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RESEARCH ARTICLE
Comparison of microwave processing and excess steam jetcooking for spherulite production from amylose–fatty acidinclusion complexesy
Frederick C. Felker1, James A. Kenar1, George F. Fanta2 and Atanu Biswas2
1 Functional Foods Research Unit, USDA, Agricultural Research Service, National Center for Agricultural Utilization Research,Peoria, IL, USA
2 Plant Polymer Research Unit, USDA, Agricultural Research Service, National Center for Agricultural Utilization Research,Peoria, IL, USA
Helical inclusion complexes of amylose with fatty acids can form spherulites of various morpho-
logical types. Previous studies have described the spherulites obtained by cooling dispersions of
steam jet cooked corn starch either by itself or supplemented with various fatty acids. In light of
potential advantages of microwave processing, we investigated the use of a laboratory microwave
instrument as an alternative method for spherulite production. With native high amylose corn
starch (HAS), spherulites were formed with morphology similar to those observed previously by
steam jet cooking. Adjustments to the reaction conditions led to a slight improvement in yield over
jet cooking. Using solvent-defatted HAS supplemented with straight-chain fatty acids (C10:0 to
C22:0), microwave processing produced only small, disc-shaped spherulites in a gel matrix.
However, when defatted HAS was supplemented with either capric or palmitic acid and processed
by steam jet cooking, uniform dispersions of toroidal spherulites were obtained. These results
show that although jet cooking is not required for spherulite formation when native HAS is used,
defatted HAS requires the high-shear steam jet cooking method of heating for optimal spherulite
growth. Researchers and product developers could use the results of microwave experiments to
refine jet cooking methods for large scale spherulite production.
Received: September 26, 2012
Revised: January 30, 2013
Accepted: January 31, 2013
Keywords:
Jet cooking / Microwave / Spherulites / V-amylose
1 Introduction
When amylose forms V-type inclusion complexes with vari-
ous fatty acids, the resulting complexes can be precipitated
from aqueous solutions upon cooling to form either amor-
phous material or semi-crystalline structures or spherulites
[1, 2]. Much research has been directed towards understand-
ing the molecular interactions between amylose, the fatty acid
ligands, and water leading to the stabilization of the complex
and formation of the unit cell structures and crystalline
lamellae. However, the mechanisms involved in the for-
mation of larger supramolecular assemblies or micron-sized
spherulites are not well understood [3]. For example, no basis
has yet been suggested to explain why a V-amylose spherulite
would develop in a toroidal versus radial manner, or what
limits the growth of spherulites to yield uniform dispersions
of spherulites with a narrow size range.
Spherulites in the micron size range can be prepared by
cooling dispersions of corn starch that have been passed
through a steam jet cooker under excess steam conditions
to provide a high shear environment and a peak temperature
yMention of trade names or commercial products in this publi-cation is solely for the purpose of providing specific informationand does not imply recommendation or endorsement by the U.S.Department of Agriculture. USDA is an equal opportunity pro-vider and employer.
Correspondence: Dr. Frederick C. Felker, Functional FoodsResearch Unit, USDA, Agricultural Research Service, NationalCenter for Agricultural Utilization Research, 1815 N. UniversitySt., Peoria, IL 61604, USAE-mail: [email protected]: þ1-309-681-6685
Abbreviations: HAS, high amylose corn starch
DOI 10.1002/star.201200218864 Starch/Starke 2013, 65, 864–874
� 2013WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim www.starch-journal.com
of 1408C. The native lipid constituents of corn starch that
complex with amylose produce both torus/disc-shaped and
spherical/lobed spherulites of various sizes [4]. When defat-
ted corn starch, supplemented with a variety of specific fatty
acids, was similarly jet-cooked, spherulites with variations in
morphology and size were formed [5]. These spherulites are
dissimilar in several respects from the radially symmetrical
spherulites obtained from lipid-free amylose processed
at higher temperatures, which have been the subject of
extensive research in terms of their synthesis and character-
ization [6–8].
