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

Timestamp record

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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.

4 problems