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- W3103795666 abstract "We report a quantum Monte Carlo calculation of the equation of state of symmetric nuclear matter using local interactions derived from chiral effective field theory up to next-to-next-to-leading order fit to few-body observables only. The empirical saturation density and energy are well reproduced within statistical and systematic uncertainties. We have also derived the symmetry energy as a function of the density, finding good agreement with available experimentally derived constraints at saturation and twice saturation density. We find that the corresponding pressure is also in excellent agreement with recent constraints extracted from gravitational waves of the neutron-star merger GW170817 by the LIGO-Virgo detection." @default.
- W3103795666 created "2020-11-23" @default.
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- W3103795666 date "2020-05-07" @default.
- W3103795666 modified "2023-10-18" @default.
- W3103795666 title "Nuclear and neutron-star matter from local chiral interactions" @default.
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- W3103795666 doi "https://doi.org/10.1103/physrevresearch.2.022033" @default.
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