A number of factors influence the yield, size, and
morphology of V-amylose spherulites, including starch and
ligand concentrations, cooling rates, ligand structure, and the
presence or absence of native lipids. By varying these con-
ditions, spherulite yields on the order of 80%, based on
amylose content, could be obtained using excess steam jet
cooking to disperse the starch [9]. In order to enable the
consistent production of uniform spherulite dispersions in
large quantities sufficient to develop specific biobased appli-
cations, the identification of the necessary feedstock type,
ligand, and preparation conditions would be required.
Excess steam jet cooking is an efficient, scalable technique
for producing starch dispersions in which the high tempera-
ture and shear forces completely disrupt the starch granules
and slightly reduce the molecular weight of both the amylose
and amylopectin fractions [10]. It was recently shown that
steam jet cooking corn starch at a temperature as low as 1008Cresulted in significantly smaller particle size and a higher
level of starch granule degradation than hot water boiling at
908C, due to the higher shear forces of the jet cooking process[11]. Because high temperature and shear are inseparable
factors with steam jet cooking, an alternative method was
needed to provide high temperature in a low-shear processing
system in order to evaluate the role of shear in the preparation
of starch for spherulite formation.
Laboratory microwave technology offers several advan-
tages for these investigations including programmable heat-
ing, smaller batch size, and the availability of high pressure
reactor vessels. The versatility of this heating approach has
been used to advantage in the preparation of starch acetates
[12, 13]. In addition to these practical considerations, the
ability of microwave irradiation to rapidly heat and activate
a reaction sequence often leads to higher reaction rates,
yields, and efficiency [14]. Magnetic stirring can also be used
in the reaction vessels employed for microwave heating, thus
providing uniform heating in a low-shear environment
relative to that obtained in a steam jet cooker. This factor
allows the effects of the high shear component of the cooking
process on the yield and morphology of spherulites to be
evaluated. Although steam jet cooking ismore readily scalable
to commercial production requirements, the use of micro-
wave processing may allow researchers and product devel-
opers to efficiently investigate and optimize such factors as
ligand type, reagent concentration, reaction times, tempera-
ture requirements, and stirring conditions for spherulite
formation.
The purpose of this study was to determine (1) whether the
high shear method of steam jet cooking is necessary for
spherulite production, (2) whether microwave heating would
reveal factors which improve the yield of spherulites over that
obtained by jet cooking, and (3) to determine whether uniform
dispersions of spherulites could be obtained with defatted high
amylose starch supplemented with individual fatty acids.
Establishment of the usefulness of microwave processing
for spherulite formation would allow the investigation of other
potential ligands, which might not be available in the relatively
large amounts necessary for processing by jet cooking.
2 Materials and methods
2.1 Materials
High amylose corn starch (HAS) (AmyloGel 03003, contain-
ing 70% apparent amylose) was a product of Cargill
(Minneapolis, MN). Defatted HAS was prepared by sequen-
tial extraction with refluxing 85%methanol–water and 75% n-propanol–water [15]. Fatty acids and other reagents were
purchased from Sigma Chemical Co. (St. Louis, MO). Fatty
acids were either dissolved in ethanol, applied to the dry
starch, and the ethanol evaporated before jet cooking or
microwave processing of the starch, or dry mixed with the
starch before processing, as indicated in the results section.
2.2 Processing by steam jet cooking
Spherulites were prepared by jet cooking using a Penick and
Ford (Cedar Rapids, IA) Laboratory Model steam jet cooker
operating with 65 psig (550 kPa) line pressure and 40 psig
(380 kPa) back pressure (1408C) [10]. Samples were immedi-
ately transferred to a programmable water bath preheated to
958C, and allowed to cool to 408C over 22 h. Dispersions were
then diluted with water to give a 10-fold reduction in solids
concentration, and the spherulites were isolated by centrifu-
gation in a Beckman GS-6KR centrifuge (Beckman
Instruments Inc., Fullerton, CA) at 3000 rpm (approx.
