  The Hawking radiation can be viewed from very different perspectives, not all
of which can be proved to be rigorously equivalent to one another. On the other
hand, an old interest in the zitterbewegung (ZB) of the Dirac electron has
recently been rekindled by the investigations on spintronics and graphene, etc.
In this letter, we show that, if particles emitted by black holes are electrons
or positrons, one can also regard the Hawking radiation as a ZB process.
