star-hp-l AT lists.bnl.gov
Subject: STAR HardProbes PWG
List archive
Re: [Star-hp-l] Preliminary request for J/psi spin alignment measurement in Isobar data
- From: tc88qy <tc88qy AT rcf.rhic.bnl.gov>
- To: Nihar Sahoo <nihar AT rcf.rhic.bnl.gov>
- Cc: STAR HardProbes PWG <star-hp-l AT lists.bnl.gov>, Barbara Trzeciak <barbara.trzeciak AT gmail.com>
- Subject: Re: [Star-hp-l] Preliminary request for J/psi spin alignment measurement in Isobar data
- Date: Fri, 22 Sep 2023 13:55:40 +0800
Hi Nihar,
Yes, that plot is not in the preliminary request.
Qian Yang
On 2023-09-22 12:34, Nihar Sahoo wrote:
Hello Qina,
Please find my reply inline.
On 2023-09-21 19:52, tc88qy wrote:
Hello Nihar,
STAR released ZDC first-order EP results at QM. People may ask do we
have a comparison
between first-order EP and second-order EP. That the reason we did the
comparison.
We can keep in mind that they do have difference just as you and
Subhash motioned.
I look at your preliminary request:
https://drupal.star.bnl.gov/STAR/system/files/Preliminary_figures_request_1.pdf
You have probably removed that comparison plots. Is not it?
Besides, your preliminary request looks fine to me.
With these, I sing off.
Thank you
Nihar
If you don't have further question, can I understand it as an sign-off?
Hello Subhash
Thanks for pointing to the paper
Qian Yang
On 2023-09-21 16:40, Nihar Sahoo wrote:
Hello Qian,
Thank you addressing my comments. All your responses are fine to me.
One follow up on your this reply.
Actually, Do you have any physics expectation to the comparison if2.I just talking about the data, error bars can touch each other bySorry, Not clear.
using "TPC 2nd order EP" and "ZDC 1st order EP".
the 1st order EP have such large error bars?
If you look at my earlier comment copied here. Probably, my earlier
comment was not clear.
2. On Slide 4, My expectation that "TPC 2nd order EP" and "ZDC 1st
order EP" may give a bit different results. But you quote "Results are
consistent with each other due to large error bars in first order
measurement". It sounds like using different Detectors ( TPC vs. EPD)
and EP order (1st vs 2nd) results are still consistent. Is that you
want to say?
What I want say is, if we use different detectors (central vs. forward
acceptance) and also different (1st vs 2nd) order EP to calculate your
J/psi spin alignment then do we expect the results would be the same
or not?
My expectation: it may not give the same because using TPC and ZDC
detector have different correlation to acceptance region. And also
different order EP could be another factor.
But you quote "Results are consistent ..."
Just to know your comment on it.
Thank you
Nihar
On 2023-09-21 13:00, tc88qy wrote:
Hello Nihar,
Please find my reply inline.
On 2023-09-20 18:16, Nihar Sahoo wrote:
Hello Qian,we probably need to think about the physics information we want to look at.
Please find my reply inline.
On 2023-09-20 14:56, tc88qy wrote:
Hello Barbara and NiharHow do you know what is _clear physics_?
I included 0-5% centrality to the first bin in the preliminary
request plots. The results have been updated in the preliminary
request plots. Please look at the it in this link:
https://drupal.star.bnl.gov/STAR/system/files/Preliminary_figures_request_1.pdf
Hi Nihar
1.Just as I mentioned in previous email. We should look at a
centrality range with clear physics information.
In our case, it is the charm and anti-charm correlation that affecting by QGP.
In most the Au+Au analysis, STAR paper then talk about QGP in a
centrality of 0-60% or 0-50%, just like the phi spin alignment paper
are carry out at 20-60%. 20-50% or 20-60% centrality is what people
usually look at for QGP related study.
In peripheral collision, the case could very different from central
and semi-central collision.
I think it would be good to using 0-20%, 20-50% and 50-80% centrality bins.Actually, Do you have any physics expectation to the comparison if
2.I just talking about the data, error bars can touch each other bySorry, Not clear.
using "TPC 2nd order EP" and "ZDC 1st order EP".
the 1st order EP have such large error bars?
done
3. donePlease include in your preliminary request also.
