QCD phase diagram at high temperature and density
At zero net baryon density, heating turns ordinary nuclear matter into a quark-gluon plasma smoothly, near $1.8 \times 10^{12}\,\mathrm{K}$. At higher densities the change may become abrupt, and mapping where this happens is a central goal of the field.
Why it matters
The phase structure of hot and dense QCD matter fixes the properties of the early universe and of matter in neutron-star mergers.
Review
Bzdak, Esumi, Koch, Liao, Stephanov, Xu, Mapping the phases of quantum chromodynamics with beam energy scan, Physics Reports, 2020. https://arxiv.org/abs/1906.00936 reference checked
Editors' decisions
- Accept of version 2, , on 2026-10-15. Decision record
Timestamp record
- Signed record
- 8cebfc31c6df…
- Public log
- Entry 292, in checkpoint 2,123
- In the log by
- Block 969,698, 2026-10-03
This text was in the PubPhys log by that date. The date says nothing about when the problem was first posed.