1470 � g). Dissolved starch was removed from the precipi-
tated spherulites by washing two times with excess water
followed by centrifugation. Percent yield was determined
by freeze drying the water-washed spherulites. Data presented
are the mean of three experiments.
2.3 Microwave processing
An Ethos 1600 (Milestone Inc., Monroe, CT) microwave
reactor oven was used to irradiate mixtures of starch–fatty
acid mixtures dispersed in 100 mL deionized water in a
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sealed 100 mL perfluoroalkoxy Teflon1 reactor vessel (prod-
uct code 45111T). The sample was stirred using a Teflon1
4-bar magnetic stirrer at maximum speed and heated from 0
to 1208C in 1.5 min, 120 to 1408C in 1.5 min, and held at
1408C for 10 min (Fig. 1) unless otherwise specified. The
reaction mixture was allowed to cool for 10 min to 1008C and
then maintained at 1008C for 60 min unless otherwise speci-
fied. The reactor vessel was then transferred to a program-
mable water bath preheated to 958C, and allowed to cool to
408C over 22 h. Spherulites were diluted, washed, and freeze-
dried as described above for processing by steam jet cooking.
2.4 Microscopy
Aqueous dispersions of spherulites were observed with a
Zeiss Axioskop light microscope equipped with an
Axiocam ICc 3 digital camera (Carl Zeiss, Inc.,
Thornwood, NY) using phase contrast optics. For SEM,
samples were dehydrated with ethanol, critical point dried
with CO2 onto aluminum stubs, sputter coated with gold, and
examined and photographed with a JEOL 6400V scanning
electron microscope (JEOL, Peabody, MA).
2.5 X-ray diffraction
Freeze-dried samples were equilibrated at 238C and 45%
relative humidity prior to analysis. X-ray powder diffraction
patterns were obtained with a Phillips 1820 diffractometer
operated at 40 kV with graphite-filtered Cu Ka radiation and a
u compensating slit. Data were acquired in 2u ¼ 0.058, 4 s
steps.
2.6 Differential scanning calorimetry (DSC)
Thermal properties were determined using a TA Instruments
(New Castle, DE) model Q2000 DSC calibrated against an
indium standard (156.68C, 28.86 J/g). Data was collected and
analyzed with TA Universal Analysis 2000 V3.9A software.
Freeze-dried samples for DSC were prepared at 20–25 wt%
(dry weight basis) of sample (approximately 10–12 mg) in
water using high volume stainless steel DSC pans. The pans
were hermetically sealed and allowed to equilibrate at least
4 h before analysis. Samples were referenced against an
identical DSC pan containing water and analyzed using
modulation (�0.408C every 40 s) at a heating rate (b) of
5.08C/min. Samples were analyzed by first heating from 0
to 2058C, immediately cooling back to 08C at 5.08C/min, and
then reheating from 0 to 1908C. The melting point (TM) was
taken at the peaks of the DSC curve. Exothermic signals are
reported in the upward direction.
3 Results and discussion
3.1 Formation of spherulites from Native HAS-
palmitic acid mixtures
For a direct comparison with the previously published con-
ditions used with steam jet cooking [5], aqueous dispersions
of 3.5% w/v native HAS combined with 5% palmitic acid
(based on amylose content) were processed by steam jet
cooking followed by slow cooling, giving a spherulite yield
of 82.9% (Experiment 1, Table 1). The microwave processing
method was designed to simulate as closely as possible the
conditions afforded by steam jet cooking, so a 10-min hold
period at 1408Cwas included to insure complete dispersion of
the starch and solubility of the ligand. When the dispersion
was not held for 60 min at 1008C after cooling from 1408C,the spherulite yield was 58.1% (Experiment 2, Table 1). A
single experiment was carried out with a doubling of the
palmitic acid supplementation to 10% (based on amylose),
giving only a slightly higher yield of 70.9%. This suggested
Figure 1. Temperature profile for microwave processing.
