Bayesian uncertainty quantification of perturbative QCD input to the neutron-star equation of state
Bayesian uncertainty quantification of perturbative QCD input to the neutron-star equation of state
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Berlin/Heidelberg: Springer Berlin Heidelberg
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English
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Berlin/Heidelberg: Springer Berlin Heidelberg
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bstract
The equation of state of neutron-star cores can be constrained by requiring a consistent connection to the perturbative Quantum Chromodynamics (QCD) calculations at high densities. The constraining power of the QCD input depends on uncertainties from missing higher-order terms, the choice of the unphysical renormalization scale, and...
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Bayesian uncertainty quantification of perturbative QCD input to the neutron-star equation of state
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TN_cdi_doaj_primary_oai_doaj_org_article_2dcf121c97a24c71b9cafa7a55db5b79
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_doaj_primary_oai_doaj_org_article_2dcf121c97a24c71b9cafa7a55db5b79
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ISSN
1029-8479
E-ISSN
1029-8479
DOI
10.1007/JHEP06(2023)002
