10 research outputs found
Method for the Solution Deposition of Phase-Pure CoSe<sub>2</sub> as an Efficient Hydrogen Evolution Reaction Electrocatalyst
We demonstrate the
ability of a thiol–amine solvent mixture
to deposit phase-pure marcasite-type CoSe<sub>2</sub> nanostructured
thin films as effective hydrogen evolution reaction (HER) electrocatalysts.
Electrodes are readily prepared by spin coating a precursor ink onto
highly ordered pyrolytic graphite substrates followed by annealing
to 350 °C. The resulting CoSe<sub>2</sub> films have an onset
potential for HER of −117 mV vs RHE and Tafel slopes of ca.
60 mV dec<sup>–1</sup>. Normalization based on electrochemically
active surface area reveals that simple optimization of film thickness,
based on the number of layers deposited, leads to electrodes with
better surface utilization. Based on the electrocatalytic performance
of the solution-processed CoSe<sub>2</sub> presented here (η<sub>10mA/cm<sup>2</sup></sub> = −272 mV vs RHE), this approach
shows promise as a simple method to deposit a wide range of useful
dichalcogenide electrocatalysts
Crystal Structure Evolution and Notable Thermal Expansion in Hybrid Perovskites Formamidinium Tin Iodide and Formamidinium Lead Bromide
The
temperature-dependent structure evolution of the hybrid halide perovskite
compounds, formamidinium tin iodide (FASnI<sub>3</sub>, FA<sup>+</sup> = CH[NH<sub>2</sub>]<sub>2</sub><sup>+</sup>) and formamidinium lead bromide (FAPbBr<sub>3</sub>), has
been monitored using high-resolution synchrotron X-ray powder diffraction
between 300 and 100 K. The data are consistent with a transition from
cubic <i>Pm</i>3<i>m</i> (No.
221) to tetragonal <i>P</i>4/<i>mbm</i> (No. 127)
for both materials upon cooling; this occurs for FAPbBr<sub>3</sub> between 275 and 250 K, and for FASnI<sub>3</sub> between 250 and
225 K. Upon further cooling, between 150 and 125 K, both materials
undergo a transition to an orthorhombic <i>Pnma</i> (No.
62) structure. The transitions are confirmed by calorimetry and dielectric
measurements. In the tetragonal regime, the coefficients of volumetric
thermal expansion of FASnI<sub>3</sub> and FAPbBr<sub>3</sub> are
among the highest recorded for any extended inorganic crystalline
solid, reaching 219 ppm K<sup>–1</sup> for FASnI<sub>3</sub> at 225 K. Atomic displacement parameters of all atoms for both materials
suggest dynamic motion is occurring in the inorganic sublattice due
to the flexibility of the inorganic network and dynamic lone pair
stereochemical activity on the <i>B</i>-site. Unusual pseudocubic
behavior is displayed in the tetragonal phase of the FAPbBr<sub>3</sub>, similar to that previously observed in FAPbI<sub>3</sub>
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Unraveling the Chemical Nature of the 3D “Hollow” Hybrid Halide Perovskites
The newly introduced class of 3D
halide perovskites, termed “hollow”
perovskites, has been recently demonstrated as light absorbing semiconductor
materials for fabricating lead-free perovskite solar cells with enhanced
efficiency and superior stability. Hollow perovskites derive from
three-dimensional (3D) <i>AMX</i><sub>3</sub> perovskites
(<i>A</i> = methylammonium (MA), formamidinium (FA); M =
Sn, Pb; X = Cl, Br, I), where small molecules such as ethylenediammonium
cations (<i>en</i>) can be incorporated as the dication
without altering the structure dimensionality. We present in this
work the inherent structural properties of the hollow perovskites
and expand this class of materials to the Pb-based analogues. Through
a combination of physical and spectroscopic methods (XRD, gas pycnometry, <sup>1</sup>H NMR, TGA, SEM/EDX), we have assigned the general formula
(A)<sub>1–<i>x</i></sub>(<i>en</i>)<sub><i>x</i></sub>(M)<sub>1–0.7<i>x</i></sub>(X)<sub>3–0.4<i>x</i></sub> to the hollow
perovskites. The incorporation of <i>en</i> in the 3D perovskite
structure leads to massive <i>M</i> and <i>X</i> vacancies in the 3D [<i>MX</i><sub>3</sub>] framework,
thus the term hollow. The resulting materials are semiconductors with
significantly blue-shifted direct band gaps from 1.25 to 1.51 eV for
Sn-based perovskites and from 1.53 to 2.1 eV for the Pb-based analogues.
