activity
20062026
most citedEquation of state and neutron star properties constrained by nuclear physics and observation

764 citations · 9.4k across the 83 of their papers we have counts for

collaborators
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5 papers · 1 filter

nucl-th2024★ 25 cited

Improved structure of calcium isotopes from ab initio calculations

M. Heinz, T. Miyagi, S. R. Stroberg +3

The in-medium similarity renormalization group (IMSRG) is a powerful and flexible many-body method to compute the structure of nuclei starting from nuclear forces. Recent developme…

nucl-th2024★ 13 cited

Neutron matter from local chiral effective field theory interactions at large cutoffs

I. Tews, R. Somasundaram, D. Lonardoni +6

Neutron matter is an important many-body system that provides valuable constraints for the equation of state (EOS) of neutron stars. Neutron-matter calculations employing chiral ef…

astro-ph.HE2024★ 91 cited

Constraining the dense matter equation of state with new NICER mass-radius measurements and new chiral effective field theory inputs

Nathan Rutherford, Melissa Mendes, Isak Svensson +12

Pulse profile modeling of X-ray data from NICER is now enabling precision inference of neutron star mass and radius. Combined with nuclear physics constraints from chiral effective…

nucl-th2024★ 7 cited

Neutron star matter as a dilute solution of protons in neutrons

J. Keller, K. Hebeler, C. J. Pethick +1

Neutron stars contain neutron-rich matter with around 5% protons at nuclear saturation density. In this Letter, we consider equilibrium between bulk phases of matter based on asymm…

nucl-th2024★ 2 cited

Neutron-rich nuclei and neutron skins from chiral low-resolution interactions

P. Arthuis, K. Hebeler, A. Schwenk

Neutron-rich nuclei provide important insights to nuclear forces and to the nuclear equation of state. Advances in ab initio methods combined with new opportunities with rare isoto…