Quantum Monte Carlo calculations of A=9,10 nuclei
Steven C. Pieper, K. Varga, R. B. Wiringa
Abstract
We report on quantum Monte Carlo calculations of the ground and low-lying excited states of A=9,10 nuclei using realistic Hamiltonians containing the Argonne v18 two-nucleon potential alone or with one of several three-nucleon potentials, including Urbana IX and three of the new Illinois models. The calculations begin with correlated many-body wave functions that have an α-like core and multiple p-shell nucleons, LS-coupled to the appropriate (Jπ;T) quantum numbers for the state of interest. After optimization, these variational trial functions are used as input to a Green's function Monte Carlo calculation of the energy, using a constrained path algorithm. We find that the Hamiltonians that include Illinois three-nucleon potentials reproduce ten states in 9Li, 9Be, 10Be, and 10B with an rms deviation as little as 900 keV. In particular, we obtain the correct 3+ ground state for 10B, whereas the Argonne v18 alone or with Urbana IX predicts a 1+ ground state. In addition, we calculate isovector and isotensor energy differences, electromagnetic moments, and one- and two-body density distributions.
Create a lesson
Related papers
Impact of ab initio E1 strength on neutron capture rates along the nickel isotopic chain
Francesca Bonaiti, Joanna E. Sobczyk
Final-state centrality in relativistic heavy-ion simulations from neural networks
Anibal Bezerra, Fernando G. Gardim
Constrained coupled-cluster computations yield negative-parity rotational bands
Gaute Hagen, Benjamin Bally, Thomas Papenbrock
Levy-shaped femtoscopic sources from an exact solution of relativistic hydrodynamics
Bence Szentkuti, Mate Csanad
Octupole correlations in the excited 0+ states and two-neutron transfers in actinide nuclei
Kosuke Nomura
Macroscopic study of ϕ-mesic nuclei in pp collisions at s = 7 TeV with the PACIAE model
Qiang Wang, Zhi-Lei She, An-Ke Lei et al.