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QCD in the cores of neutron stars

I discuss why state-of-the art perturbative QCD calculations of the equation of state at large chemical potential that are reliable at asymptotically high densities constrain the same equation of state at neutron-star densities. I describe how these theoretical calculations affect the EOS at lower density. I argue that the ab-initio calculations in QCD offer significant information about the equation of state of the neutron-star matter, which is complementary to the current astrophysical observations.

preprint2022arXivOpen access
Oleg Komoltsev
hep-phastro-ph.HEnucl-th
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Oleg Komoltsev

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