star-fcv-l AT lists.bnl.gov
Subject: STAR Flow, Chirality and Vorticity PWG
List archive
- From: Sooraj Radhakrishnan <skradhakrishnan AT lbl.gov>
- To: subhash <subhash AT rcf.rhic.bnl.gov>
- Cc: star-fcv-l AT lists.bnl.gov, mfarhan_taseer AT impcas.ac.cn, Diyu Shen <dyshen AT fudan.edu.cn>, Richard Seto <seto AT ucr.edu>, Subhash Singha <subhash AT impcas.ac.cn>, Prithwish Tribedy <prithwish2005 AT gmail.com>
- Subject: Re: [[Star-fcv-l] ] v1 v2 talk at the workshop
- Date: Mon, 2 Dec 2024 10:31:20 -0800
Hi Subhash,
You meant CB = 0 is no diffusion and CB = 1 is with diffusion, right? CB = 1 may not be extreme, seen other calculations with 1.2 etc.
Shinichi, some more details on CB can be found here https://arxiv.org/pdf/1804.10557
Best,
Sooraj
You meant CB = 0 is no diffusion and CB = 1 is with diffusion, right? CB = 1 may not be extreme, seen other calculations with 1.2 etc.
Shinichi, some more details on CB can be found here https://arxiv.org/pdf/1804.10557
Best,
Sooraj
On Mon, Dec 2, 2024 at 5:27 AM subhash <subhash AT rcf.rhic.bnl.gov> wrote:
Dear Shinichi, All,
If you check slide#21, you will see that the parameter C_B is
controlling the baryon diffusion. C_B=0 and 1 is roughly the extreme
cases with and without baryon diffusion.
Thanks and regards,
Subhash
On 2024-12-02 09:19 PM, EsumiShinIchi wrote:
> Dear Sooraj and Muhammad
> Thank you very much for the information.
> Could you please tell me what is the difference between CB=0
> and CB=1 at the page 36-39 of Muhammad’s paper proposal
> slide on 13/Nov/2024?
> Best regards, ShinIchi
>
>> 2024/12/02 16:06、Sooraj Radhakrishnan
>> <skradhakrishnan AT lbl.gov>のメール:
>>
>> Hi Shinichi, Prithwish,
>> Thanks for the slides and comments
>>
>> Regarding the v1 difference and hadro comparisons, there are a
>> couple of points to note
>>
>> 1) The difference in v1 between protons and anti-protons is
>> explained using different initial tilted distributions for the bulk
>> and for transported protons. There is no independent constraint on
>> this and the tilts are tuned to data. In other words, the difference
>> in the final state v1 is carried over to the difference in initial
>> distributions - but without an independent constraint. So doesnt
>> have much predictive power or helps explaining the v1 difference we
>> see. Please find some more details here
>> https://arxiv.org/pdf/2211.15659 [2]
>>
>> 2) What is interesting though is that the centrality dependence is
>> explained through baryon diffusion. As you can see on S.37 here
>>
> https://drupal.star.bnl.gov/STAR/system/files/FCV_Comments_Measurement%20of%20system%20size%20dependence%20of%20directed%20flow%20of%20protons%20%28anti-protons%29%20at%20RHIC_2.pdf,
>> its the baryon diffusion that makes the difference go negative in
>> peripheral collisions. The initial tilt difference is such that the
>> proton v1 gets a positive contribution compared to anti-proton v1.
>> Without the diffusion the difference doesnt go negative. Not sure,
>> but I think its possible, constraints on the baryon diffusion can be
>> checked with other measurements, for example on spectra or v2
>>
>> In short its the baryon inhomogeneity coupled with baryon diffusion
>> that produced negative delta v1 in hydro calculations. Thought that
>> is useful to point out
>>
>> Best,
>> Sooraj
>>
>> On Sun, Dec 1, 2024 at 6:41 PM EsumiShinIchi
>> <esumi.shinichi.gn AT u.tsukuba.ac.jp> wrote:
>>
>>> Dear Prithwish and Diyu
>>> Thank you very much for the suggestions, ALICE D0-D0bar are
>>> already included.
>>> Let’s discuss whether we want to move this to Friday or not.
>>> I’ll try to include
>>> the Lambda results.
>>> Best regards, ShinIchi
>>>
>>>> 2024/12/02 10:48、Diyu Shen <dyshen AT fudan.edu.cn>のメール:
>>>>
>>>> Hi Prithwish and ShinIchi,
>>>>
>>>> I think for this topic it is necessary to include all the
>>> results in heavy-ion experiment, not only from STAR but also from
>>> ALICE.
>>>> So I would suggest to discuss D meson splitting observed by
>>> ALICE after point 5.