The increased structural disorder and hollow nature were validated
by single crystal X-ray diffraction analysis as well as pair distribution
function (PDF) analysis. Density functional theory (DFT) calculations
support the experimental trends and suggest that the observed widening
of the band gap is attributed to the massive <i>M</i> and <i>X</i> vacancies, which create a less connected 3D hollow structure.
The resulting materials have superior air stability, where in the
case of Sn-based hollow perovskites it exceeds two orders of temporal
magnitude compared to the conventional full perovskites of MASnI<sub>3</sub> and FASnI<sub>3</sub>. The hollow perovskite compounds pose
as a new platform of promising light absorbers that can be utilized
in single junction or tandem solar cells
Unraveling the Chemical Nature of the 3D “Hollow” Hybrid Halide Perovskites
The newly introduced class of 3D
halide perovskites, termed “hollow”
perovskites, has been recently demonstrated as light absorbing semiconductor
materials for fabricating lead-free perovskite solar cells with enhanced
efficiency and superior stability. Hollow perovskites derive from
three-dimensional (3D) <i>AMX</i><sub>3</sub> perovskites
(<i>A</i> = methylammonium (MA), formamidinium (FA); M =
Sn, Pb; X = Cl, Br, I), where small molecules such as ethylenediammonium
cations (<i>en</i>) can be incorporated as the dication
without altering the structure dimensionality. We present in this
work the inherent structural properties of the hollow perovskites
and expand this class of materials to the Pb-based analogues. Through
a combination of physical and spectroscopic methods (XRD, gas pycnometry, <sup>1</sup>H NMR, TGA, SEM/EDX), we have assigned the general formula
(A)<sub>1–<i>x</i></sub>(<i>en</i>)<sub><i>x</i></sub>(M)<sub>1–0.7<i>x</i></sub>(X)<sub>3–0.4<i>x</i></sub> to the hollow
perovskites. The incorporation of <i>en</i> in the 3D perovskite
structure leads to massive <i>M</i> and <i>X</i> vacancies in the 3D [<i>MX</i><sub>3</sub>] framework,
thus the term hollow. The resulting materials are semiconductors with
significantly blue-shifted direct band gaps from 1.25 to 1.51 eV for
Sn-based perovskites and from 1.53 to 2.1 eV for the Pb-based analogues.
The increased structural disorder and hollow nature were validated
by single crystal X-ray diffraction analysis as well as pair distribution
function (PDF) analysis. Density functional theory (DFT) calculations
support the experimental trends and suggest that the observed widening
of the band gap is attributed to the massive <i>M</i> and <i>X</i> vacancies, which create a less connected 3D hollow structure.
The resulting materials have superior air stability, where in the
case of Sn-based hollow perovskites it exceeds two orders of temporal
magnitude compared to the conventional full perovskites of MASnI<sub>3</sub> and FASnI<sub>3</sub>. The hollow perovskite compounds pose
as a new platform of promising light absorbers that can be utilized
in single junction or tandem solar cells
Unraveling the Chemical Nature of the 3D “Hollow” Hybrid Halide Perovskites
The newly introduced class of 3D
halide perovskites, termed “hollow”
perovskites, has been recently demonstrated as light absorbing semiconductor
materials for fabricating lead-free perovskite solar cells with enhanced
efficiency and superior stability. Hollow perovskites derive from
three-dimensional (3D) <i>AMX</i><sub>3</sub> perovskites
(<i>A</i> = methylammonium (MA), formamidinium (FA); M =
Sn, Pb; X = Cl, Br, I), where small molecules such as ethylenediammonium
cations (<i>en</i>) can be incorporated as the dication
without altering the structure dimensionality. We present in this
work the inherent structural properties of the hollow perovskites
and expand this class of materials to the Pb-based analogues. Through
a combination of physical and spectroscopic methods (XRD, gas pycnometry, <sup>1</sup>H NMR, TGA, SEM/EDX), we have assigned the general formula
(A)<sub>1–<i>x</i></sub>(<i>en</i>)<sub><i>x</i></sub>(M)<sub>1–0.7<i>x</i></sub>(X)<sub>3–0.4<i>x</i></sub> to the hollow
perovskites. The incorporation of <i>en</i> in the 3D perovskite
structure leads to massive <i>M</i> and <i>X</i> vacancies in the 3D [<i>MX</i><sub>3</sub>] framework,
thus the term hollow. The resulting materials are semiconductors with
significantly blue-shifted direct band gaps from 1.25 to 1.51 eV for
Sn-based perovskites and from 1.53 to 2.1 eV for the Pb-based analogues.
