 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 for a
review,
please have a look:
https://drupal.star.bnl.gov/STAR/node/61264

Deadline: 2022-10-11
---
If you have any problems with the review process, please contact
webmaster AT www.star.bnl.gov
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