REVIEW 2 cited by
The Equation of State for Dense QCD and Quark Stars
Not yet reviewed by Pith; the record is open.
This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.
SPECIMEN: schema-true, not a live event
T0 review · schema-true
One-sentence machine reading of the paper's core claim.
pith:XXXXXXXX · record.json · timestamp
read the original abstract
We calculate the equation of state for degenerate quark matter to leading order in hard-dense-loop (HDL) perturbation theory. We solve the Tolman-Oppenheimer-Volkov equations to obtain the mass-radius relation for dense quark stars. Both the perturbative QCD and the HDL equations of state have a large variation with respect to the renormalization scale for quark chemical potential below 1 GeV which leads to large theoretical uncertainties in the quark star mass-radius relation.
Forward citations
Cited by 2 Pith papers
-
Moment of Inertia of an Interacting Bose Gas
For a weakly interacting phi^4 Bose gas, the moment of inertia density is the perpendicular radius squared times the enthalpy density, holding through order lambda^(3/2) including ring-diagram resummation.
-
One-loop HDL thermodynamics of a strongly magnetized isospin asymmetric cold quark matter
In the lowest Landau level, one-loop HDLpt pressure of cold quark matter grows with quark and isospin chemical potentials, and the magnetization is positive, making transverse pressure smaller than longitudinal.
Discussion (0). Continue with ORCID to comment.