Table 1. Formation of spherulites from native high amylose starch and palmitic acid using steam jet cooking and microwave processing
Experiment # Method Min 1408C hold Min 1008C hold % Yield/amylosea)
1 Jet cooker n/a n/a 82.9 (1.7)
2 Microwave 10 0 58.1 (6.9)
3 Microwave 10 60 85.3 (3.3)
4 Microwave 0 60 88.7 (2.8)
a) Yield of spherulites based on amylose content, mean (SD) of three experiments.
866 F. C. Felker et al. Starch/Starke 2013, 65, 864–874
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that the availability of dissolved palmitic acid for complex
formation was not the limiting factor using microwave proc-
essing. To determine whether the time available for inclusion
complex formation before spherulite formation was a factor,
the dispersion was held at 1008C for 60 min after reducing
the temperature from 1408C, and before beginning the 22-h
cooling period to 408C (Experiment 3, Table 1). This pro-
cedure gave a spherulite yield of 85.3%, which was essentially
the same as the yield from the steam jet cooking method
(82.9%). A slightly higher yield of 88.7% was obtained by
eliminating the 10-min hold at 1408C (Experiment 4, Table 1).
This could be due to less reduction of amylose molecular
weight resulting from less time at 1408C, and indicates that
raising the dispersion to 1408C even briefly provides suffi-
cient heat to adequately dissolve the ligand and disperse the
amylose.
Phase contrast images of representative samples from
each of the four experiments are shown in Fig. 2. In each
case, the most abundant spherulite type was toroidal, with a
much less frequent abundance of the lobed morphology
indicated by arrows in the micrographs. Very little difference
was seen between the treatments, indicating that steam jet
cooking is not essential for preparing starch for spherulite
formation. In all treatments, there was a strong tendency for
spherulites to adhere to each other and form large clumps,
especially after washing treatments involving centrifugation.
The toroidal nature of the most abundant spherulite type was
confirmed by SEM as shown in Fig. 3.
Figure 2. Phase contrast light micrographs of spherulites formed from non-defatted HAS processed with steam jet cooking or microwaveheating. Specific treatments are described in Table 1. A–D, Experiments 1–4 (Table 1). Arrows indicate spherulites of spherical/lobedmorphology.
Figure 3. Scanning electron micrographs of toroidal spherulitesobtained from Experiment 3 (Table 1).
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When the palmitic acid supplementation was omitted (in a
single experiment), the spherulite yield dropped to 19.6%,
which is about the same yield reported previously for HAS jet-
cooked without added lipids [9]. However, the morphology of
the spherulites was a mixture of smaller toroidal and lobed
forms essentially similar in shape to those observed with
added palmitic acid. This suggests that the native lipids
present in the high amylose starch may determine the spher-
ulite morphology, whereas the size and yield of those spher-
ulites are enhanced by fatty acid supplementation.
In addition to the spherulite types described above, there
were two other forms of solid material observed in these
experiments. One form appeared as expansive clusters or
networks of uniformly sized, apparently spherical particles
slightly less than 1 mm in diameter (Fig. 4A and B,). The
relative abundance of these particles varied with minor differ-
ences in stirring speed during the microwave experiments,
and they were also present to a lesser extent in samples
prepared by steam jet cooking. The other form appeared
as disorganized, amorphous masses ranging in size from
tens to hundreds of micrometers in diameter (Fig. 4C
and D). The randomly oriented sectors in these very large
particles exhibited a conspicuous striated appearance both in
phase contrast light micrographs (Fig. 4C) and in SEM
images (Fig. 4D). Such striations are characteristic of the
spherical/lobed spherulite morphology visible in the larger
spherulites designated by arrows in Fig. 2. The large masses
were never observed among spherulites produced by steam
jet cooking, and they were only found in microwave exper-
iments in which the palmitic acid was delivered with an
ethanol solution to the starch granules before processing.
