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Neutron stars and the nuclear equation of state
We review the current status and recent progress of microscopic many-body approaches
and phenomenological models, which are employed to construct the equation of state of …
and phenomenological models, which are employed to construct the equation of state of …
Three-nucleon forces: Implementation and applications to atomic nuclei and dense matter
K Hebeler - Physics Reports, 2021 - Elsevier
Recent advances in nuclear structure theory have significantly enlarged the accessible part
of the nuclear landscape via ab initio many-body calculations. These developments open …
of the nuclear landscape via ab initio many-body calculations. These developments open …
How well do we know the neutron-matter equation of state at the densities inside neutron stars? A Bayesian approach with correlated uncertainties
We introduce a new framework for quantifying correlated uncertainties of the infinite-matter
equation of state derived from chiral effective field theory (χ EFT). Bayesian machine …
equation of state derived from chiral effective field theory (χ EFT). Bayesian machine …
High-quality two-nucleon potentials up to fifth order of the chiral expansion
We present NN potentials through five orders of chiral effective field theory ranging from
leading order (LO) to next-to-next-to-next-to-next-to-leading order (N 4 LO). The construction …
leading order (LO) to next-to-next-to-next-to-next-to-leading order (N 4 LO). The construction …
Accurate nuclear radii and binding energies from a chiral interaction
With the goal of develo** predictive ab initio capability for light and medium-mass nuclei,
two-nucleon and three-nucleon forces from chiral effective field theory are optimized …
two-nucleon and three-nucleon forces from chiral effective field theory are optimized …
Chiral interactions up to next-to-next-to-next-to-leading order and nuclear saturation
We present an efficient Monte Carlo framework for perturbative calculations of infinite
nuclear matter based on chiral two-, three-, and four-nucleon interactions. The method …
nuclear matter based on chiral two-, three-, and four-nucleon interactions. The method …
Limiting masses and radii of neutron stars and their implications
We combine the equation of state of dense matter up to twice nuclear saturation density n
sat obtained using chiral effective field theory (χ EFT) and recent observations of neutron …
sat obtained using chiral effective field theory (χ EFT) and recent observations of neutron …
Neutron star tidal deformabilities constrained by nuclear theory and experiment
We confront observational data from gravitational wave event GW170817 with microscopic
modeling of the cold neutron star equation of state. We develop and employ a Bayesian …
modeling of the cold neutron star equation of state. We develop and employ a Bayesian …
Saturation with chiral interactions and consequences for finite nuclei
We explore the impact of nuclear matter saturation on the properties and systematics of finite
nuclei across the nuclear chart. By using the ab initio in-medium similarity renormalization …
nuclei across the nuclear chart. By using the ab initio in-medium similarity renormalization …
Quantifying uncertainties and correlations in the nuclear-matter equation of state
We perform statistically rigorous uncertainty quantification (UQ) for chiral effective field
theory (χ EFT) applied to infinite nuclear matter up to twice nuclear saturation density. The …
theory (χ EFT) applied to infinite nuclear matter up to twice nuclear saturation density. The …