Ab initio methods (nuclear physics)
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In nuclear physics, ab initio methods seek to describe the atomic nucleus from the ground up by solving the Schrödinger equation in terms of the individual nucleons and the interactions between them. This is a more fundamental approach compared to e.g. the nuclear shell model. Previously limited to very light nuclei, recent progress has enabled ab initio treatment of heavier nuclei such as nickel.[1]
A significant challenge in the ab initio treatment stems from the complexities of the inter-nucleon interaction. The strong nuclear force is believed to emerge from the strong interaction described by quantum chromodynamics (QCD), but QCD is non-pertubative in the low-energy regime relevant to nuclear physics. This makes the direct use of QCD for the description of the inter-nucleon interactions very difficult, and a model must be used instead. The most sophisticated models available are based on chiral effective field theory. This effective field theory (EFT) includes all interactions compatible with the symmetries of QCD, ordered by the size of their contributions. The degrees of freedom in this theory are nucleons and pions, as opposed to quarks and gluons as in QCD. The effective theory contains parameters called low-energy constants, which can be determined from scattering data.[1][2]
Chiral EFT implies the existence of many-body forces, most notably the three-nucleon interaction which is known to be an essential ingredient in the nuclear many-body problem.[1][2]
After arriving at a Hamiltonian (based on chiral EFT or other models) one must solve the Schrödinger equation
- .
Various ab initio methods have been devised to numerically find solutions to this equation:
- Green's function Monte Carlo (GFMC)[3]
- No-core shell model (NCSM)[4]
- Coupled cluster (CC)[5]
- Self-consistent Green's function (SCGF)[6]
- In-medium similarity renormalization group (IM-SRG)[7]
Further reading
Dean, D. (2007). "Beyond the nuclear shell model". Physics Today. Vol. 60, no. 11. p. 48. doi:10.1063/1.2812123.
References
- ^ a b Machleidt, R.; Entem, D.R. (2011). "Chiral effective field theory and nuclear forces". Physics Reports. 503 (1): 1–75. arXiv:1105.2919v1. Bibcode:2011PhR...503....1M. doi:10.1016/j.physrep.2011.02.001.
- ^ Pieper, S.C.; Wiringa, R.B. (2001). "Quantum Monte Carlo calculations of light nuclei". Annual Review of Nuclear and Particle Science. 51: 53–90. doi:10.1146/annurev.nucl.51.101701.132506.
- ^ Barrett, B.R.; Navrátil, P.; Vary, J.P. (2013). "Ab initio no core shell model". Progress in Particle and Nuclear Physics. 69: 131–181. doi:10.1016/j.ppnp.2012.10.003.
- ^ Hagen, G.; Papenbrock, T.; Hjorth-Jensen, M.; Dean, D. J. (2014). "Coupled-cluster computations of atomic nuclei". Reports on Progress in Physics. 77 (9): 096302. doi:10.1088/0034-4885/77/9/096302.
- ^ Cipollone, A.; Barbieri, C.; Navrátil, P. (2013). "Isotopic Chains Around Oxygen from Evolved Chiral Two- and Three-Nucleon Interactions". Phys. Rev. Lett. 111 (6): 062501. doi:10.1103/PhysRevLett.111.062501.
- ^ Hergert, H.; Binder, S.; Calci, A.; Langhammer, J.; Roth, R. (2013). "Ab Initio Calculations of Even Oxygen Isotopes with Chiral Two-Plus-Three-Nucleon Interactions". Phys. Rev. Lett. 110 (24): 242501. doi:10.1103/PhysRevLett.110.242501.