Equation of State

Equation of state at neutron-star densities and beyond from perturbative QCD
Equation of state at neutron-star densities and beyond from perturbative QCD

We show that equations of state that are extremely stiff within the cores of maximally massive neutron stars are incompatible with the behavior of the speed of sound at high densities 25-40$n_\mathrm{sat}$

Dec 21, 2023

Quark matter and nuclear astrophysics: Recent developments
Quark matter and nuclear astrophysics: Recent developments

Proceedings from Quark Matter 2023 summarizing my recent work (as well as a few others') on quark matter and nuclear astrophysics.

Dec 15, 2023

Bounding the QCD Equation of State with the Lattice
Bounding the QCD Equation of State with the Lattice

We show that the pressure of phase-quenched QCD -- a theory that is simpler to compute on the lattice -- agrees with the pressure of true QCD up to next-to-next-to-next to leading order, where it differes in only one part of one diagram (pictured).

Sep 26, 2023

Equation of State of Cold Quark Matter to $O(\alpha_s^3 \ln \alpha_s)$
Equation of State of Cold Quark Matter to $O(\alpha_s^3 \ln \alpha_s)$

We calculate the state-of-the-art pressure of cold and dense deconfined matter by accounting for the physics from all of the long-wavelength, dynamically screened gluons at next-to-next-to-next-to-leading order.

Jul 17, 2023

Lectures on Perturbative QCD at finite temperature and density
Lectures on Perturbative QCD at finite temperature and density

Jun 10, 2023

3 Lectures on Neutron stars and their equation of state
3 Lectures on Neutron stars and their equation of state

May 15, 2022

Lectures on Perturbative QCD at high densities
Lectures on Perturbative QCD at high densities

A two-hour lecture on the basics of in-medium field theory as applied to cold quark matter at high densities.

Nov 17, 2021

Youtube interview with the Cosmic Companion
Youtube interview with the Cosmic Companion

An interview about my Nature Physics paper, providing compelling evidence for the existence of deconfined cold quark matter in the cores of the most massive neutron stars in the universe.

Jun 23, 2020