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Re: [Star-fcv-l] STAR presentation by Yicheng Feng for QPT 2023 submitted for review
- From: "Feng, Yicheng" <feng216 AT purdue.edu>
- To: "STAR Flow, Chirality and Vorticity PWG" <star-fcv-l AT lists.bnl.gov>
- Subject: Re: [Star-fcv-l] STAR presentation by Yicheng Feng for QPT 2023 submitted for review
- Date: Fri, 22 Sep 2023 13:35:43 +0000
Hi Subhash,
Thank you for your comments.
I have followed them and modified the abstract accordingly,
which has been uploaded to the same drupal node:
To identify the changes, a latexdiff file is attached to this email.
Sincerely,
Yicheng
From: Star-fcv-l <star-fcv-l-bounces AT lists.bnl.gov> on behalf of subhash via Star-fcv-l <star-fcv-l AT lists.bnl.gov>
Sent: Thursday, September 21, 2023 9:52 PM
To: STAR Flow, Chirality and Vorticity PWG <star-fcv-l AT lists.bnl.gov>
Cc: subhash <subhash AT rcf.rhic.bnl.gov>
Subject: Re: [Star-fcv-l] STAR presentation by Yicheng Feng for QPT 2023 submitted for review
Sent: Thursday, September 21, 2023 9:52 PM
To: STAR Flow, Chirality and Vorticity PWG <star-fcv-l AT lists.bnl.gov>
Cc: subhash <subhash AT rcf.rhic.bnl.gov>
Subject: Re: [Star-fcv-l] STAR presentation by Yicheng Feng for QPT 2023 submitted for review
---- External Email: Use caution with attachments, links, or sharing data ----
Dear Yicheng,
Nice abstract. I sign off with the following wording suggestions for
your consideration:
l#11-13: "The background baseline for the isobar ratio Y =
(∆γ/v2)Ru(∆γ/v2)Zr is naively expected to be (1/N)Ru(1/N)Zr, however,
genuine two- and three-particle correlations are expected to alter it."
--> The background baseline of the isobar ratio Y (=(∆γ/v2)Ru /
(∆γ/v2)Zr) is naively anticipated to be (1/N)Ru / (1/N)Zr. However,
genuine two- and three-particle correlations have the potential to alter
this baseline.
l#13-15: "We estimate the contributions from those correlations to Y ,
utilizing the STAR isobar data as well as HIJING simulations. Including
those contributions, we arrive at a final background baseline for Y."
--> We calculate the influence of these correlations on Y by
incorporating data from STAR isobar experiments and HIJING simulations.
By accounting for these contributions, we establish a comprehensive
background reference for Y.
Thanks and regards,
Subhash
On 2023-09-20 09:20 PM, webmaster--- via Star-fcv-l wrote:
> Dear star-fcv-l AT lists.bnl.gov members,
>
> Yicheng Feng (feng216 AT purdue.edu) has submitted a material for a
> review,
> please have a look:
> https://nam04.safelinks.protection.outlook.com/?url="https%3A%2F%2Fdrupal.star.bnl.gov%2FSTAR%2Fnode%2F65199&data=05%7C01%7Cfeng216%40purdue.edu%7Ca998701fce9b4d0c697c08dbbb0ea5ac%7C4130bd397c53419cb1e58758d6d63f21%7C0%7C0%7C638309443829473867%7CUnknown%7CTWFpbGZsb3d8eyJWIjoiMC4wLjAwMDAiLCJQIjoiV2luMzIiLCJBTiI6Ik1haWwiLCJXVCI6Mn0%3D%7C3000%7C%7C%7C&sdata=p8Dm1Pmnzpo6%2FZ7jxzFXaTwFyKrGSa1C0KetoKkYn8Y%3D&reserved=0
>
> Deadline: 2023-10-10
> ---
> If you have any problems with the review process, please contact
> webmaster@https://nam04.safelinks.protection.outlook.com/?url="http%3A%2F%2Fwww.star.bnl.gov%2F&data=05%7C01%7Cfeng216%40purdue.edu%7Ca998701fce9b4d0c697c08dbbb0ea5ac%7C4130bd397c53419cb1e58758d6d63f21%7C0%7C0%7C638309443829473867%7CUnknown%7CTWFpbGZsb3d8eyJWIjoiMC4wLjAwMDAiLCJQIjoiV2luMzIiLCJBTiI6Ik1haWwiLCJXVCI6Mn0%3D%7C3000%7C%7C%7C&sdata=4eImW8WQj0ds08Csig84g9YyJuLvHLZPGCV0k8ybcZ8%3D&reserved=0
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Dear Yicheng,
Nice abstract. I sign off with the following wording suggestions for
your consideration:
l#11-13: "The background baseline for the isobar ratio Y =
(∆γ/v2)Ru(∆γ/v2)Zr is naively expected to be (1/N)Ru(1/N)Zr, however,
genuine two- and three-particle correlations are expected to alter it."
