From nucleons to nuclei to fusion reactions
arXiv:1203.0268 · doi:10.1088/1742-6596/402/1/012037
Abstract
Nuclei are prototypes of many-body open quantum systems. Complex aggregates of protons and neutrons that interact through forces arising from quantum chromo-dynamics, nuclei exhibit both bound and unbound states, which can be strongly coupled. In this respect, one of the major challenges for computational nuclear physics, is to provide a unified description of structural and reaction properties of nuclei that is based on the fundamental underlying physics: the constituent nucleons and the realistic interactions among them. This requires a combination of innovative theoretical approaches and high-performance computing. In this contribution, we present one of such promising techniques, the ab initio no-core shell model/resonating-group method, and discuss applications to light nuclei scattering and fusion reactions that power stars and Earth-base fusion facilities.
arXiv comment17 pages, 13 figures, Contribution submitted to the Proceedings of the Conference on Computational Physics 2011 (CCP2011)
References in corpus (34)
- Accurate Charge-Dependent Nucleon-Nucleon Potential at Fourth Order of Chiral Perturbation Theory
- Solar fusion cross sections II: the pp chain and CNO cycles
- Solar Fusion Cross Sections
- Properties of C in the {\it ab initio} nuclear shell-model
- Similarity Renormalization Group for Nucleon-Nucleon Interactions
- The R-matrix theory
- Gamow Shell Model Description of Neutron-Rich Nuclei
- Few-nucleon systems in translationally invariant harmonic oscillator basis
- Ab Initio Many-Body Calculations of n-3H, n-4He, p-{3,4}He, and n-10Be Scattering
- Evolution of Nuclear Many-Body Forces with the Similarity Renormalization Group
- Quantum Monte Carlo calculations of neutron-alpha scattering
- Importance Truncation for Large-Scale Configuration Interaction Approaches
- Ab initio many-body calculations of nucleon-nucleus scattering
- Two-Particle Resonant States in a Many-Body Mean Field
- Gamow Shell Model Description of Weakly Bound Nuclei and Unbound Nuclear States
- Continuum Shell Model
- Ab initio many-body calculation of the 7Be(p,gamma)8B radiative capture
- Ab initio many-body calculations of the 3H(d,n)4He and 3He(d,p)4He fusion
- Precise measurement of the ^7Be(p,gamma)^8B S-factor
- Evolving Nuclear Many-Body Forces with the Similarity Renormalization Group
- Ab initio many-body calculations of nucleon scattering on 4He, 7Li, 7Be, 12C and 16O
- Large basis ab initio shell model investigation of 9-Be and 11-Be
- Study of the and capture reactions using the shell model embedded in the continuum
- Coulomb dissociation of 8B and the low-energy cross section of the 7Be(p,gamma)8B solar fusion reaction
- Theory of the two-proton radioactivity in the continuum shell model
- Ab initio many-body calculations of deuteron-4He scattering and 6Li states
- Shell-model calculations for the three-nucleon system
- Unitary Correlation Operator Method and Similarity Renormalization Group: Connections and Differences
- Ab initio computation of the 17F proton-halo state and resonances in A = 17 nuclei
- Charge radii and neutron correlations in helium halo nuclei
- Low-energy cross section of the 7Be(p,g)8B solar fusion reaction from Coulomb dissociation of 8B
- Wilson Loops as Precursors
- Bonnor stars in d spacetime dimensions
- Chargino Contributions in Asymmetry
Cited by in corpus (6)
- Unified ab initio approach to bound and unbound states: no-core shell model with continuum and its application to 7He
- P-shell nuclei using Similarity Renormalization Group evolved three-nucleon interactions
- Nuclear rotation in the continuum
- Deuteron-induced nucleon transfer reactions within an ab initio framework: First application to p-shell nuclei
- Calculating reactions with use of no-core shell-model states
- Li(,)Li transfer reaction in the NCSM/RGM approach