4. The rho_00 central value in 50-80% is on top of 1/3. While by
looking at the pT dependence of the same centrality,
every data points central value is above 1/3. This is
inconsistency and related to yield extraction method.
5. will done in the talk
This is the first time I know that we have style requirement for Physics plots.
6. Please check in the preliminary request plot
Please find additional comment on your preliminary request:
https://drupal.star.bnl.gov/STAR/system/files/Preliminary_figures_request_1.pdf
1) Slide13-14: "Centrality Integral" data point, the plotting style is
incorrect because of X-axis.
I suggest to use the style of plotting in Fig.2 of Uplsilon PRL paper.
https://journals.aps.org/prl/pdf/10.1103/PhysRevLett.130.112301
I have update it in the same link.
In each plots, I updated it with a legend to mention the pT and y
2) Slide 15: "global spin alignment signal mainly from the pT range 1-3 GeV/c"
Do you mean you only use 1-3 gev/c range only for centrality
dependence plot like fig. in SLide13,14?
If so, why don't you consider 3-4 gev/c range?
range we used in the analysis.
And after discuss with fcv group, we decide not show the pT dependence.Yes, we plan to show both. Fig 1. just show people the signal over centralities.
3) Do you have plan to show both Fig.1 and Fig,2 outside as STAR preliminary?
I am wondering because Fig.2 shows there may be a centrality
dependence, other hand Fig.1 shows fluctuations across centralities
and also contradicts the earlier.
In figure 2, We do not say there is a centrality dependence.
We emphasize the centrality range we selected.
0-20% with the largest J/psi regeneration probability.
20-50%, QGP with largest angle momentum or particle v2.
50-80%, a reference
Qian Yang
Thank you
Nihar
Regards,
Qian Yang
On 2023-09-20 15:51, Nihar Sahoo wrote:
Hello Qian,
My apologies, for my late response.
Please find my comments on your preliminary request.
1. On Slide3 "Centrality binning", I would prefer to use 0-20%,
20-40%, and 40-80% binning. Let me know what do you think. As is done
in Slide4 right side figure with STAR preliminary.
2. On Slide 4, My expectation that "TPC 2nd order EP" and "ZDC 1st
order EP" may give a bit different results. But you quote "Results are
consistent with each other due to large error bars in first order
measurement". It sounds like using different Detectors ( TPC vs. EPD)
and EP order (1st vs 2nd) results are still consistent. Is that you
want to say?
3. Slide5 left fig: I think you need to include 0-20% instead of 5-20%
centrality for pT-dependence plot. Is not it? [same for Slide7]
4. Slide5: "ρ00 systematic above 1/3 in pT dependence study for
50-80%…" -> But it looks all are consistent with 1/3 (dotted line)
within uncertainty except 2-3 GeV/c pT bin (just ~1 sigma difference).
Is not that?
5. SLide8: Please Include ALICE reference.
6. Please include also Physics message/conclusion on Slide 6,7,8.
Thank you
Nihar
On 2023-09-20 11:39, Barbara Trzeciak via Star-hp-l wrote:
Hi Qian,
I don't have strong preference about the 40, 50 or 60%, you can leave
it as you had, 20-50 and 50-80%.
The main point was about not excluding the 0-5% range.
So from my side it's fine. But please wait if conveners have any
comments on this.
Cheers,
Barbara
On Wed, 20 Sept 2023, 07:55 tc88qy, <tc88qy AT rcf.rhic.bnl.gov> wrote:
Hi Barbara,https://drupal.star.bnl.gov/STAR/system/files/jpsiSpinAlignment_20230917.pdf
The last centrality bin will have large error bar as shown in my
binning study.
What about 50-80%, it will reduce the error bars.
I also checked the 50-80% <N_part> in Isobar, it is comparable
with
60-80% <N_part> in Au+Au.
Qian Yang
On 2023-09-20 12:51, Barbara Trzeciak wrote:
Hi Qian,check.
that's also fine. My only worry is that you will have large
uncertainty for the pT different rho00 in this bin. But you can
wrote:
Cheers,
Barbara
On Wed, 20 Sept 2023, 05:39 tc88qy, <tc88qy AT rcf.rhic.bnl.gov>
want
Hi Barbara,
I see your point. I agree to include 0-5% centrality to the
first
bin.
