Pseudo-spectral methods for atoms in strong magnetic fields
Abstract
We present a new pseudo-spectral algorithm for the calculation of the structure of atoms in strong magnetic fields. We have verified this technique for one-, two- and three-electron atoms in zero magnetic fields against laboratory results and find typically better than 1 per cent accuracy. We further verify this technique against the state-of-the-art calculations of hydrogen, helium and lithium in strong magnetic fields (up to about 2 × 106 T) and find a similar level of agreement. The key enabling advantages of the algorithm are its simplicity (about 130 lines of commented code) and its speed (about 102-105 times faster than finite-element methods to achieve similar accuracy).
- Publication:
-
Monthly Notices of the Royal Astronomical Society
- Pub Date:
- September 2010
- DOI:
- 10.1111/j.1365-2966.2010.16937.x
- arXiv:
- arXiv:0903.0020
- Bibcode:
- 2010MNRAS.407..590H
- Keywords:
-
- atomic data;
- magnetic fields;
- methods: numerical;
- stars: magnetic field;
- stars: neutron;
- white dwarfs;
- Physics - Atomic Physics;
- Astrophysics - Solar and Stellar Astrophysics
- E-Print:
- 10 pages, version accepted to MNRAS