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Journal of the European Ceramic Society 35 (2015) 3103–3109
Enhanced structural and phase stability of titania inverse opals
Robert M. Pasquarelli
a,∗
, Hooi Sing Lee
b
, Roman Kubrin
a,d
, Robert Zierold
c
,
Alexander Yu. Petrov
b
, Kornelius Nielsch
c
, Gerold A. Schneider
a
, Manfred Eich
b
, Rolf Janssen
a
a
Institute of Advanced Ceramics, Hamburg University of Technology (TUHH), 21073 Hamburg, Germany
b
Institute of Optical and Electronic Materials, Hamburg University of Technology (TUHH), 21073 Hamburg, Germany
c
Institute of Nanostructure and Solid State Physics, Universität Hamburg, 20355 Hamburg, Germany
d
Laboratory for High Performance Ceramics, Empa, Swiss Federal Laboratories for Materials Science and Technology, 8600 Dübendorf, Switzerland
Received 21 February 2015; received in revised form 20 April 2015; accepted 24 April 2015
Available online 15 May 2015
Abstract
The applications and processing of nanostructured materials at high temperatures require stability of their morphology. However, in such envi-
ronments (>1000
◦
C), these structures are prone to significant undesired microstructural changes that result in a loss of functional properties. The
thermal stability of titania inverse opal films, prepared from self-assembled templates of monodisperse polystyrene spheres by infiltration utilizing
atomic layer deposition and subsequent calcination, was assessed. Resistance to grain growth and a shift in the anatase-to-rutile transformation
to higher temperatures was observed, with dramatic stability under vacuum. Vacuum annealed samples retained the anatase phase and exhibited
minimal grain growth even after 3 h at 1300
◦
C. Photonic properties were retained until the transformation onset. The remarkable resistance was
attributed to inhibition of surface diffusion and structure-substrate constraints. In addition to being technologically enabling, the results provide
further insight into the titania system and its phase transformation mechanism.
© 2015 Elsevier Ltd. All rights reserved.
Keywords: Titania; Anatase-to-rutile; Phase transformation; Inverse opal; Photonic crystal
1. Introduction
Titania is one of the most widely applied materials in cataly-
sis, optics, and photonics [1–3]. Its high refractive index (anatase
n = 2.5 and rutile n = 2.9) makes it particularly attractive for fab-
rication of photonic crystals (PhCs) [4–6]. Synthetic methods
to titania PhCs, typically in the form of three-dimensionally
ordered macropores (3DOM, e.g. inverse opals), commonly
yield the anatase polymorph. However, titania structures are
rarely considered for high temperature applications due to a
phase transformation from anatase to the more thermodynami-
cally stable rutile polymorph, which starts at temperatures as
low as ∼600
◦
C for bulk and nanocrystalline material [1].
The transformation itself is a reconstructive nucleation and
∗
Corresponding author. Tel.: +49 40428783646.
E-mail addresses: robert.pasquarelli@gmail.com (R.M. Pasquarelli),
janssen@tuhh.de (R. Janssen).
growth process. It occurs via surface/interface nucleation, which
initiates rearrangement within the grain [7–9]. Additionally, this
reconstructive phase transformation is accompanied by rapid
coalescence and grain growth [10–13], leading to severe degra-
dation of the morphology of the structural features and a loss of
properties. While a recent study by Li et al. reported the transfor-
mation of anatase inverse opals to rutile [6], no clear comparison
between performance and morphology of the anatase and rutile
structures has been made.
Highly porous periodic structures, especially for high-
temperature photonic applications in thermophotovoltaics
(TPV) and thermal barrier coatings, require the thermal stabil-
ity of these features at the desired service temperatures [14,15].
However, at temperatures on the order of 1000
◦
C, even 3DOM
structures made of refractory oxides, such as alumina or yttria-
stabilized zirconia, exhibit significant undesired microstructural
changes [16–19]. Thermal stabilization of macroporous struc-
tures and photonic crystals remains a significant challenge.
In order to achieve phase stabilization in the titania system,
http://dx.doi.org/10.1016/j.jeurceramsoc.2015.04.041
0955-2219/© 2015 Elsevier Ltd. All rights reserved.