If we do 20-40% and 40-80% centrality, the last bin do gain
precisions.
But we probably need to think about the physics information we
talkto
look at. In our case, it is the charm and anti-charm correlation
that
affecting by QGP. In most the Au+Au analysis, STAR paper then
paperabout
QGP in a centrality of 0-60%, just like the phi spin alignment
don'tare
carry out at 20-60%.
So, I suggest we do the binning of 0-20% , 20-60% and 60-80%.
What do you think?
Qian Yang
On 2023-09-19 23:39, Barbara Trzeciak wrote:
Hi Qian,remove
thanks for point to the slides with additional checks.
Regarding 0-5% centrality bin:
As ShinIch also commented, sometimes the most central bin is
due to poor event plane resolution. However, in this case I
thansee
the resolution being particularly bad, it's not so much worse
notfor
the mid-central case. If we have enough confidence to have thispoint
in the centrality differential plot, I don't see a reason why
to
include it when you integrate to wider centrality ranges.the
Regarding the other binning:
The reason for having 20-40% and 40-80% is that the precision of
mid-central point is almost the same while the peripheral bingains in
precision compare to the 50-80% centrality range.wrote:
Cheers,
Barbara
On Tue, 19 Sept 2023, 17:21 tc88qy, <tc88qy AT rcf.rhic.bnl.gov>
Hi Barbara,
I replied to the HP list for the comments I got from last HP
meeting.
Please find the details in this link:
https://drupal.star.bnl.gov/STAR/system/files/Preliminary_figures_request_1.pdfbin.In terms of the binning, I am not sure the reason of 20-40%
case)
Qian Yang
On 2023-09-19 22:15, Barbara Trzeciak wrote:
Hi Qian,slides
I see that you consider three centrality classes on plots on
14-16 - same as you presented last week.looks a
As we discussed in more detail at the previous HP meeting, it
bit weird (and I don't know what's the motivation in this
20-40%that
you exclude 0-5% centrality bin.
I suggest having the first bin as 0-20% centrality, then
thatand
40-80%.
Also, could you please prepare a comparison to the results
use
the first order event plane.
Cheers,
Barbara
On Mon, Sep 18, 2023 at 10:36 AM tc88qy via Star-hp-l
<star-hp-l AT lists.bnl.gov> wrote:
Hello all,
Please find my preliminary plots request in link below:
_______________________________________________
Qian Yang
_______________________________________________
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
-
Re: [Star-hp-l] Preliminary request for J/psi spin alignment measurement in Isobar data
, (continued)
- Re: [Star-hp-l] Preliminary request for J/psi spin alignment measurement in Isobar data, Nihar Sahoo, 09/22/2023
- Re: [Star-hp-l] Preliminary request for J/psi spin alignment measurement in Isobar data, Nihar Sahoo, 09/22/2023
- Re: [Star-hp-l] Preliminary request for J/psi spin alignment measurement in Isobar data, tc88qy, 09/22/2023
- Re: [Star-hp-l] Preliminary request for J/psi spin alignment measurement in Isobar data, Nihar Sahoo, 09/22/2023
- Re: [Star-hp-l] Preliminary request for J/psi spin alignment measurement in Isobar data, tc88qy, 09/22/2023
- Re: [Star-hp-l] Preliminary request for J/psi spin alignment measurement in Isobar data, tc88qy, 09/22/2023
- Re: [Star-hp-l] Preliminary request for J/psi spin alignment measurement in Isobar data, Yi Yang, 09/22/2023
- Re: [Star-hp-l] Preliminary request for J/psi spin alignment measurement in Isobar data, tc88qy, 09/22/2023
- Re: [Star-hp-l] Preliminary request for J/psi spin alignment measurement in Isobar data, Yi Yang, 09/22/2023
- Re: [Star-hp-l] Preliminary request for J/psi spin alignment measurement in Isobar data, tc88qy, 09/22/2023
- Re: [Star-hp-l] Preliminary request for J/psi spin alignment measurement in Isobar data, tc88qy, 09/22/2023
Archive powered by MHonArc 2.6.24.