--> The background baseline of the isobar ratio Y (=(∆γ/v2)Ru /
(∆γ/v2)Zr) is naively anticipated to be (1/N)Ru / (1/N)Zr. However,
genuine two- and three-particle correlations have the potential to alter
this baseline.
l#13-15: "We estimate the contributions from those correlations to Y ,
utilizing the STAR isobar data as well as HIJING simulations. Including
those contributions, we arrive at a final background baseline for Y."
--> We calculate the influence of these correlations on Y by
incorporating data from STAR isobar experiments and HIJING simulations.
By accounting for these contributions, we establish a comprehensive
background reference for Y.
Thanks and regards,
Subhash
On 2023-09-20 09:20 PM, webmaster--- via Star-fcv-l wrote:
> Dear star-fcv-l AT lists.bnl.gov members,
>
> Yicheng Feng (feng216 AT purdue.edu) has submitted a material for a
> review,
> please have a look:
> https://nam04.safelinks.protection.outlook.com/?url="https%3A%2F%2Fdrupal.star.bnl.gov%2FSTAR%2Fnode%2F65199&data=05%7C01%7Cfeng216%40purdue.edu%7Ca998701fce9b4d0c697c08dbbb0ea5ac%7C4130bd397c53419cb1e58758d6d63f21%7C0%7C0%7C638309443829473867%7CUnknown%7CTWFpbGZsb3d8eyJWIjoiMC4wLjAwMDAiLCJQIjoiV2luMzIiLCJBTiI6Ik1haWwiLCJXVCI6Mn0%3D%7C3000%7C%7C%7C&sdata=p8Dm1Pmnzpo6%2FZ7jxzFXaTwFyKrGSa1C0KetoKkYn8Y%3D&reserved=0
>
> Deadline: 2023-10-10
> ---
> If you have any problems with the review process, please contact
> webmaster@https://nam04.safelinks.protection.outlook.com/?url="http%3A%2F%2Fwww.star.bnl.gov%2F&data=05%7C01%7Cfeng216%40purdue.edu%7Ca998701fce9b4d0c697c08dbbb0ea5ac%7C4130bd397c53419cb1e58758d6d63f21%7C0%7C0%7C638309443829473867%7CUnknown%7CTWFpbGZsb3d8eyJWIjoiMC4wLjAwMDAiLCJQIjoiV2luMzIiLCJBTiI6Ik1haWwiLCJXVCI6Mn0%3D%7C3000%7C%7C%7C&sdata=4eImW8WQj0ds08Csig84g9YyJuLvHLZPGCV0k8ybcZ8%3D&reserved=0
> _______________________________________________
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Attachment:
diff_QPT2023Abs_IsobarNfBkg_v1v2.pdf
Description: diff_QPT2023Abs_IsobarNfBkg_v1v2.pdf
-
[Star-fcv-l] STAR presentation by Yicheng Feng for QPT 2023 submitted for review,
webmaster, 09/20/2023
-
Re: [Star-fcv-l] STAR presentation by Yicheng Feng for QPT 2023 submitted for review,
subhash, 09/21/2023
- Re: [Star-fcv-l] STAR presentation by Yicheng Feng for QPT 2023 submitted for review, Feng, Yicheng, 09/22/2023
-
Re: [Star-fcv-l] STAR presentation by Yicheng Feng for QPT 2023 submitted for review,
subhash, 09/21/2023
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