The increased structural disorder and hollow nature were validated
by single crystal X-ray diffraction analysis as well as pair distribution
function (PDF) analysis. Density functional theory (DFT) calculations
support the experimental trends and suggest that the observed widening
of the band gap is attributed to the massive <i>M</i> and <i>X</i> vacancies, which create a less connected 3D hollow structure.
The resulting materials have superior air stability, where in the
case of Sn-based hollow perovskites it exceeds two orders of temporal
magnitude compared to the conventional full perovskites of MASnI<sub>3</sub> and FASnI<sub>3</sub>. The hollow perovskite compounds pose
as a new platform of promising light absorbers that can be utilized
in single junction or tandem solar cells
Unraveling the Chemical Nature of the 3D “Hollow” Hybrid Halide Perovskites
The newly introduced class of 3D
halide perovskites, termed “hollow”
perovskites, has been recently demonstrated as light absorbing semiconductor
materials for fabricating lead-free perovskite solar cells with enhanced
efficiency and superior stability. Hollow perovskites derive from
three-dimensional (3D) <i>AMX</i><sub>3</sub> perovskites
(<i>A</i> = methylammonium (MA), formamidinium (FA); M =
Sn, Pb; X = Cl, Br, I), where small molecules such as ethylenediammonium
cations (<i>en</i>) can be incorporated as the dication
without altering the structure dimensionality. We present in this
work the inherent structural properties of the hollow perovskites
and expand this class of materials to the Pb-based analogues. Through
a combination of physical and spectroscopic methods (XRD, gas pycnometry, <sup>1</sup>H NMR, TGA, SEM/EDX), we have assigned the general formula
(A)<sub>1–<i>x</i></sub>(<i>en</i>)<sub><i>x</i></sub>(M)<sub>1–0.7<i>x</i></sub>(X)<sub>3–0.4<i>x</i></sub> to the hollow
perovskites. The incorporation of <i>en</i> in the 3D perovskite
structure leads to massive <i>M</i> and <i>X</i> vacancies in the 3D [<i>MX</i><sub>3</sub>] framework,
thus the term hollow. The resulting materials are semiconductors with
significantly blue-shifted direct band gaps from 1.25 to 1.51 eV for
Sn-based perovskites and from 1.53 to 2.1 eV for the Pb-based analogues.
The increased structural disorder and hollow nature were validated
by single crystal X-ray diffraction analysis as well as pair distribution
function (PDF) analysis. Density functional theory (DFT) calculations
support the experimental trends and suggest that the observed widening
of the band gap is attributed to the massive <i>M</i> and <i>X</i> vacancies, which create a less connected 3D hollow structure.
The resulting materials have superior air stability, where in the
case of Sn-based hollow perovskites it exceeds two orders of temporal
magnitude compared to the conventional full perovskites of MASnI<sub>3</sub> and FASnI<sub>3</sub>. The hollow perovskite compounds pose
as a new platform of promising light absorbers that can be utilized
in single junction or tandem solar cells
Unraveling the Chemical Nature of the 3D “Hollow” Hybrid Halide Perovskites
The newly introduced class of 3D
halide perovskites, termed “hollow”
perovskites, has been recently demonstrated as light absorbing semiconductor
materials for fabricating lead-free perovskite solar cells with enhanced
efficiency and superior stability. Hollow perovskites derive from
three-dimensional (3D) <i>AMX</i><sub>3</sub> perovskites
(<i>A</i> = methylammonium (MA), formamidinium (FA); M =
Sn, Pb; X = Cl, Br, I), where small molecules such as ethylenediammonium
cations (<i>en</i>) can be incorporated as the dication
without altering the structure dimensionality. We present in this
work the inherent structural properties of the hollow perovskites
and expand this class of materials to the Pb-based analogues. Through
a combination of physical and spectroscopic methods (XRD, gas pycnometry, <sup>1</sup>H NMR, TGA, SEM/EDX), we have assigned the general formula
(A)<sub>1–<i>x</i></sub>(<i>en</i>)<sub><i>x</i></sub>(M)<sub>1–0.7<i>x</i></sub>(X)<sub>3–0.4<i>x</i></sub> to the hollow
perovskites. The incorporation of <i>en</i> in the 3D perovskite
structure leads to massive <i>M</i> and <i>X</i> vacancies in the 3D [<i>MX</i><sub>3</sub>] framework,
thus the term hollow. The resulting materials are semiconductors with
significantly blue-shifted direct band gaps from 1.25 to 1.51 eV for
Sn-based perovskites and from 1.53 to 2.1 eV for the Pb-based analogues.
