Skip to Content.
Sympa Menu

star-fcv-l - [[Star-fcv-l] ] STAR presentation by Sharang Rav Sharma for Quark Matter 2025 got commented by Prithwish Tribedy

star-fcv-l AT lists.bnl.gov

Subject: STAR Flow, Chirality and Vorticity PWG

List archive

Chronological Thread  
  • From: webmaster AT star.bnl.gov
  • To: star-fcv-l AT lists.bnl.gov
  • Subject: [[Star-fcv-l] ] STAR presentation by Sharang Rav Sharma for Quark Matter 2025 got commented by Prithwish Tribedy
  • Date: Wed, 13 Nov 2024 18:17:38 -0500

Dear star-fcv-l AT lists.bnl.gov members,

Prithwish Tribedy ( ptribedy AT bnl.gov ) has commented on a material originally

submitted by Sharang Rav Sharma ( sharang.rav AT students.iisertirupati.ac.in )
at
https://drupal.star.bnl.gov/STAR/presentations/Quark-Matter-2025/Anisotropic-flow-correlated-first-order-and-higher-order-event-plane

Comment:
Nice abstract!! I sign off with minor comments, please consider them in the
next version.
It's not clear what this line means: "At the lowest energies, collision
timescales become comparable to those of flow development, enabling the study

of effects such as spectator shadowing."
Do you mean "At the lowest energies, due to passing time of two ions,
collision timescales become comparable...." ?

"This trend has been suggested as a signature of the phase transition" -->
"This trend has been suggested as a POSSIBLE signature of the phase
transition"

"normal nuclear matter" --> "hadronic nuclear matter" (not sure ??)



---
If you have any problems with the review process, please contact
webmaster AT www.star.bnl.gov



Archive powered by MHonArc 2.6.24.

Top of Page