activity
20102025
most citedEquation of state and neutron star properties constrained by nuclear physics and observation

764 citations · 1.6k across the 10 of their papers we have counts for

collaborators

10 papers

nucl-th2025★ 1 cited

Neutron star crust and outer core equation of state from chiral effective field theory with quantified uncertainties

H. Göttling, L. Hoff, K. Hebeler +1

We study the order-by-order expansion of the energy per particle of asymmetric nuclear matter up to twice saturation density in chiral effective field theory (EFT) within a Bayesia…

nucl-th2024

Multicomponent Fermi systems at low densities

C. J. Pethick, A. Schwenk

We calculate, to second order in the scattering length between two fermions, the Landau quasiparticle interaction for a low-density mixture of two fermion species with unequal dens…

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…

nucl-th2023★ 40 cited

Impact of two-body currents on magnetic dipole moments of nuclei

T. Miyagi, X. Cao, R. Seutin +5

We investigate the effects of two-body currents on magnetic dipole moments of medium-mass and heavy nuclei using the valence-space in-medium similarity renormalization group with c…

nucl-th2017★ 341 cited

Chiral interactions up to next-to-next-to-next-to-leading order and nuclear saturation

C. Drischler, K. Hebeler, A. Schwenk

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 enabl…

nucl-th2014★ 6 cited

Pairing and superfluidity of nucleons in neutron stars

A. Gezerlis, C. J. Pethick, A. Schwenk

We survey the current status of understanding of pairing and superfluidity of neutrons and protons in neutron stars from a theoretical perspective, with emphasis on basic physical…

astro-ph.SR2013★ 764 cited

Equation of state and neutron star properties constrained by nuclear physics and observation

K. Hebeler, J. M. Lattimer, C. J. Pethick +1

Microscopic calculations of neutron matter based on nuclear interactions derived from chiral effective field theory, combined with the recent observation of a 1.97 +- 0.04 M_sun ne…

astro-ph.HE2011★ 38 cited

Neutrino processes in partially degenerate neutron matter

S. Bacca, K. Hally, M. Liebendörfer +3

We investigate neutrino processes for conditions reached in simulations of core-collapse supernovae. Where neutrino-matter interactions play an important role, matter is partially…

nucl-th2010★ 376 cited

Constraints on neutron star radii based on chiral effective field theory interactions

K. Hebeler, J. M. Lattimer, C. J. Pethick +1

We show that microscopic calculations based on chiral effective field theory interactions constrain the properties of neutron-rich matter below nuclear densities to a much higher d…