Evolution of Nuclear Spectra with Nuclear Forces

Details Evolution of Nuclear Spectra with Nuclear Forces Evolution of Nuclear Spectra with Nuclear Forces

Apr 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aps..apro13001w&link_type=abstract

American Physical Society, April Meeting, Jointly Sponsored with the High Energy Astrophysics Division (HEAD) of the American As

Astronomy and Astrophysics

Astrophysics

Scientific paper

We examine how the features of nuclear spectra evolve as a consequence of the complexity (or completeness) of the forces between individual nucleons. Starting from a Hamiltonian containing the realistic Argonne v18 two-nucleon and Illinois-2 three-nucleon potentials, we construct a series of progressively simpler force models by eliminating various operator components. At each stage, we reproject the remaining operators to preserve the deuteron binding and as much nucleon-nucleon scattering behavior as feasible. We then use these models as input to quantum Monte Carlo calculations of the spectra of light nuclei up to A=10, to see how nuclear spectra evolve as the nuclear forces are made increasingly realistic.

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