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
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NCSMC enables ab initio predictions of structure, resonances, and reactions in halo nuclei such as 6He, 8B, 11Be, and 15C from chiral interactions alone.
Bayesian EOS inference with χEFT uncertainty priors and LIGO/NICER data yields posteriors consistent with prior work, a stiffening above 3n0, negligible pQCD impact, and an inferred symmetry-energy slope L of 42.6-56.7 MeV.
citing papers explorer
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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.
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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.
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Astrophysics equation of state inference with Bayesian chiral effective field theory uncertainties
Bayesian EOS inference with χEFT uncertainty priors and LIGO/NICER data yields posteriors consistent with prior work, a stiffening above 3n0, negligible pQCD impact, and an inferred symmetry-energy slope L of 42.6-56.7 MeV.