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The diffusion quantum Monte Carlo method is extended to solve the oldtheoretical physics problem of many-electron atoms and ions in intense magneticfields. The feature of our approach is the use of adiabatic approximation wavefunctions augmented by a Jastrow factor as guiding functions to initialize thequantum Monte Carlo prodecure. We calcula te the ground state energies of atomsand ions with nuclear charges from Z= 2, 3, 4, ..., 26 for magnetic fieldstrengths relevant for neutron stars.

Diffusion Monte Carlo calculations for the ground states of atoms and ions in neutron star magnetic fields