28 research outputs found
Pressure-Stabilized Ir<sup>3–</sup> in a Superconducting Potassium Iridide
The first charge-separated iridide
(Ir<sup>3–</sup>) in
an extended solid was identified at elevated pressure when combined
with potassium. According to an unbiased structure searching method
that combines first-principles calculations with particle swarm optimization
algorithms, K<sub>3</sub>Ir in the Cu<sub>3</sub>Ti-type structure
shows a favorable formation enthalpy (Δ<i>H</i>) compared
to the elements and is dynamically stable above 10 GPa. This novel
semiconductor (<i>E</i><sub>g</sub> ≈ 1.6 eV) has
sufficient orbital separation to allow complete charge transfer from
K to Ir, and Bader charge analysis supports the formation of a formally
anionic Ir<sup>3–</sup>. Further, electron doping of K<sub>3</sub>Ir through Pt substitution makes the system metallic, and
electron–phonon coupling calculations indicate that K<sub>3</sub>(Ir<sub>0.875</sub>Pt<sub>0.125</sub>) falls in the strong-coupling
regime, with a predicted superconducting transition temperature (<i>T</i><sub>c</sub>) of ∼27 K at 20 GPa. These results
suggest that systems containing elements isoelectronic with classical
BCS superconductors such as mercury might have an increased probability
of exhibiting a superconducting transition
Validation of Interstitial Iron and Consequences of Nonstoichiometry in Mackinawite (Fe<sub>1+<i>x</i></sub>S)
A theoretical investigation of the relationship between
chemical
composition and electronic structure was performed on the nonstoichiometric
iron sulfide, mackinawite (Fe<sub>1+x</sub>S), which is isostructural
and isoelectronic with the superconducting Fe<sub>1+<i>x</i></sub>Se and Fe<sub>1+<i>x</i></sub>(Te<sub>1–<i>y</i></sub>Se<sub><i>y</i></sub>) phases. Even though
Fe<sub>1+x</sub>S has not been measured for superconductivity, the
effects of stoichiometry on transport properties and electronic structure
in all of these iron-excess chalcogenide compounds has been largely
overlooked. In mackinawite, the amount of Fe that has been reported
ranges from a large excess, Fe<sub>1.15</sub>S, to nearly stoichiometric,
Fe<sub>1.00(7)</sub>S. Here, we analyze, for the first time, the electronic
structure of Fe<sub>1+<i>x</i></sub>S to justify these nonstoichiometric
phases. First principles electronic structure calculations using supercells
of Fe<sub>1+<i>x</i></sub>S yield a wide range of energetically
favorable compositions (0 < <i>x</i> < 0.30). The
incorporation of interstitial Fe atoms originates from a delicate
balance between the Madelung energy and the occupation of Fe–S
and Fe–Fe antibonding orbitals. A theoretical assessment of
various magnetic structures for “FeS” and Fe<sub>1.06</sub>S indicate that striped magnetic ordering along [110] is the lowest
energy structure and the interstitial Fe affects the values of moments
in the square planes as a function of distance. Moreover, the formation
of the magnetic moment is dependent on the unit cell volume, thus
relating it to composition. Finally, changes in the composition cause
a modification of the Fermi surface and ultimately the loss of a nested
vector
Predicting the Band Gaps of Inorganic Solids by Machine Learning
A machine-learning
model is developed that can accurately predict
the band gap of inorganic solids based only on composition. This method
uses support vector classification to first separate metals from nonmetals,
followed by quantitatively predicting the band gap of the nonmetals
using support vector regression. The superb accuracy of the regression
model is obtained by using a training set composed entirely of experimentally
measured band gaps and utilizing only compositional descriptors. In
fact, because of the unique training set of experimental data, the
machine learning predicted band gaps are significantly closer to the
experimentally reported values than DFT (PBE-level) calculated band
gaps. Not only does this resulting tool provide the ability to accurately
predict the band gap for any composition but also the versatility
and speed of the prediction based only on composition will make this
a great resource to screen inorganic phase space and direct the development
of functional inorganic materials
Predicting the Band Gaps of Inorganic Solids by Machine Learning
A machine-learning
model is developed that can accurately predict
the band gap of inorganic solids based only on composition. This method
uses support vector classification to first separate metals from nonmetals,
followed by quantitatively predicting the band gap of the nonmetals
using support vector regression. The superb accuracy of the regression
model is obtained by using a training set composed entirely of experimentally
measured band gaps and utilizing only compositional descriptors. In
fact, because of the unique training set of experimental data, the
machine learning predicted band gaps are significantly closer to the
experimentally reported values than DFT (PBE-level) calculated band
gaps. Not only does this resulting tool provide the ability to accurately
predict the band gap for any composition but also the versatility
and speed of the prediction based only on composition will make this
a great resource to screen inorganic phase space and direct the development
of functional inorganic materials
Magnetic Ordering in Tetragonal 3d Metal Arsenides M<sub>2</sub>As (M = Cr, Mn, Fe): An Ab Initio Investigation
The electronic and magnetic structures
of the tetragonal Cu<sub>2</sub>Sb-type 3d metal arsenides (M<sub>2</sub>As, M = Cr, Mn, Fe) were examined using density functional
theory to identify chemical influences on their respective patterns
of magnetic order. Each compound adopts a different antiferromagnetic
(AFM) ordering of local moments associated with the 3d metal sites,
but every one involves a doubled crystallographic <i>c</i>-axis. These AFM ordering patterns are rationalized by the results
of VASP calculations on several magnetically ordered models using <i>a</i> × <i>a</i> × 2<i>c</i> supercell.
