A parametric low-rank update to the Hamiltonian reduces the A-body problem exactly to a low-dimensional matrix equation at fixed energy.
R., Machleidt, R., & Nosyk, Y
3 Pith papers cite this work, alongside 346 external citations. Polarity classification is still indexing.
3
Pith papers citing it
346
external citations · OpenAlex
citation-role summary
background 1
method 1
citation-polarity summary
fields
nucl-th 3years
2026 3representative citing papers
NCSMC enables ab initio predictions of structure, resonances, and reactions in halo nuclei such as 6He, 8B, 11Be, and 15C from chiral interactions alone.
Multi-messenger observations of neutron stars imply L=42.6–52 MeV (piecewise polytrope) or 44.2–56.7 MeV (speed-of-sound) at 68% credibility, and show pQCD constraints barely change the posterior EOS.
citing papers explorer
-
Exact emulation of few-body systems at low cost
A parametric low-rank update to the Hamiltonian reduces the A-body problem exactly to a low-dimensional matrix equation at fixed energy.
-
Halo Nuclei from Ab Initio Nuclear Theory
NCSMC enables ab initio predictions of structure, resonances, and reactions in halo nuclei such as 6He, 8B, 11Be, and 15C from chiral interactions alone.
-
Astrophysics equation of state inference with Bayesian chiral effective field theory uncertainties
Multi-messenger observations of neutron stars imply L=42.6–52 MeV (piecewise polytrope) or 44.2–56.7 MeV (speed-of-sound) at 68% credibility, and show pQCD constraints barely change the posterior EOS.