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star-hp-l - Re: [Star-hp-l] STAR presentation by Sooraj Radhakrishnan for AUM 2022 submitted for review

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Subject: STAR HardProbes PWG

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  • From: Sooraj Radhakrishnan <skradhakrishnan AT lbl.gov>
  • To: Barbara Trzeciak <barbara.trzeciak AT gmail.com>
  • Cc: STAR HardProbes PWG <star-hp-l AT lists.bnl.gov>, webmaster <webmaster AT star.bnl.gov>
  • Subject: Re: [Star-hp-l] STAR presentation by Sooraj Radhakrishnan for AUM 2022 submitted for review
  • Date: Mon, 6 Jun 2022 10:58:07 +0530

Dear Barbara,
   Thanks for the sign off and the helpful comments.I have updated the slides with yours and Nihar's suggestions. Please find at the same page. Please find some responses below

//s4: CSM) -> (CSM). And please add the reference for this:  Jean-Philippe Lansberg, Physics Reports, 889, 1 (2020)
s5: CNM - you use this abbreviation for the first time. You can spell it out here, or on slide 2 change: Impact of cold nuclear matter on quarkonia production -> Impact of cold nuclear matter (CNM) effects
 on quarkonia production //
------- Done

//s8: of deconfined charm quarks - I would add here thermalized or partially thermalized//
------- Even for v2, its argued a few collisions suffice. So I am not sure if we should say thermalization as a prerequisite here 

//s9: D0 production suppressed -> D0 and D+/- production suppressed
s17: with good precision in with -> with good precision with//
------- Done

thanks
Sooraj

On Fri, Jun 3, 2022 at 2:54 PM Barbara Trzeciak <barbara.trzeciak AT gmail.com> wrote:
Hi Sooraj,
nice slides. 
I have a few minor comments and sign off.

Cheers,
Barbara

s4: CSM) -> (CSM). And please add the reference for this:  Jean-Philippe Lansberg, Physics Reports, 889, 1 (2020)
s5: CNM - you use this abbreviation for the first time. You can spell it out here, or on slide 2 change: Impact of cold nuclear matter on quarkonia production -> Impact of cold nuclear matter (CNM) effects
 on quarkonia production 
s8: of deconfined charm quarks - I would add here thermalized or partially thermalized
s9: D0 production suppressed -> D0 and D+/- production suppressed
s17: with good precision in with -> with good precision with

On Thu, Jun 2, 2022 at 8:22 PM Sooraj Radhakrishnan via Star-hp-l <star-hp-l AT lists.bnl.gov> wrote:
Dear All,
   I was invited to give a talk on 'The STAR Results and Perspective' at the HF+Jet session for the RHIC AGS AUM. Sorry for the late submission. Please let me know if you have any comments or suggestions

thanks
Sooraj

On Thu, Jun 2, 2022 at 11:47 PM webmaster--- via Star-hp-l <star-hp-l AT lists.bnl.gov> wrote:
Dear Star-hp-l AT lists.bnl.gov members,

Sooraj Radhakrishnan (skradhakrishnan AT lbl.gov) has submitted a material for a 
review, please have a look:
https://drupal.star.bnl.gov/STAR/node/59836

---
If you have any problems with the review process, please contact 
webmaster AT www.star.bnl.gov
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--
Sooraj Radhakrishnan
Research Scientist,
Department of Physics
Kent State University
Kent, OH 44243

Physicist Postdoctoral Affiliate
Nuclear Science Division
Lawrence Berkeley National Lab
MS70R0319, One Cyclotron Road
Berkeley, CA 94720
Ph: 510-495-2473
_______________________________________________
Star-hp-l mailing list
Star-hp-l AT lists.bnl.gov
https://lists.bnl.gov/mailman/listinfo/star-hp-l


--
Sooraj Radhakrishnan
Research Scientist,
Department of Physics
Kent State University
Kent, OH 44243

Physicist Postdoctoral Affiliate
Nuclear Science Division
Lawrence Berkeley National Lab
MS70R0319, One Cyclotron Road
Berkeley, CA 94720
Ph: 510-495-2473



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