Effective exchange parameters obtained from SPRKKR calculations indicate
that both direct and indirect exchange couplings play essential roles
in understanding the different magnetic orderings observed. The nature
of nearest-neighbor direct exchange couplings, that is, either ferromagnetic
(FM) or AFM, were predicted by analysis of the corresponding crystal
orbital Hamilton population (COHP) curves obtained by TB-LMTO calculations.
Interestingly, the magnetic structures of Fe<sub>2</sub>As and Mn<sub>2</sub>As show tetragonal symmetry, but a magnetostrictive tetragonal-to-orthorhombic
distortion could occur in Cr<sub>2</sub>As through AFM Cr1–Cr2
coupling between symmetry inequivalent Cr atoms along the <i>a</i>-axis, but FM coupling along the <i>b</i>-axis.
A LSDA+U approach is required to achieve magnetic moment values for
Mn<sub>2</sub>As in better agreement with experimental values, although
computations always predict the moment at the M1 site to be lower
than that at the M2 site. Finally, a rigid-band model applied to the
calculated DOS curve of Mn<sub>2</sub>As correctly assesses the magnetic
ordering patterns in Cr<sub>2</sub>As and Fe<sub>2</sub>As
Structure Transformation and Cerium-Substituted Optical Response across the Carbonitridosilicate Solid Solution (La<sub>δ</sub>Y<sub>1−δ</sub>)<sub>2</sub>Si<sub>4</sub>N<sub>6</sub>C (δ = 0–0.5)
Following an investigation proving
La<sub>2</sub>Si<sub>4</sub>N<sub>6</sub>C crystallizes in a monoclinic
space group, isostructural to Y<sub>2</sub>Si<sub>4</sub>N<sub>6</sub>C, the reportedly hexagonal (La<sub>0.5</sub>Y<sub>0.5</sub>)<sub>2</sub>Si<sub>4</sub>N<sub>6</sub>C was reinvestigated to examine
the apparent crystal structure change across the solid solution. Initially,
calculating the electronic structure and phonon density of states
of (La<sub>0.5</sub>Y<sub>0.5</sub>)<sub>2</sub>Si<sub>4</sub>N<sub>6</sub>C in the <i>P</i>6<sub>3</sub><i>mc</i> space group revealed an imaginary phonon mode, which is indicative
of a structural instability. Displacing the atoms along the pathway
of the imaginary vibration led to a previously unreported space group
for carbonitridosilicates, trigonal <i>P</i>31<i>c</i>. The assignment of the trigonal space group was subsequently confirmed
by synthesizing (La<sub>0.5</sub>Y<sub>0.5</sub>)<sub>2</sub>Si<sub>4</sub>N<sub>6</sub>C using high-temperature, solid state synthesis
and analyzing the crystal structure with high-resolution synchrotron
X-ray powder diffraction. Preparing the solid solution, (La<sub>δ</sub>Y<sub>1−δ</sub>)<sub>1.98</sub>Ce<sub>0.02</sub>Si<sub>4</sub>N<sub>6</sub>C (δ = 0–0.5), showed that the crystal
structure changes from the monoclinic to the trigonal space group
at δ ≈ 0.25. Finally, substituting Ce<sup>3+</sup> in
the crystal structure to investigate the optical response via steady-state
luminescent and photoluminescent quantum yield measurements reveals
severe luminescent quenching with increasing La<sup>3+</sup> content,
due to a combination of absorption of luminescence by the host structure
and thermal quenching. These results display the virtue of combining
computational and experimental techniques to solve inorganic crystal
structures and assess potential phosphor hosts
Predicting the Band Gaps of Inorganic Solids by Machine Learning
A machine-learning
model is developed that can accurately predict
the band gap of inorganic solids based only on composition. This method
uses support vector classification to first separate metals from nonmetals,
followed by quantitatively predicting the band gap of the nonmetals
using support vector regression. The superb accuracy of the regression
model is obtained by using a training set composed entirely of experimentally
measured band gaps and utilizing only compositional descriptors. In
fact, because of the unique training set of experimental data, the
machine learning predicted band gaps are significantly closer to the
experimentally reported values than DFT (PBE-level) calculated band
gaps. Not only does this resulting tool provide the ability to accurately
predict the band gap for any composition but also the versatility
and speed of the prediction based only on composition will make this
a great resource to screen inorganic phase space and direct the development
