Asymptotic normalization coefficients from ab initio calculations
arXiv:1102.1787 · doi:10.1103/PhysRevC.83.041001
Abstract
We present calculations of asymptotic normalization coefficients (ANCs) for one-nucleon removals from nuclear states of mass numbers 3 to 9. Our ANCs were computed from variational Monte Carlo solutions to the many-body Schroedinger equation with the combined Argonne v18 two-nucleon and Urbana IX three-nucleon potentials. Instead of computing explicit overlap integrals, we applied a Green's function method that is insensitive to the difficulties of constructing and Monte Carlo sampling the long-range tails of the variational wave functions. This method also allows computation of the ANC at the physical separation energy, even when it differs from the separation energy for the Hamiltonian. We compare our results, which for most nuclei are the first ab initio calculations of ANCs, with existing experimental and theoretical results and discuss further possible applications of the technique.
5 pages, 3 figures; minor changes to match published version, and minor additional corrections to Fig. 3
References in corpus (16)
- An accurate nucleon-nucleon potential with charge-independence breaking
- Quantum Monte Carlo Calculations of Nuclei
- Quantum Monte Carlo Calculations of Light Nuclei
- Realistic models of pion-exchange three-nucleon interactions
- Recent developments in no-core shell-model calculations
- Radiative capture of nucleons at astrophysical energies with single-particle states
- Calculation of the Alpha--Particle Ground State within the Hyperspherical Harmonic Basis
- Radiative alpha-capture cross sections from realistic nucleon-nucleon interactions and variational Monte Carlo wave functions
- A relation between proton and neutron asymptotic normalization coefficients for light mirror nuclei and its relevance to nuclear astrophysics
- Asymptotic normalization coefficients for 8B->7Be+p from a study of 8Li->7Li+n
- Six-body calculation of the alpha-deuteron radiative capture cross section
- 7Be(p,gamma)8B S-factor from ab initio no-core shell model wave functions
- Scattering of Be and B and the astrophysical S factor
- The Three-Nucleon System Near the N-d Threshold
- Unitary correlation in nuclear reaction theory
- Determination of the S_18 astrophysical factor for 8B(p,gamma)9C from the breakup of 9C at intermediate energies
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