Despite significant recent developments
in the field of high entropy
oxides, previously reported HEOs are overwhelmingly stoichiometric
structures containing a single cationic site and are stabilized solely
by intermixing increasing numbers of cations. For the first time,
we demonstrate here that cationic vacancies can significantly increase
configurational entropy and stabilize phase-pure HEOs. Aluminate spinel
HEOs with AB2O4 stoichiometry are used as a
model crystal structure. These spinels tolerate large divalent cation
deficiencies without changing phase, allowing for high concentrations
of cationic vacancies. Stoichiometric and sub-stoichiometric spinels
(with A:B molar ratios <0.5), which contained various mixtures
of Co, Cu, Mg, Mn, Ni, and cationic vacancies in nominal equimolar
concentration, were systematically compared as a function of heat
treatment temperature and number of unique cationic species. We found
that the same number of cationic species were needed to stabilize
both stoichiometric and sub-stoichiometric nickel-containing spinels
at 800 °C calcination, as exemplified by (CoCuMgNi)Al2O4 and (CoMgNi)0.75Al2Ox samples, signifying that vacancies stabilize phase-pure spinels
similarly to cations. The chromatic, structural, and chemical properties
of these complex spinels were highly tunable via incorporation of
cationic vacancies and multiple divalent metals, promoting their potential
application as unique pigments, catalysts, and thermal coatings.