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.
The Equation of State for Dense QCD and Quark Stars
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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.
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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.