The energy distributions of electron emission from a Schottky emitter
have been studied at tip temperatures from 1450 to 1800 K and angular
current densities from 0.1 to 240 mu A/sr. We have observed broadening
of the energy distribution, with increase of angular current density
and decrease of tip temperature, from 0.4 to 1.32 eV resulting from el
ectron tunneling and electron-electron interaction. Good agreement bet
ween the experimental results and predictions from Monte Carlo simulat
ion of the emission process is observed. (C) 1997 American Institute o
f Physics.