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The newly born millisecond pulsars are investigated as possible energysources for creating ultra-high energy electrons. The transfer of energy fromthe star rotation to high energy electrons takes place through the Landaudamping of centrifugally driven (via a two stream instability) electrostaticLangmuir waves. Generated in the bulk magnetosphere plasma, such waves grow tohigh amplitudes, and then damp, very effectively, on relativistic electronsdriving them to even higher energies. We show that the rate of transfer ofenergy is so efficient that no energy losses might affect the mechanism ofparticle acceleration; the electrons might achieve energies of the order of10^{18}eV for parameters characteristic of a young star.

Millisecond newly born pulsars as efficient accelerators of electrons