Investigation of $\pi$, K, p Production Beyond Mid-Rapidity $\sqrt{s_{NN}}=27$ GeV at STAR
Updated on Thu, 2022-01-20 14:31 by galatyuk. Originally created by bkimel on 2020-10-19 11:24.
Under:
| Author | : | Benjamin Kimelman |
| Meeting | : | 2020 Fall Meeting of the Division of Nuclear Physics of the American Physical Society - New Orleans , LA, Oct. 29 - Nov. 1, 2020 |
| Format | : | talk |
| QCD Type | : | Hot QCD |
| Is selected by STC | : | No |
| File(s) | : |