At high baryon chemical potential µB, the equation of state of QCD allows a weak-coupling expansion in the QCD coupling αs. The result is currently known up to and including the full next-to-next-to-leading order (NNLO) α 2 s . Starting at this order, the computations are complicated by the modification of particle propagation in a dense medium, which necessitates non-perturbative treatment of the scale α 1/2 s µB. In this work, we apply a Hard-Thermal-Loop scheme for capturing the contributions of this scale to the weak-coupling expansion, and use it to determine the leadinglogarithm contribution to N 3 LO: α 3 s ln 2 αs. This result is the first improvement to the equation of state of massless cold quark matter in 40 years. The new term is negligibly small, and thus significantly increases our confidence in the applicability of the weak-coupling expansion. arXiv:1807.04120v2 [hep-ph]

We discuss the prospects of performing high-order perturbative calculations in systems characterized by a vanishing temperature but finite density. In particular, we show that the determination of generic Feynman integrals containing fermionic chemical potentials can be reduced to the evaluation of three-dimensional phase space integrals over vacuum on-shell amplitudes - a result reminiscent of a previously proposed "naive real-time formalism" for vacuum diagrams. Applications of these rules are discussed in the context of the thermodynamics of cold and dense QCD, where it is argued that they facilitate an extension of the Equation of State of cold quark matter to higher perturbative orders.Comment: 22 pages, 3 figures; v2: discussion extended and references adde

In 2+1 dimensions, QED becomes exactly solvable for all values of the fermion charge e in the limit of many fermions N f 1. We present results for the free energy density at finite temperature T to next-to-leading-order in large N f . In the naive large N f limit, we uncover an apparently UV-divergent contribution to the vacuum energy at order O( e 6 N 3 f ), which we argue to become a finite contribution of order O(e 6 N 4 f ) when resumming formally higher-order 1/N f contributions. We find the finite-temperature free energy to be well-behaved for all values of the dimensionless coupling e 2 N f /T , and to be bounded by the free energy of N f free fermions and non-interacting QED3, respectively. We invite follow-up studies from finite-temperature lattice gauge theory at large but fixed N f to test our results in the regime e 2 N f /T 1.