They were absent in samples prepared by dry mixing the
starch and palmitic acid. These results suggest that ligands
dried onto starch granules via ethanol solutions were
unevenly distributed, resulting in ligand-rich domains during
granule gelatinization in the heating phase of the microwave
procedure, when the dispersion viscosity was presumably
highest. This would create zones very rich in complexes
which might begin to form spherulitic structures so rapidly
that they grow together, resulting in the discrete, striated
sectors observed in the large masses. In contrast, discrete
palmitic acid particles dry-mixed with the starch may have
dissolved more gradually during heating, and with stirring
there was more uniform distribution of the ligand when not
dried onto individual starch granules. Both the small,
spherical particles and the large disorganized masses exhib-
Figure 4. Phase contrast light micrographs (A and C) and SEM images (B and D) of small, spherical particles (A and B) and large,disorganized masses (C and D) observed in spherulite preparations from non-defatted HAS depending on stirring conditions or methodof ligand addition.
868 F. C. Felker et al. Starch/Starke 2013, 65, 864–874
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ited XRD patterns typical of V6 helical complexes (data not
shown), confirming their interpretation as structures prim-
arily composed of amylose complexes.
3.2 Microwave processing of defatted HASwith fatty
acids varying in chain length
The microwave processing conditions of Experiment 4
(Table 1) were used to determine the type of spherulites
obtained with defatted HAS supplemented with the following
straight-chain fatty acids: capric (C10:0), lauric (C12:0), myr-
istic (C14:0), palmitic (C16:0), stearic (C18:0), and behenic
(C22:0). Unlike the experiments carried out with native HAS,
all six saturated fatty acids yielded dispersions containing a
fragmented gel matrix in which small, flat, disc-shaped spher-
ulites were embedded (Fig. 5A–F). With capric and myristic
acid supplementation, the disc-shaped spherulites were com-
pletely embedded in the gel (Fig. 5A and C), whereas for the
other four fatty acids, individual spherulites were detached
from the gelmatrix (Fig. 5B andD–F).When embedded in the
Figure 5. Phase contrast lightmicrographs of cooled dispersions preparedwithmicrowave heating fromdefatted HAS supplementedwithcapric (A), lauric (B), myristic (C), palmitic (D), stearic (E), and behenic (F) acids. Arrows indicate disc-shaped spherulites.
Starch/Starke 2013, 65, 864–874 869
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gel matrix, only those spherulites oriented vertically (edge-
wise) in the light path could be seen as straight, dark lines,
suggesting the presence of dense, needle-shaped particles.
However, when detached spherulites were seen away from
the gel matrix, many of them settled horizontally on the slide
and could be seen as round objects with a lighter center
region. Horizontally aligned disc-shaped spherulites super-
imposed with the gelled material were apparently obscured
by the mottled gel appearance. SEM showed a similar
appearance of the flat disc morphology in all six treatments
(Fig. 6A–F). Also in each experiment, the SEM images
revealed a fine textured, fibrous network associated with
the spherulites, which was probably the dehydrated remains
of the gelled material seen in the phase contrast images. The
presence of gelled material associated with the spherulites
precluded isolation of the latter, and therefore the spherulite
yield from defatted HAS preparations could not be accurately
determined.
XRD analyses were performed on the defattedHASmicro-
wave-processed samples to confirm the identity of the pre-
cipitated solid as V-amylose complexes. For reference,
the diffraction pattern for the precipitate isolated from
Figure 6. Scanning electron micrographs of cooled dispersions prepared with microwave heating from defatted HAS supplemented withcapric (A), lauric (B), myristic (C), palmitic (D), stearic (E), and behenic (F) acids. Arrows indicate disc-shaped spherulites.
870 F. C. Felker et al. Starch/Starke 2013, 65, 864–874
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native high amylose starch after microwave processing in the
absence of added fatty acid was obtained using the same
procedure as that used for the fatty acid-supplemented prep-
arations (Fig. 7A). Reflections were observed at scattering
angles of 7.58, 138, 188, 19.58, and 228. Three of these reflec-tions, 7.58, 138, and 19.58, are typical of V6 helical complexes
[16, 17], and patterns with those three reflections were also
observed for the smaller, torus-shaped spherulites isolated
from jet-cooked, non-defatted corn starch. The reflection at
188 may be due to V7-complexed amylose formed from the
more bulky components of the native lipid mixture, such as
linoleic acid. The diffraction pattern obtained from micro-
wave-processed, defatted HAS is shown in Fig. 7B. The main
reflections in this case are represented by a peak at 178 and a
broad, rounded peak at 228–248. When well-defined, this
pattern is indicative of retrograded amylose [18]. Thus, the
non-defatted high amylose starch pattern shown in Fig. 7A
indicates the presence of both retrograded starch, as revealed
by the peaks at 178 and 228–248, and inclusion complexes
from native lipids represented by the other reflection angles.