The increased structural disorder and hollow nature were validated
by single crystal X-ray diffraction analysis as well as pair distribution
function (PDF) analysis. Density functional theory (DFT) calculations
support the experimental trends and suggest that the observed widening
of the band gap is attributed to the massive <i>M</i> and <i>X</i> vacancies, which create a less connected 3D hollow structure.
The resulting materials have superior air stability, where in the
case of Sn-based hollow perovskites it exceeds two orders of temporal
magnitude compared to the conventional full perovskites of MASnI<sub>3</sub> and FASnI<sub>3</sub>. The hollow perovskite compounds pose
as a new platform of promising light absorbers that can be utilized
in single junction or tandem solar cells
Unraveling the Chemical Nature of the 3D “Hollow” Hybrid Halide Perovskites
The newly introduced class of 3D
halide perovskites, termed “hollow”
perovskites, has been recently demonstrated as light absorbing semiconductor
materials for fabricating lead-free perovskite solar cells with enhanced
efficiency and superior stability. Hollow perovskites derive from
three-dimensional (3D) <i>AMX</i><sub>3</sub> perovskites
(<i>A</i> = methylammonium (MA), formamidinium (FA); M =
Sn, Pb; X = Cl, Br, I), where small molecules such as ethylenediammonium
cations (<i>en</i>) can be incorporated as the dication
without altering the structure dimensionality. We present in this
work the inherent structural properties of the hollow perovskites
and expand this class of materials to the Pb-based analogues. Through
a combination of physical and spectroscopic methods (XRD, gas pycnometry, <sup>1</sup>H NMR, TGA, SEM/EDX), we have assigned the general formula
(A)<sub>1–<i>x</i></sub>(<i>en</i>)<sub><i>x</i></sub>(M)<sub>1–0.7<i>x</i></sub>(X)<sub>3–0.4<i>x</i></sub> to the hollow
perovskites. The incorporation of <i>en</i> in the 3D perovskite
structure leads to massive <i>M</i> and <i>X</i> vacancies in the 3D [<i>MX</i><sub>3</sub>] framework,
thus the term hollow. The resulting materials are semiconductors with
significantly blue-shifted direct band gaps from 1.25 to 1.51 eV for
Sn-based perovskites and from 1.53 to 2.1 eV for the Pb-based analogues.
The increased structural disorder and hollow nature were validated
by single crystal X-ray diffraction analysis as well as pair distribution
function (PDF) analysis. Density functional theory (DFT) calculations
support the experimental trends and suggest that the observed widening
of the band gap is attributed to the massive <i>M</i> and <i>X</i> vacancies, which create a less connected 3D hollow structure.