>>>>
>>>> Say D-Dbar results show 2.8 sigma splitting, despite D’s have
>>> no electrical charge — challenges naive EM-field explanation.
>>>>
>>>> Best,
>>>> Diyu
>>>>
>>>>
>>>>> On Dec 2, 2024, at 05:05, Prithwish Tribedy
>>> <ptribedy AT rcf.rhic.bnl.gov> wrote:
>>>>>
>>>>> Hi ShinIchi and all,
>>>>> Thank you for the excellent compilation! Should we consider
>>> moving your v1 talk to Friday? This would allow you to include
>>> both public and STAR internal results, providing more flexibility
>>> to address key issues that support or challenge EM-field
>>> explanations. I list a few points for you to consider on both
>>> support and apparent challenge to EM-field explanations:
>>>>>
>>>>> 1. Proton results change sign with centrality across all
>>> energies -- supports naive EM-field expectations
>>>>> 2. Kaon results follow proton trends but are weaker --
>>> supports EM-field if we assume strange quark behave differently
>>>>> 3. Pion results align with protons/kaons at low energies,
>>> pion-proton-kaon all showing same trend -- challenging
>>> transport-only explanations.
>>>>> 4. Above (#3) may not be the case for 200 GeV, it's unclear
>>> if pion results change sign like protons at 200 GeV -- points to
>>> something is missing in our understanding
>>>>> 5. Net-ΛΛ results are almost on top of protons, despite
>>> Λ's have no electric charge -- challenges naive EM-field
>>> explanation
>>>>> 6. Splitting increases with ΔqΔq, ΔBΔB, and ΔSΔS, if
>>> you assume NCQ scaling holds for produced particles -- supports
>>> both EM-field & has been explained by hydro models with baryon
>>> inhomogeneity
>>>>> 8. NCQ scaling -- crucial but is hard to verify, attempt made
>>> for produced quarks only with limited significance, but there are
>>> proof that it does not hold for mixture of produced & transported
>>> quarks
>>>>> 7. Hydro models explain proton data without EM fields --
>>> challenging EM explanations
>>>>> 8. Hydro models has not demonstrated that they can explain
>>> all PID data -- incompleteness to hydro models that challenge
>>> EM-field explanations
>>>>> 9. Other models such as mean field -- I am not an expert but
>>> it's worth touching.
>>>>>
>>>>> Overall, this is a fascinating topic that deserves lengthy
>>> discussion, so having it as the last talk of the day may not be
>>> ideal.
>>>>>
>>>>> Let me know your thoughts!
>>>>>
>>>>> Best,
>>>>> Prithwish
>>>>>
>>>>>
>>>>> On 2024-12-01 12:40, EsumiShinIchi wrote:
>>>>>> Dear Rich, Subhash, Prithwish and all
>>>>>> I send you the draft of my talk on v1 splitting with materials
>>> that
>>>>>> are already in public,
>>>>>> if you have any suggestions, please let me know. Thank you
>>> very much
>>>>>> in advance.
>>>>>> Best regards, ShinIchi
>>>>>>
>>>
>>
> https://drupal.star.bnl.gov/STAR/system/files/v1split_bes2star_Esumi_2024Dec04.pdf
>>> [1]
>>>>>>> Hi Everyone
>>>>>>> I like Subash’s suggestion
>>>>>>> To be clear it is now
>>>>>>> Sooraj - v1, v2 (and v3?) of light and strange hadrons and
>>>>>>> implications
>>>>>>> Chengdong Han - light and hyper nuclei flow
>>>>>>> Xingrui Gou - Global and local polarization in BES-II COL
>>> (note that
>>>>>>> we intend to make FXT-polarization a separate talk)
>>>>>>> Zhiwan Xu - Chiral effects (CME related) in BES-II and 200GeV
>>>>>>> Shinichi - v1 splitting and possible interpretations
>>>>>>> Pretty good. Hope we can fit it all in. I think at least
>>> Sooraj and
>>>>>>> Shinichi’s talks should be in the open session with the
>>> theorists
>>>>>>> -Rich
>>>>>>>> Dear Sooraj, ShinIchi, Richard and Prithwish,
>>>>>>>> My understanding is that we were looking for candidates
>>> whose
>>>>>>>> talks could present an unbiased perspective on topics such
>>> as the
>>>>>>>> onset of partonic collectivity (bringing together all
>>> viewpoints)
>>>>>>>> and the electromagnetic field (covering both electromagnetic
>>> and
>>>>>>>> non-electromagnetic scenarios). However, we did not reach a
>>>>>>>> consensus on the EM-talk.