XRD patterns for the series of products prepared by
microwave processing of defatted HAS with the six fatty acids
are shown in Fig. 8A–F. In each case, peaks of varying
intensity could be seen at scattering angles normally associ-
ated with V6 complexes. Capric, lauric, myristic, palmitic, and
stearic acid-supplemented preparations showed strong peaks
at 138 and 19.58, with smaller but still distinct peaks at 7.58(Fig. 8A–E), indicating the presence of V6 complexes which
would be expected for the small disc-shaped spherulites seen
in the phase contrast and SEM images. Also discernible in
these patterns are smaller and less well-defined peaks at 178and 228, which suggests the presence of some retrograded
amylose. The behenic acid-supplemented HAS preparation
showed less prominent peaks at the typical V6 scattering
angles (Fig. 8F). Bhatnagar and Hanna [19] demonstrated
by XRD that extrusion of normal corn starch with behenic
acid (4% based on dry weight of starch) in a single screw
laboratory extruder at 1408C and 22% moisture gave an
amylose-behenic acid inclusion complex. A lower degree of
spherulite formation with behenic acid than with the other
fatty acids could be attributed to the lower solubility of the
behenic acid ligand under the conditions used in this study.
Since the V6 XRD pattern observed with the small disc
spherulites is the same as that seen with larger, toroid spher-
ulites in previous studies, and some of the disc spherulites
seen in phase contrast images have a lighter center, we
conclude that the discs represent a very early stage in the
growth of toroid spherulites. The low intensity of peaks more
typical of retrograded starch in the X-ray patterns for products
prepared from capric, lauric, myristic, palmitic, and stearic
acids suggests that some portion of the background gel
observed in these preparations may also be V6-complexed
amylose that was unable to form spherulites under the con-
ditions of microwave heating. If retrograded starch was
present in these samples, the amount was not sufficient to
form an overall, rigid gel structure typical of that normally
seen with high amylose starch. Instead, the gelled material
fell apart on dilution and readily separated into very small,
irregular fragments with clumps of embedded spherulites.
DSC has been used extensively to examine V-amylose
complexes prepared using fatty acids [20–22]. Accordingly,
the thermal behavior of the microwave-processed samples of
defatted HAS complexed with the series of fatty acids (C10:0
through C22:0) were examined by DSC. The initial heating
scans, shown in Fig. 9A–E, showed prominent melting endo-
therms with a (TM) of 112.78C (DH ¼ 21.1 J/g), 115.08C(DH ¼ 25.1 J/g), 116.98C (DH ¼ 24.6 J/g), 117.38C
Figure 7. XRD patterns of native HAS (A) and defatted HAS(B) after microwave heating.
Figure 8. XRD patterns of solid material recovered from slowlycooled dispersions prepared with microwave heating fromdefatted HAS supplemented with capric (A), lauric (B), myristic(C), palmitic (D), stearic (E), and behenic (F) acids.
