Bjorken initial energy density estimation in Xe-Xe collisions at $\sqrt{s_{NN}} = 5.44$ TeV using ALICE
Mohammad Asif Bhat, Akankshya Nayak, P. K. Sahu

TL;DR
This study estimates the initial energy density in Xe-Xe collisions at 5.44 TeV using the Bjorken formula, comparing different assumptions and with Pb-Pb collisions, to understand quark-gluon plasma formation.
Contribution
It introduces a comparative analysis of initial energy density estimation methods in Xe-Xe collisions and evaluates their consistency with Pb-Pb collision data.
Findings
Energy density varies with centrality and assumptions.
Xe-Xe system size is smaller than Pb-Pb at similar energies.
Case III provides more consistent energy density estimates.
Abstract
The Bjorken initial energy density () has been estimated in different centrality classes in Xe-Xe collisions using Bjorken formula. Three different cases have been considered. In Case I, we have fixed the formation time () and varied the area of overlap region (). In Case II, we have fixed both and and we have varied both and in Case III. We observed that the is first increasing and then decreasing while going from central to peripheral collisions in Case I whereas it is decreasing in Case II and III, as expected. The value for top central and mid central collisions in Case II and for all centrality classes in Case III are greater than 1 , indicating the possibility of QGP medium formation respectively. The results of the Pb-Pb at…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsHigh-Energy Particle Collisions Research · Dust and Plasma Wave Phenomena · Astrophysics and Cosmic Phenomena
