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Re: [[Star-hp-l] ] STAR presentation by Sooraj Radhakrishnan for HP2024 submitted for review
- From: Nihar Sahoo <nihar AT rcf.rhic.bnl.gov>
- To: star-hp-l AT lists.bnl.gov
- Cc: Sooraj Radhakrishnan <skradhakrishnan AT lbl.gov>
- Subject: Re: [[Star-hp-l] ] STAR presentation by Sooraj Radhakrishnan for HP2024 submitted for review
- Date: Sun, 22 Sep 2024 12:27:18 +0530
Hello Sooraj,
Thank you for implementing some of my comments and answering.
I have no further comments. I sign off.
Best
Nihar
On 2024-09-20 21:05, Sooraj Radhakrishnan wrote:
Hi Nihar,
Thanks for the careful review and comments. The slides are updated
at the same location. Please find my responses to your comments below
//“STAR Preliminary” needs to be included in all plots.//
----- I believe I have it on all plots, could you please point out
which was missing?
Slide3:
You need to define what is “v1”? Formula/expression.
---- Done
//_ Alternate observable - energy loss measurements without need for
p+p
-> This is not needed. Although I understand what do you mean because
unlike R_AA/I_AA. It doesn’t tell about the amount of energy loss.
Jet
v1 is sensitive to path length dependence of energy loss but it can
not
measure energy loss as it is done in R_AA/I_AA. So in this context I
would prefer to drop this.//
------- But it is still accessing energy loss. I changed to 'access to
energy loss'. I think it is important to keep, as there are cases
where we dont have needed p+p baseline for the measurements
//Slide4:
_ I hope you will update the right cartoon that we made recently
_ “Asymmetry along impact parameter direction at finite rapidity”
->
This is not clear to me. I think you mean to say here, “asymmetries
in
participant nucleons motion along the impact parameter axis within
finite rapidity”//
----- I have updated the cartoon and edited the sentences. Please see
//_”Creates difference in path length for hard produced partons at
finite
rapidity” -> By adding new cartoon, you can rephrase this as
“Creates
difference in path length for hard produced partons at forward and
backward direction”//
------ I think finite rapidity is better, I will point to the cartoon
to explain
//Slide5:
_Taking the same dependence for differential production in x and y, ->
for outsider, it is not clear what are x and y ? Please mention it.//
------- I have changed the sentence
//Slide7:
Glauber + Theory -> Please mention what is “Theory” ?
I think, you can combine Slide6 and 7 to make a message that
“asymmetry
of participants along b direction”//
------- I have added the expression in slide for clarification
//Slide8,9:
You can consider to combine these two slides.
And also if you can add that AMPT simulation plot with zero-v1 for
binary profile and non-zero v1 from bulk that would be clear
message.//
-------- I have added the binary profile in the back up
//Slide10:
“hard-soft asymmetry” -> Please mention what is “hard-soft
asymmetry”
Define PL (path length ) before
_ “Can directly access Parton energy loss” -> This is not a
correct
question to impose. Rather I would say “Is jet v1 sensitive to the
path
length dependence of Parton energy loss?
Becasue as I mentioned before we are not measuring energy loss.//
-------- Made the changes. Last bullet changed to 'can access parton
energy loss'
//Slide11:
I think it would be better to discuss EPD and ZDC detectors and how do
you use those detectors to calculate 1st Order event plane angle
compromising 1-2 introductory slides//
------ Given the time, I dont think this is needed. Also this is very
standard. We dont use EPD, use ZDC for both datasets
//Slide12:
_ Before this slide, I think you need to discuss how do you select jet
in this measurement. How do you mitigate combinatoric jet using
pT^lead
cut?
_ You need to mention somewhere this slide, that “AuAu 200 GeV
(2014+2016) data” or similar
_ Need to mention “p_{T,jet}^{reco}” in stead of pT,jet; and you
need to
define “p_{T,jet}^{reco} = pT,jet - rho*A.”//
--------- I have added a slide, Let me know if any more information
needs to be included. Added the definition for p_T,jet^reco
//Slide13: You can keep this slide in backup//
----- I would prefer to show the comparison. I will try to make a
version including charge hadron v1 on the same figure
//Slide14:
_ Need to change x-axis title to “p_{T,jet}^{reco}”
_ Need to mention that are those purple tick markers are. (Bin size of
“p_{T,jet}^{reco}”)
_ Please include what are the sources contributing to this systematic
uncertainty.
_ R dependence -> jet R dependence//
----------- Done. Systematic sources are added in the back-up
//Slide16:
_ Please cite this proceedings https://arxiv.org/pdf/2008.08789 [1]
for
bottom right figure//
----- This slide is remove now. Added comparison to v1 calculation
//Slide17:
Please keep Au+Au and Isobar data (from slide14) side-by side to make
a
statement “isobar collisions consistent with Au+Au within
uncertainties”
Slide18:
I think you don’t need to a dedicated slide for an outlook, you can
have
just one sentence at the end.//
----- I moved this to after summary as an outlook
thanks,
Sooraj
On Wed, Sep 18, 2024 at 5:51 AM Nihar Sahoo <nihar AT rcf.rhic.bnl.gov>
wrote:
Hello Sooraj,
Thank you for this interesting measurement and slides.
Please find my comments below.
“STAR Preliminary” needs to be included in all plots.
Slide3:
You need to define what is “v1”? Formula/expression.
_ Alternate observable - energy loss measurements without need for
p+p
-> This is not needed. Although I understand what do you mean
because
unlike R_AA/I_AA. It doesn’t tell about the amount of energy loss.