Starch/Starke 2013, 65, 864–874 871
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(DH ¼ 29.1 J/g), and 117.48C (DH ¼ 27.0 J/g) correspond-
ing to the fatty acid treatments C10:0, C12:0, C14:0, C16:0,
and C18:0, respectively. The C22:0 fatty acid sample (Fig. 9F)
gave two endothermic melting transitions at 108.38C(DH ¼ 13.6 J/g) and 122.68C (DH ¼ 8.1 J/g). The observed
endotherms occur in the correct temperature region
(TM � 100–1208C) for V-amylose fatty acid complexes. The
TM progressively increased as the chain length of the fatty acid
increased, in accord with previous reports [20, 23]. The higher
melting nature of these peaks suggests they may represent
Type II V-amylose fatty acid complexes analogous to those
previously reported [21, 24]. Also visible in these thermo-
grams were minor peaks corresponding to uncomplexed fatty
acid (indicated with asterisks in Fig. 9). Further evidence that
the observed endotherms represented V-amylose complexes
was obtained by examining the second reheating scans (data
not shown). Under the DSC conditions used, the first heating
scan fully dissociated the complexes to release the fatty acids,
disordered the amylose, and avoided reforming the com-
plexes upon cooling [25]. The reheating scans showed an
increase in the peaks between 31 and 808C corresponding
to themelting point of released fatty acids and no endotherms
between 112 and 1188C indicative of the amylose–fatty acid
complexes. In the case of the C22:0 fatty acid sample, both
peaks disappeared. The presence in the initial heating scan
and disappearance in the second scan of the two endotherms
for C22:0 complexes could be the result of heterogeneity of
the complexes, such as both helical sizes (6 and 7 glucosyl
units per turn) being present [26], or recrystallization of
complexes during the course of the DSC scan [27].
Typically, the endothermic transitions of retrograded amy-
lose occur in the region of �140–1608C [23]. No significant
endotherms in that temperature range were observed in
any of these samples. The method used for the isolation of
precipitated materials was such that the warm material from
the water bath was immediately diluted to avoid retrograda-
tion of uncomplexed amylose. The DSC profiles suggest that
most of the amylose was complexed by the supplemented
fatty acid ligands, and that only very minor amounts of
retrograded starch, if any, were present.
3.3 Processing of defatted HAS–fatty acid mixtures
by steam jet cooking
To determine whether the partially gelled products and small
size of the spherulites obtained from microwave processing
of defatted HAS supplemented with saturated, straight-chain
fatty acids were a result of the microwave processing method
used, defatted HAS was supplemented with lauric and pal-
mitic acids and processed by steam jet cooking for compari-
son. These preparations were then subjected to the same
cooling profile used for the microwave experiments. Phase
contrast micrographs of the resulting dispersions are shown
in Fig. 10. In contrast to the relatively small disc-shaped
spherulites embedded in gel observed with microwave proc-
essing, the predominant material in these preparations con-
sisted of toroid spherulites with about the same range of sizes
observed with non-defatted HAS processed by microwave
heating and also observed previously using steam jet cooking
[5]. The toroidal spherulites formed from capric acid
(Fig. 10A) were about 5 mm in diameter, while those from
palmitic acid (Fig. 10B) were about 8 mm in diameter. The
spherulite yield from the palmitic acid supplemented prep-
aration was 73% based on amylose, but this is not directly
comparable to the yield obtained with non-defatted HAS
(Experiment 4, Table 1), since these were uniform toroidal
spherulites with none of the spherical/lobed variety present.
As noted previously, most of the spherulites obtained with
microwave processing from non-defatted HAS plus palmitic
acid were very similar in size and morphology to those
produced by steam jet cooking (Figs. 2 and 3). The formation
of gel-embedded, relatively small, disc-shaped spherulites
observed in the series of fatty-acid supplemented, defatted
HAS microwave preparations (Figs. 5 and 6) was unexpected.
The larger size, uniformity, and abundance of toroidal spher-
ulites obtained with defatted HAS supplemented with capric
and palmitic acids processed by steam jet cooking (Fig. 10)
therefore indicates that some aspect of the microwave proc-
essing method was interfering with spherulite formation,
since the same reagents, concentrations, and cooling profiles
led to normal spherulite formation after jet-cooking. The
solubility of the fatty acid ligand under the conditions of
microwave processing is probably not the most important
factor, since with palmitic acid, both steam jet cooking and
microwave processing with non-defatted starch gave good
yields of spherulites. Since the solubility of a fatty acid in
Figure 9. DSC of solid material recovered from slowly cooleddispersions prepared with microwave heating from defattedHAS supplemented with capric (A), lauric (B), myristic (C), palmi-tic (D), stearic (E), andbehenic (F) acids. Endotherms representinguncomplexed fatty acids are indicated with asterisks.
