Halide perovskites are soft, ionic semiconductors with exceptional optoelectronic properties. They typically have direct bandgaps in the visible spectrum that can be tuned by composition. For example, MAPbI₃ has a direct bandgap of about 1.5–1.6 eV, while replacing I⁻ by Br⁻ or Cl⁻ raises the gap to approximately 2.3 eV (green emission) or about 3.0 eV (blue) respectively. Depending on the halide used, the band gap can be tuned from around 1.6 eV (I) to approximately 3.2 eV (Cl). Mixed-halide perovskites allow continuous tuning across this range.
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For example, MAPbI₃ crystallizes in a tetragonal perovskite structure at room temperature, consisting of PbI₆ octahedra sharing corners, with MA⁺ cations occupying the interstitial spaces. Variants of the perovskite structure also exist: for instance, layered (2D) perovskites have alternating organic and inorganic sheets (formula A₂BX₄), and “double” perovskites (e.g. A₂BB′X₆) replace Pb²⁺ by a combination of a monovalent and trivalent cation to eliminate lead. However, the defining feature of halide perovskites is the 3D corner-sharing BX₆ framework with monovalent A ions in the cavities
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Ideal halide perovskites adopt a cubic ABX₃ lattice (space group Pm3̅m ), but most undergo distortions (to tetragonal or orthorhombic symmetry) as a function of temperature, composition and ionic sizes. In the cubic form the B cation is octahedrally coordinated (6-fold) by X, and the A cation sits in a 12-fold cuboctahedral site formed by the vertices of eight adjacent BX₆ octahedra. (This can be quantified by the Goldschmidt tolerance factor t = (r_A + r_X) / √2(r_B + r_X), which must be ≈0.8–1 for a stable perovskite.)
Halide perovskites - Non-Elaborate Posts - Post 1
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Halide perovskites are crystalline semiconductors of the general formula ABX₃ , where A is a monovalent organic or inorganic cation (e.g. methylammonium CH₃NH₃⁺ (MA), formamidinium HC(NH₂)₂⁺ (FA), Cs⁺), B is a divalent metal cation (most commonly Pb²⁺ or Sn²⁺), and X is a halide anion (Cl⁻, Br⁻, I⁻). In these materials the B-site cation is surrounded by six halide anions to form a BX₆ octahedron, and the A cations occupy the cavities between the corner-sharing octahedral This ABX₃ motif is derived from the same perovskite structure as CaTiO₃, but with oxygen replaced by a halide. For example, CH₃NH₃PbI₃ (MAPbI₃) consists of a 3D network of PbI₆ octahedra with CH₃NH₃⁺ in the interstitial cuboctahedral sites. Common A‐site ions include MA⁺, FA⁺ or Cs⁺; B‐site is typically Pb²⁺ or Sn²⁺; and X is I⁻, Br⁻ or Cl⁻.
Solubility of Sucrose Ethanol - Nuclear Chemistry Topics - Non-Elaborate Posts - Post 5
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Rich imagery helps: the nucleus as a million-year clock; decay as slow erosion; unstable isotopes as ephemeral ghosts of atoms, appearing for a moment then fading; gamma rays as invisible sunbeams, radiant yet dangerous. A book like The Disappearing Spoon traces those scientific curves and human curves together: discoverers, mistakes, triumphs, consequences. It teaches that nuclear chemistry is not just about energy levels, decay constants, or cross-sections — it is about what we, as humans, do with knowledge of the atom, how we shape it, fear it, hope from it.
Solubility of Sucrose Ethanol - Nuclear Chemistry Topics - Non-Elaborate Posts - Post 4
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To understand this, one must grapple with the nuclear binding energy curve — the tug-of-war between protons’ repulsion and the strong nuclear force; the magic of shell closures; the grace of stability at certain “magic numbers” of nucleons. And one must trace how we produce isotopes: in stars that burn lighter elements into heavier ones, in labs with particle accelerators, reactors, cosmic rays crashing in meteorites.
Solubility of Sucrose Ethanol - Nuclear Chemistry Topics - Non-Elaborate Posts - Post 3
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Usage of a bit of a parallel post In nuclear chemistry, certain isotopes are like solutes trying to dissolve in an unforgiving medium called “ground state, ambient conditions.” Some isotopes are “soluble” — stable, long-lived, found in nature. Others are “insoluble” — they decay quickly, they cannot persist without external energy or intervention. Just as sucrose flounders in ethanol at room temperature, existing only in minuscule amounts (≈ 0.5–0.6 g per 100 mL ethanol), many would-be isotopes flounder in the ambient universe — they are energetically disfavored, or quickly decay via alpha, beta, or gamma emission.