of functional inorganic materials
Producing Tunable Broadband Near-Infrared Emission through Co-Substitution in (Ga<sub>1–<i>x</i></sub>Mg<sub><i>x</i></sub>)(Ga<sub>1–<i>x</i></sub>Ge<sub><i>x</i></sub>)O<sub>3</sub>:Cr<sup>3+</sup>
Broadband near-infrared (NIR) phosphors are in high demand
for
creating “smart” NIR phosphor-converted light-emitting
diode (pc-LED) sources. In this work, a series of Cr3+-substituted
NIR-emitting materials with highly efficient, broad, tunable emission
spectra are achieved by modifying the simple oxide Ga2O3 using [Mg2+-Ge4+] and [Ga3+-Ga3+] co-unit substitution. The results show that the
emission peak can be shifted from 726 to 830 nm while maintaining
a constant excitation peak in the blue light region, enabling extensive
application. The optical properties stem from changes in the Cr3+ crystal field environment upon substitution. Intriguingly,
the temperature-dependent photoluminescence emission peak position
shows virtually no change in the [Mg2+-Ge4+]
co-substituted materials. This abnormal phenomenon is found to be
a comprehensive embodiment of a weakening crystal field environment
(red-shift) as the temperature increases and reduced local structure
distortion (blue-shift) with increasing temperature. The high quantum
yield, NIR emission, and net-zero emission shift as a function of
temperature make this phosphor class optimal for device incorporation.
As a result, their performance was studied by coating the phosphor
on a 450 nm emitting LED chip. The fabricated device demonstrates
an excellent NIR output power and NIR photoelectric conversion efficiency.
This study provides a series of efficient, tunable, broadband NIR
materials for spectroscopy applications and contributes to the basic
foundation of Cr3+-activated NIR phosphors
Iodine Anions beyond −1: Formation of Li<sub><i>n</i></sub>I (<i>n</i> = 2–5) and Its Interaction with Quasiatoms
Novel phases of Li<sub><i>n</i></sub>I (<i>n</i> = 2, 3, 4, 5) compounds are predicted
to form under high pressure
using first-principles density functional theory and an unbiased crystal
structure search algorithm. All of the phases identified are thermodynamically
stable with respect to decomposition into elemental Li and the binary
LiI at a relatively low pressure (≈20 GPa). Increasing the
pressure to 100 GPa yields the formation of a high pressure electride
where electrons occupy interstitial quasiatom (ISQ) orbitals. Under
these extreme pressures, the calculated charge on iodine suggests
the oxidation state goes beyond the conventional and expected −1
charge for the halogens. This strange oxidative behavior stems from
an electron transfer going from the ISQ to I<sup>–</sup> and
Li<sup>+</sup> ions as high pressure collapses the void space. The
resulting interplay between chemical bonding and the quantum chemical
nature of enclosed interstitial space allows this first report of
a halogen anion beyond a −1 oxidation state
Identifying a Structural Preference in Reduced Rare-Earth Metal Halides by Combining Experimental and Computational Techniques
The structures of two new cubic {TnLa<sub>3</sub>}Br<sub>3</sub> (Tn = Ru, Ir; <i>I</i>4<sub>1</sub>32, <i>Z</i> = 8; Tn = Ru: <i>a</i> = 12.1247(16) Å, <i>V</i> = 1782.4(4) Å<sup>3</sup>; Tn = Ir: <i>a</i> = 12.1738(19)
Å, <i>V</i> = 1804.2(5) Å<sup>3</sup>) compounds
belonging to a family of reduced rare-earth metal halides were determined
by single-crystal X-ray diffraction. Interestingly, the isoelectronic
compound {RuLa<sub>3</sub>}I<sub>3</sub> crystallizes in the monoclinic
modification of the {TnR<sub>3</sub>}X<sub>3</sub> family, while {IrLa<sub>3</sub>}I<sub>3</sub> was found to be isomorphous with cubic {PtPr<sub>3</sub>}I<sub>3</sub>. Using electronic structure calculations, a
pseudogap was identified at the Fermi level of {IrLa<sub>3</sub>}Br<sub>3</sub> in the new cubic structure. Additionally, the structure attempts
to optimize (chemical) bonding as determined through the crystal orbital
Hamilton populations (COHP) curves. The Fermi level of the isostructural
{RuLa<sub>3</sub>}Br<sub>3</sub> falls below the pseudogap, yet the
cubic structure is still formed. In this context, a close inspection
of the distinct bond frequencies reveals the subtleness of the structure
determining factors