872 F. C. Felker et al. Starch/Starke 2013, 65, 864–874
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hot water would be inversely proportional to chain length, it is
likely that the smaller fatty acids (capric, lauric, and myristic)
also be sufficiently soluble under these conditions. Both the
dispersion morphology and XRD profile of the stearic acid
supplemented defatted HAS preparation were similar to
those of the shorter chain-length ligands, suggesting suffi-
cient solubility of even the C18:0 ligand. Only the behenic acid
preparation indicated a possible reduced solubility condition
as evidenced by the smaller V6 reflections on the XRD pattern
(Fig. 8F). Therefore, we conclude that insufficient solubility of
the fatty acid ligands during microwave heating and incu-
bation is not likely to be the reason for the differences
observed in dispersion morphology.
One factor that might explain the inhibition of spherulite
formation in microwave-processed preparations with defatted
HAS is the possible modification of the properties of HAS by
solvent defatting. It is well known that HAS requiresmore heat
than normal dent corn to fully disperse or dissolve the starch
granules. In a previous study, it was also found that normal
dent corn starch granules from which lipids were completely
removed by extraction with refluxing 75/25 v/v n-propanol–
water exhibited reduced swelling under standard pasting con-
ditions as compared to native, unextracted starch [28]. This
difference suggested that the amylose remaining after lipid
removal had associated during the solvent extraction process,
thus inhibiting granule swelling and solubility. The water
content of the hot solvent would cause a partial gelatinization
followed by retrogradation during cooling. The combination of
usingHAS, which is intrinsicallymore difficult to dissolve, and
the use of hot aqueous solvent extraction may together have
raised the threshold of heat and shear required to disrupt the
granule structure and thus allow the spherulites to form.
Consistent with this possibility is the fact that jet cooking
defatted HAS supplemented with capric and palmitic acids
resulted in the formation of full-size toroidal spherulites as
expected. Alternatively, lower temperature methods of defat-
ting the HAS, or using a different type of starch as a source of
lipid-free amylose, could be used for further investigations of
spherulite formation using microwave processing.
4 Conclusions
When native, non-defatted HAS was used as the amylose
source for V-amylose spherulite formation by microwave
processing with palmitic acid supplementation, the yield of
spherulites was comparable to that obtained by steam jet
cooking. The high shear processing conditions used for steam
jet cooking are therefore not necessary for spherulite prep-
aration. However, if the HAS was defatted by extraction with
refluxing aqueous solvents and then supplemented with
specific fatty acids to form a specific spherulite morphology,
microwave processing yielded very small, disc-shaped spher-
ulites in a gelled matrix. Solvent-defatted HAS supplemented
with capric or palmitic acid and processed by steam jet cook-
ing yielded dispersions of uniform, larger toroidal spheru-
lites, suggesting that the mechanical shear of steam jet
cooking was sufficient to overcome the limitation of amylose
solubility. The practical significance of this finding is that for
large-scale production of spherulites, steam jet cooking pro-
vides a more reliable means of maximally dispersing the
starch as a prerequisite for inclusion complex formation
and spherulite growth. For research purposes, as long as
non-defatted starch is used, microwave processing would
provide a more flexible heating and cooling program useful
for investigating alternative ligands or optimizing heating and
cooling conditions. Information gained from microwave
studies could then be readily adapted to large scale processing
methods using steam jet cooking.
The assistance of Gary Grose with XRD, Arthur Thompsonwith SEM, and Jeanette Little, Janet Berfield, and JanetLingenfelter is gratefully acknowledged.
The authors have declared no conflict of interest.
Figure 10. Phase contrast micrographs of uniform toroidalspherulites prepared by steam jet cooking defatted HAS supple-mented with capric (A) and palmitic (B) acid.
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