The resulting materials have superior air stability, where in the
case of Sn-based hollow perovskites it exceeds two orders of temporal
magnitude compared to the conventional full perovskites of MASnI<sub>3</sub> and FASnI<sub>3</sub>. The hollow perovskite compounds pose
as a new platform of promising light absorbers that can be utilized
in single junction or tandem solar cells
Unraveling the Chemical Nature of the 3D “Hollow” Hybrid Halide Perovskites
The newly introduced class of 3D
halide perovskites, termed “hollow”
perovskites, has been recently demonstrated as light absorbing semiconductor
materials for fabricating lead-free perovskite solar cells with enhanced
efficiency and superior stability. Hollow perovskites derive from
three-dimensional (3D) <i>AMX</i><sub>3</sub> perovskites
(<i>A</i> = methylammonium (MA), formamidinium (FA); M =
Sn, Pb; X = Cl, Br, I), where small molecules such as ethylenediammonium
cations (<i>en</i>) can be incorporated as the dication
without altering the structure dimensionality. We present in this
work the inherent structural properties of the hollow perovskites
and expand this class of materials to the Pb-based analogues. Through
a combination of physical and spectroscopic methods (XRD, gas pycnometry, <sup>1</sup>H NMR, TGA, SEM/EDX), we have assigned the general formula
(A)<sub>1–<i>x</i></sub>(<i>en</i>)<sub><i>x</i></sub>(M)<sub>1–0.7<i>x</i></sub>(X)<sub>3–0.4<i>x</i></sub> to the hollow
perovskites. The incorporation of <i>en</i> in the 3D perovskite
structure leads to massive <i>M</i> and <i>X</i> vacancies in the 3D [<i>MX</i><sub>3</sub>] framework,
thus the term hollow. The resulting materials are semiconductors with
significantly blue-shifted direct band gaps from 1.25 to 1.51 eV for
Sn-based perovskites and from 1.53 to 2.1 eV for the Pb-based analogues.
The increased structural disorder and hollow nature were validated
by single crystal X-ray diffraction analysis as well as pair distribution
function (PDF) analysis. Density functional theory (DFT) calculations
support the experimental trends and suggest that the observed widening
of the band gap is attributed to the massive <i>M</i> and <i>X</i> vacancies, which create a less connected 3D hollow structure.
The resulting materials have superior air stability, where in the
case of Sn-based hollow perovskites it exceeds two orders of temporal
magnitude compared to the conventional full perovskites of MASnI<sub>3</sub> and FASnI<sub>3</sub>. The hollow perovskite compounds pose
as a new platform of promising light absorbers that can be utilized
in single junction or tandem solar cells
Unraveling the Chemical Nature of the 3D “Hollow” Hybrid Halide Perovskites
The newly introduced class of 3D
halide perovskites, termed “hollow”
perovskites, has been recently demonstrated as light absorbing semiconductor
materials for fabricating lead-free perovskite solar cells with enhanced
efficiency and superior stability. Hollow perovskites derive from
three-dimensional (3D) <i>AMX</i><sub>3</sub> perovskites
(<i>A</i> = methylammonium (MA), formamidinium (FA); M =
Sn, Pb; X = Cl, Br, I), where small molecules such as ethylenediammonium
cations (<i>en</i>) can be incorporated as the dication
without altering the structure dimensionality. We present in this
work the inherent structural properties of the hollow perovskites
and expand this class of materials to the Pb-based analogues. Through
a combination of physical and spectroscopic methods (XRD, gas pycnometry, <sup>1</sup>H NMR, TGA, SEM/EDX), we have assigned the general formula
(A)<sub>1–<i>x</i></sub>(<i>en</i>)<sub><i>x</i></sub>(M)<sub>1–0.7<i>x</i></sub>(X)<sub>3–0.4<i>x</i></sub> to the hollow
perovskites. The incorporation of <i>en</i> in the 3D perovskite
structure leads to massive <i>M</i> and <i>X</i> vacancies in the 3D [<i>MX</i><sub>3</sub>] framework,
thus the term hollow. The resulting materials are semiconductors with
significantly blue-shifted direct band gaps from 1.25 to 1.51 eV for
Sn-based perovskites and from 1.53 to 2.1 eV for the Pb-based analogues.
The increased structural disorder and hollow nature were validated
by single crystal X-ray diffraction analysis as well as pair distribution
function (PDF) analysis. Density functional theory (DFT) calculations
support the experimental trends and suggest that the observed widening
of the band gap is attributed to the massive <i>M</i> and <i>X</i> vacancies, which create a less connected 3D hollow structure.
The resulting materials have superior air stability, where in the
case of Sn-based hollow perovskites it exceeds two orders of temporal
magnitude compared to the conventional full perovskites of MASnI<sub>3</sub> and FASnI<sub>3</sub>. The hollow perovskite compounds pose
as a new platform of promising light absorbers that can be utilized
in single junction or tandem solar cells