>>>>>>>> Therefore, may I suggest having ShinIchi give a summary talk
>>> on
>>>>>>>> the experimental results of v1-splitting from STAR (if
>>> possible
>>>>>>>> and if you agree), followed by a theorist? I would recommend
>>>>>>>> Sandeep Chatterjee to discuss v1 with hydrodynamics. He is
>>> an
>>>>>>>> expert on v1 splitting due to EM (predicted D-meson v1
>>> splitting)
>>>>>>>> and non-electromagnetic scenario with baryon. This talk
>>> could be
>>>>>>>> part of an open session, as most of our v1 results are
>>> public.
>>>>>>>> Although I don't see much space in agenda to accommodate
>>>>>>>> v1-splitting theory speaker, I’m cc’ing ShinIchi here
>>> to get
>>>>>>>> his opinion on this.
>>>>>>>> The followings are rest of the talks from FCV:
>>>>>>>> Sooraj - Summarizing v1, v2 of light and strange hadrons
>>>>>>>> Chengdong Han - light and hyper nuclei flow
>>>>>>>> Xingrui Gou - Global and local polarization in BES-II COL
>>> (note
>>>>>>>> that we intend to make FXT-polarization a separate talk)
>>>>>>>> Zhiwan Xu - Chiral effects (CME related) in BES-II and
>>> 200GeV
>>>>>>>> Thanks and regards,
>>>>>>>> Subhash
>>>>
>>
>> --
>>
>> Sooraj Radhakrishnan
>>
>> Research Scientist,
>> Department of Physics
>>
>> Kent State University
>> Kent, OH 44242
>>
>> Physicist Postdoctoral Affiliate Nuclear Science Division
>> Lawrence Berkeley National Lab
>> MS70R0319, One Cyclotron Road
>> Berkeley, CA 94720
>> Ph: 510-495-2473 [3]
>>
>> Email: skradhakrishnan AT lbl.gov
>
>
>
> Links:
> ------
> [1]
> https://drupal.star.bnl.gov/STAR/system/files/v1split_bes2star_Esumi_2024Dec04.pdf
> [2]
> https://urldefense.com/v3/__https://arxiv.org/pdf/2211.15659__;!!P4SdNyxKAPE!DeQFNclXH4GbLXJ1rhi2DLiNsmhQGY7esZCvfplVqI46p7yGVkd5Gs24ya0Zo28C6fHVy2tmKIvGxXqM6NGBrlu2fk9bTTc5xWNCy4iaRLk$
> [3] tel:%28510%29%20495-2473
Sooraj Radhakrishnan
Research Scientist,
Department of Physics
Kent State University
Kent, OH 44242
Physicist Postdoctoral Affiliate
Lawrence Berkeley National Lab
MS70R0319, One Cyclotron Road
Email: skradhakrishnan AT lbl.gov
-
Re: [[Star-fcv-l] ] v1 v2 talk at the workshop,
EsumiShinIchi, 12/01/2024
-
Re: [[Star-fcv-l] ] v1 v2 talk at the workshop,
Prithwish Tribedy, 12/01/2024
-
Re: [[Star-fcv-l] ] v1 v2 talk at the workshop,
Diyu Shen, 12/01/2024
-
Re: [[Star-fcv-l] ] v1 v2 talk at the workshop,
EsumiShinIchi, 12/01/2024
-
Re: [[Star-fcv-l] ] v1 v2 talk at the workshop,
Sooraj Radhakrishnan, 12/02/2024
-
Re: [[Star-fcv-l] ] v1 v2 talk at the workshop,
EsumiShinIchi, 12/02/2024
-
Re: [[Star-fcv-l] ] v1 v2 talk at the workshop,
subhash, 12/02/2024
- Re: [[Star-fcv-l] ] v1 v2 talk at the workshop, Sooraj Radhakrishnan, 12/02/2024
- Re: [[Star-fcv-l] ] v1 v2 talk at the workshop, EsumiShinIchi, 12/04/2024
-
Re: [[Star-fcv-l] ] v1 v2 talk at the workshop,
subhash, 12/02/2024
-
Re: [[Star-fcv-l] ] v1 v2 talk at the workshop,
EsumiShinIchi, 12/02/2024
-
Re: [[Star-fcv-l] ] v1 v2 talk at the workshop,
Sooraj Radhakrishnan, 12/02/2024
-
Re: [[Star-fcv-l] ] v1 v2 talk at the workshop,
EsumiShinIchi, 12/01/2024
-
Re: [[Star-fcv-l] ] v1 v2 talk at the workshop,
Diyu Shen, 12/01/2024
-
Re: [[Star-fcv-l] ] v1 v2 talk at the workshop,
Prithwish Tribedy, 12/01/2024
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