5 research outputs found
Exothermic Self-Sustained Waves with Amorphous Nickel
The
synthesis of amorphous Ni (a-Ni) using a liquid-phase chemical reduction
approach is reported. Detailed structural analysis indicates that
this method allows for efficient fabrication of high surface area
(210 m<sup>2</sup>/g) amorphous Ni nanopowder with low impurity content.
We investigated the self-propagating exothermic waves associated with
crystallization of Ni from the amorphous precursor. Time-resolved
X-ray diffraction indicates that amorphous nickel crystallizes in
the temperature range 445–480 K. High-speed infrared imaging
reveals that local preheating of compressed a-Ni nanopowder triggers
a self-sustaining crystallization wave that propagates with velocity
∼0.3 mm/s. The maximum temperature of crystallization wave
depends on the sample density and can be as high as 600 K. The Kissinger
approach is used to determine the apparent activation energy (55.4 ±
4 kJ/mol) of crystallization. The self-diffusion activation energy
of Ni atoms in a-Ni is ∼60 kJ/mol, determined through molecular
dynamics (MD) simulations. This agreement of experimentally derived
and theoretically calculated activation energies allows us to conclude
that self-diffusion of Ni atoms is the rate-limiting stage for crystallization.
Furthermore, utilization of amorphous metal as a reactant significantly
increases the rate of solid-state reactions. For example, in reactive
intermetallic forming systems, such as Ni + Al, the self-sustaining
reaction propagation velocity with a-Ni is twice higher than with
crystalline Ni of the same morphology. Additionally, using a-Ni increases
the maximum reaction temperature in the Ni + Al system by 300 K
Nickel Oxide Reduction by Hydrogen: Kinetics and Structural Transformations
We
studied the reduction kinetics of bulk NiO crystals by hydrogen
and the corresponding structural transformations in the temperature
range of 543–1593 K. A new experimental approach allows us
to arrest and quench the reaction at different stages with millisecond
time resolution. Two distinctive temperature intervals are found where
the reaction kinetics and product microstructures are different. At
relatively low temperatures, 543–773 K, the kinetic curves
have a sigmoidal shape with long induction times (up to 2000 s) and
result in incomplete conversion. Low-temperature reduction forms a
complex polycrystalline Ni/NiO porous structure with characteristic
pore size on the order of 100 nm. No induction period was observed
for the high-temperature conditions (1173–1593 K), and full
reduction of NiO to Ni is achieved within seconds. An extremely fine
porous metal structure, with pore size under 10 nm, forms during high-temperature
reduction by a novel crystal growth mechanism. This consists of the
epitaxial-like transformation of micrometer-sized NiO single crystals
into single-crystalline Ni without any crystallographic changes, including
shape, size, or crystal orientation. The Avrami nucleation model accurately
describes the reaction kinetics in both temperature regimes. However,
the structural transformations during reduction in both nanolevel
and atomic level are very complex, and the mechanism relies on both
nucleation and the critical diffusion length for outward diffusion
of water molecules
Origin of the Size-Dependent Stokes Shift in CsPbBr<sub>3</sub> Perovskite Nanocrystals
The
origin of the size-dependent Stokes shift in CsPbBr<sub>3</sub> nanocrystals
(NCs) is explained for the first time. Stokes shifts
range from 82 to 20 meV for NCs with effective edge lengths varying
from ∼4 to 13 nm. We show that the Stokes shift is intrinsic
to the NC electronic structure and does not arise from extrinsic effects
such as residual ensemble size distributions, impurities, or solvent-related
effects. The origin of the Stokes shift is elucidated via first-principles
calculations. Corresponding theoretical modeling of the CsPbBr<sub>3</sub> NC density of states and band structure reveals the existence
of an intrinsic confined hole state 260 to 70 meV above the valence
band edge state for NCs with edge lengths from ∼2 to 5 nm.
A size-dependent Stokes shift is therefore predicted and is in quantitative
agreement with the experimental data. Comparison between bulk and
NC calculations shows that the confined hole state is exclusive to
NCs. At a broader level, the distinction between absorbing and emitting
states in CsPbBr<sub>3</sub> is likely a general feature of other
halide perovskite NCs and can be tuned via NC size to enhance applications
involving these materials
Transforming Layered to Nonlayered Two-Dimensional Materials: Cation Exchange of SnS<sub>2</sub> to Cu<sub>2</sub>SnS<sub>3</sub>
We
demonstrate the chemical transformation of layered, two-dimensional
(2D) SnS<sub>2</sub> to nonlayered Cu<sub>2</sub>SnS<sub>3</sub> via
cation exchange. Resulting Cu<sub>2</sub>SnS<sub>3</sub> nanosheets
(NSs) retain the overall starting morphology of their parent, few-layer
SnS<sub>2</sub> templates. Specifically, they possess micrometer-sized
dimensions and have controlled thicknesses dictated by the number
of initial SnS<sub>2</sub> layers. Our demonstration shows that existing
layered compounds can serve as templates for difficult-to-synthesize
nonlayered 2D specimens with cation exchange providing a bridge between
families of layered and nonlayered materials. New 2D systems are therefore
accessible, opening the door to future explorations of low-dimensional
nanostructure anisotropic optical and electrical properties
Ultrasmall α‑Fe<sub>2</sub>O<sub>3</sub> Superparamagnetic Nanoparticles with High Magnetization Prepared by Template-Assisted Combustion Process
A template-assisted combustion-based
method is developed to synthesize the ultrasmall (below 5 nm) α-Fe<sub>2</sub>O<sub>3</sub> nanoparticles. The iron and ammonium nitrate
are used as oxidizers, glycine as a “fuel” and mesoporous
silica (SBA-15) as a template. Because of the ultralow sizes and high
crystallinity, the combustion-derived α-Fe<sub>2</sub>O<sub>3</sub> nanoparticles exhibit superparamagnetism in the temperature
range of 70–300 K. The high specific surface area (132 m<sup>2</sup>/g) of α-Fe<sub>2</sub>O<sub>3</sub> indicates the important
role of surface magnetic spins resulting in remarkably high magnetization
(21 emu/g) at 300 K