A Bayesian 2D Gaussian process trained on chiral EFT many-body perturbation theory results yields neutron-star crust and outer-core equations of state with quantified EFT uncertainties up to N3LO.
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Computes quasiradial frequencies of rotating neutron and hybrid stars in slow-rotation limit and identifies distinct spin-down behavior between the two classes using BHF, RMF, and Dyson-Schwinger EOS models.
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Neutron star crust and outer core equation of state from chiral effective field theory with quantified uncertainties
A Bayesian 2D Gaussian process trained on chiral EFT many-body perturbation theory results yields neutron-star crust and outer-core equations of state with quantified EFT uncertainties up to N3LO.
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Quasiradial oscillations of rotating hybrid neutron stars
Computes quasiradial frequencies of rotating neutron and hybrid stars in slow-rotation limit and identifies distinct spin-down behavior between the two classes using BHF, RMF, and Dyson-Schwinger EOS models.