Abstract
The correlation function Monte Carlo method for calculating ground and excited state properties is extended to complex Hamiltonians and used to calculate the spectrum of neutral helium in a wide range of magnetic fields, a system of particular interest in astrophysics. Correlation functions in imaginary time are evaluated for a set of trial functions over a random walk whose dynamics is governed by the imaginary-time Schrödinger equation. Estimates of the exact energy spectrum and other expectations are made by diagonalizing the matrix of correlation functions. Using the exact results of this “released-phase” Monte Carlo approach, we assess the accuracy of the fixed-phase quantum Monte Carlo and Hartree-Fock methods for the helium atom in strong magnetic fields.
| Original language | English |
|---|---|
| Pages (from-to) | 6202-6210 |
| Number of pages | 9 |
| Journal | Physical Review E |
| Volume | 55 |
| Issue number | 5 |
| DOIs | |
| State | Published - 1997 |
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