Jet
v1 is sensitive to path length dependence of energy loss but it can
not
measure energy loss as it is done in R_AA/I_AA. So in this context I
would prefer to drop this.
_need to introduce what is v1 and v2?
Slide4:
_ I hope you will update the right cartoon that we made recently
_ “Asymmetry along impact parameter direction at finite
rapidity” ->
This is not clear to me. I think you mean to say here,
“asymmetries in
participant nucleons motion along the impact parameter axis within
finite rapidity”
_”Creates difference in path length for hard produced partons at
finite
rapidity” -> By adding new cartoon, you can rephrase this as
“Creates
difference in path length for hard produced partons at forward and
backward direction”
Slide5:
_Taking the same dependence for differential production in x and y,
->
for outsider, it is not clear what are x and y ? Please mention it.
Slide7:
Glauber + Theory -> Please mention what is “Theory” ?
I think, you can combine Slide6 and 7 to make a message that
“asymmetry
of participants along b direction”
Slide8,9:
You can consider to combine these two slides.
And also if you can add that AMPT simulation plot with zero-v1 for
binary profile and non-zero v1 from bulk that would be clear
message.
Slide10:
“hard-soft asymmetry” -> Please mention what is “hard-soft
asymmetry”
Define PL (path length ) before
_ “Can directly access Parton energy loss” -> This is not a
correct
question to impose. Rather I would say “Is jet v1 sensitive to the
path
length dependence of Parton energy loss?
Becasue as I mentioned before we are not measuring energy loss.
Slide11:
I think it would be better to discuss EPD and ZDC detectors and how
do
you use those detectors to calculate 1st Order event plane angle
compromising 1-2 introductory slides
Slide12:
_ Before this slide, I think you need to discuss how do you select
jet
in this measurement. How do you mitigate combinatoric jet using
pT^lead
cut?
_ You need to mention somewhere this slide, that “AuAu 200 GeV
(2014+2016) data” or similar
_ Need to mention “p_{T,jet}^{reco}” in stead of pT,jet; and you
need to
define “p_{T,jet}^{reco} = pT,jet - rho*A.”
Slide13: You can keep this slide in backup
Slide14:
_ Need to change x-axis title to “p_{T,jet}^{reco}”
_ Need to mention that are those purple tick markers are. (Bin size
of
“p_{T,jet}^{reco}”)
_ Please include what are the sources contributing to this
systematic
uncertainty.
_ R dependence -> jet R dependence
Slide16:
_ Please cite this proceedings https://arxiv.org/pdf/2008.08789 [1]
for
bottom right figure
Slide17:
Please keep Au+Au and Isobar data (from slide14) side-by side to
make a
statement “isobar collisions consistent with Au+Au within
uncertainties”
Slide18:
I think you don’t need to a dedicated slide for an outlook, you
can have
just one sentence at the end.
Best
Nihar
On 2024-09-11 20:32, webmaster AT star.bnl.gov wrote:
Dear Star-hp-l AT lists.bnl.gov members,material
Sooraj Radhakrishnan (skradhakrishnan AT lbl.gov) has submitted a
for a
review, please have a look:
https://drupal.star.bnl.gov/STAR/node/68896
Deadline: 2024-09-22
---
If you have any problems with the review process, please contact
webmaster AT www.star.bnl.gov
--
Sooraj Radhakrishnan
Research Scientist,
Department of Physics
Kent State University
Kent, OH 44242
Physicist Postdoctoral AffiliateNuclear Science Division
Lawrence Berkeley National Lab
MS70R0319, One Cyclotron Road
Berkeley, CA 94720
Ph: 510-495-2473 [2]
Email: skradhakrishnan AT lbl.gov
Links:
------
[1] https://urldefense.com/v3/__https://arxiv.org/pdf/2008.08789__;!!P4SdNyxKAPE!EsoglMx-W-kCoS9d-TFWue6I8RzWLZ4ZJScU15ubjLPaPqgLgbDpkpzq_jD_5SRT5HGjdA4fJBC_yxWDoHGifWhbmLXcFhzEBik$
[2] tel:%28510%29%20495-2473
-
[[Star-hp-l] ] STAR presentation by Sooraj Radhakrishnan for HP2024 submitted for review,
webmaster, 09/11/2024
- Re: [[Star-hp-l] ] STAR presentation by Sooraj Radhakrishnan for HP2024 submitted for review, Yi Yang, 09/17/2024
-
Re: [[Star-hp-l] ] STAR presentation by Sooraj Radhakrishnan for HP2024 submitted for review,
Nihar Sahoo, 09/18/2024
-
Re: [[Star-hp-l] ] STAR presentation by Sooraj Radhakrishnan for HP2024 submitted for review,
Sooraj Radhakrishnan, 09/19/2024
- Re: [[Star-hp-l] ] STAR presentation by Sooraj Radhakrishnan for HP2024 submitted for review, Yi Yang, 09/19/2024
- Re: [[Star-hp-l] ] STAR presentation by Sooraj Radhakrishnan for HP2024 submitted for review, Nihar Sahoo, 09/20/2024
-
Re: [[Star-hp-l] ] STAR presentation by Sooraj Radhakrishnan for HP2024 submitted for review,
Sooraj Radhakrishnan, 09/20/2024
- Re: [[Star-hp-l] ] STAR presentation by Sooraj Radhakrishnan for HP2024 submitted for review, Nihar Sahoo, 09/22/2024
-
Re: [[Star-hp-l] ] STAR presentation by Sooraj Radhakrishnan for HP2024 submitted for review,
Sooraj Radhakrishnan, 09/19/2024
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