The effect of composition and temperature on Ni bulk self-diffusion is inve
stigated for nine different single crystalline NiAl alloys with well-define
d compositions between 46.8 and 56.6 at.% Ni in the temperature range from
1050 to 1630K. The diffusion penetration profiles of Ni in NiAl were determ
ined by applying two different techniques of profile detection. Radiotracer
experiments have been carried out using the Ni-63 tracer, a serial section
ing technique, and sensitive liquid scintillation counting for the high tem
perature measurements, while at lower temperatures the diffusion profiles w
ere analyzed by secondary ion mass spectrometry (SIMS) using the highly enr
iched stable isotope Ni-64. In contrast to the literature data on Ni self-d
iffusion in NiAl alloys by Hancock and McDonnell [Phys. stat. sol. A4, (197
1) 143], the present measurements show an unexpected concentration dependen
ce of the Ni diffusion coefficients D with nearly constant diffusivities fo
r stoichiometric and Al-rich alloys and increasing D values with increasing
Ni content on the Ni-rich side of the NiAl composition range. The effectiv
e diffusion activation enthalpy Q is equal to about 3.0 +/-0.07 eV for the
Al-rich, stoichiometric, and slightly Ni-rich NiAl alloys, while for the co
mpositions with larger Ni content a decrease of Q was observed with increas
ing Ni content, for example, Q=2.39 eV for the Ni56.6Al42.4 alloy. The pres
ent experimental results imply that mainly the same diffusion mechanism ope
rates on both sides of stoichiometry in NiAl. This mechanism is identified
with the triple defect mechanism. Its contribution is compositionally indep
endent. The activation energy of Q=3.18 eV was calculated for the triple de
fect mechanism using empirical EAM potentials in agreement with the experim
ental data. The decreage of e at large Ni concentrations on the Ni-rich sid
e is explained by an additional contribution of the anti-structure bridge m
echanism with the activation energy of Q=1.73 eV. (C) 2001 Acta Materialia
Inc. Published by Elsevier Science Ltd. All lights reserved.