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We study the onset of neutron drip in high density matter in the presence ofmagnetic field. It has been found that for systems having only protons andelectrons, in the presence of magnetic field >~ 10^{15}G, the neutronizationoccurs at a density which is atleast an order of magnitude higher compared tothat in a nonmagnetic system. In a system with heavier ions, the effect ofmagnetic field, however, starts arising at a much higher field, >~ 10^{17}G.These results may have important implications in high magnetic neutron starsand white dwarfs and, in general, nuclear astrophysics when the system isembedded with high magnetic field.

Revised density of magnetized nuclear matter at the neutron drip line