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 Schrodinger equation. Estimates of the exact energy spectrum and other expectations are made by diagorializing 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 (US) |
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Pages (from-to) | 6202-6210 |
Number of pages | 9 |
Journal | Physical Review E - Statistical Physics, Plasmas, Fluids, and Related Interdisciplinary Topics |
Volume | 55 |
Issue number | 5 |
DOIs | |
State | Published - 1997 |
ASJC Scopus subject areas
- Statistical and Nonlinear Physics
- Statistics and Probability
- Condensed Matter Physics