Solution of large scale nuclear structure problems by wave function factorization
arXiv:nucl-th/0308027 · doi:10.1103/PhysRevC.69.024312
Abstract
Low-lying shell model states may be approximated accurately by a sum over products of proton and neutron states. The optimal factors are determined by a variational principle and result from the solution of rather low-dimensional eigenvalue problems. Application of this method to sd-shell nuclei, pf-shell nuclei, and to no-core shell model problems shows that very accurate approximations to the exact solutions may be obtained. Their energies, quantum numbers and overlaps with exact eigenstates converge exponentially fast as the number of retained factors is increased.
12 pages, 12 figures (from 15 eps files) included
References in corpus (29)
- Thermodynamic limit of the density matrix renormalization for the spin-1 Heisenberg chain
- Quantum Monte Carlo Calculations of Nuclei
- Quantum Monte Carlo Calculations of Light Nuclei
- Properties of C in the {\it ab initio} nuclear shell-model
- A class of ansatz wave functions for 1D spin systems and their relation to DMRG
- Effective interaction for pf-shell nuclei
- Quantum Monte Carlo calculations of nuclei
- Density-Matrix Spectra of Solvable Fermionic Systems
- A Full Shell Model Study of a~=~48 Nuclei
- Monte Carlo evaluation of path integrals for the nuclear shell model
- Accurate Nucleon-Nucleon Potential Based upon Chiral Perturbation Theory
- Full shell model calculation of the binding energies of the nuclei
- Density-matrix spectra for integrable models
- On Density-Matrix Spectra for Two-Dimensional Quantum Systems
- Density Matrices for a Chain of Oscillators
- Ground state correlations and mean-field in O
- Chaotic wave functions and exponential convergence of low-lying energy eigenvalues
- Shell Model Monte Carlo studies of neutron-rich nuclei in the 1s-0d-1p-0f shells
- Universal Asymptotic Eigenvalue Distribution of Density Matrices and the Corner Transfer Matrices in the Thermodynamic Limit
- Truncation Method for the Shell Model Calculation
- The Density Matrix Renormalization Group Method and Large-Scale Nuclear Shell-Model Calculations
- An extrapolation method for shell model calculations
- Factorization of shell-model ground-states
- An importance sampling algorithm for generating exact eigenstates of the nuclear Hamiltonian
- Quasi-SU(3) truncation scheme for even-even sd-shell nuclei
- Precise estimation of shell model energy by second order extrapolation method
- A New Approach to Large-Scale Nuclear Structure Calculations
- SU(3) symmetry breaking in lower fp-shell nuclei
- A mixed-mode shell-model theory for nuclear structure studies
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- Double Beta Decay
- Factorization in large-scale many-body calculations
- Ab initio coupled-cluster theory for open-shell nuclei
- Proton-neutron entanglement in the nuclear shell model
- Nuclear Forces for Precision Nuclear Physics -- a collection of perspectives
- Quantum Simulations in Effective Model Spaces (I): Hamiltonian Learning-VQE using Digital Quantum Computers and Application to the Lipkin-Meshkov-Glick Model
- BIGSTICK: A flexible configuration-interaction shell-model code (updated)
- Density matrix renormalization group and wave function factorization for nuclei
- Multi-Body Entanglement and Information Rearrangement in Nuclear Many-Body Systems
- Quantum Magic and Multi-Partite Entanglement in the Structure of Nuclei
- Weak entanglement approximation for nuclear structure
- Quantum Complexity Fluctuations from Nuclear and Hypernuclear Forces
- Extrapolation method in shell model calculations with deformed basis
- New variational Monte Carlo method with an energy variance extrapolation for large-scale shell-model calculations
- Lowest eigenvalue of the nuclear shell model Hamiltonian
- A Problem in the Statistical Description of Beta-Delayed Neutron Emission
- Practical recipes for the model order reduction, dynamical simulation, and compressive sampling of large-scale open quantum systems
- Broken Pair Model: A viable Alterative to the Shell Model for Odd-Spherical Nuclei