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The energy per particle of zero-temperature neutron matter is investigated,with particular emphasis on the role of the $\vec L\cdot\vec S$ interaction. Ananalysis of the importance of explicit spin--orbit correlations in thedescription of the system is carried out by the auxiliary field diffusion MonteCarlo method. The improved nodal structure of the guiding function, constructedby explicitly considering these correlations, lowers the energy. The proposedspin--backflow orbitals can conveniently be used also in Green's Function MonteCarlo calculations of light nuclei.Comment: 4 pages, 1 figur

Spin-orbit induced backflow in neutron matter with auxiliary field diffusion Monte Carlo method