Thermodynamics of Deconfined Matter at Finite Chemical Potential in a Quasiparticle Description
A. Peshier, B. Kampfer, G. Soff

TL;DR
This paper extends a quasiparticle model of deconfined matter's thermodynamics to finite chemical potential, aligning with lattice data and perturbative limits, and explores implications for dense matter in compact stars.
Contribution
It generalizes an effective quasiparticle model to include finite chemical potential, bridging lattice data and perturbative theory for deconfined matter.
Findings
Extended lattice equation of state to finite baryon density
Analyzed implications for cold, charge-neutral matter in stars
Provided a consistent thermodynamic framework at finite chemical potential
Abstract
An effective quasiparticle description of the thermodynamics of deconfined matter, compatible with both finite-temperature lattice data and the perturbative limit, is generalized to finite chemical potential. Within this approach, the available 4-flavor lattice equation of state is extended to finite baryon density, and implications for cold, charge-neutral deconfined matter in beta-equilibrium in compact stars are considered.
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
TopicsStellar, planetary, and galactic studies · Pulsars and Gravitational Waves Research · Astrophysics and Star Formation Studies
