First interstellar detection of HNSO with column density (8 ± 1)×10^13 cm^{-2} and abundance ~6×10^{-10} relative to H2, proposed to form via NSO + H on icy grains.
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8 Pith papers cite this work. Polarity classification is still indexing.
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representative citing papers
First analytic nuclear gradients derived and implemented for BSE@G0W0, validated on excited-state geometries and adiabatic energies against wavefunction benchmarks.
MP2SS reduces finite-size errors in periodic MP2 to millihartree accuracy at coarser k-point meshes for gapped systems via auxiliary function subtraction.
Experiments reveal that hydrogen plays a central role in forming SiC2, the key precursor to silicon carbide nanodust in carbon-rich stars.
The designed ternary liquid crystal mixture stabilizes a broad antiferroelectric SmC_A* phase, vitrifies the hexatic SmX_A* phase, and shows evidence of altered molecular organization between SmC* and SmC_A* phases based on X-ray, dielectric, and calorimetric data.
New spectroscopic measurements of 13CH3CN and CH3^13CN up to v8=2 yield precise l-component energy spacings of 22.93 and 21.79 cm^{-1} from perturbations and enable targeted searches in star-forming regions.
Electron capture at zigzag edges stabilizes armchair GNRs, eliminates spin polarization in the ground state, and induces Fermi level pinning with valence and conduction band slopes of approximately 0.1 and 0.9.
Cooling rate controls whether 10OS5 forms glass or crystallizes into conformationally disordered Cr1/Cr2 phases whose cold-crystallization energy output can be tuned by thermal history.
citing papers explorer
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Discovery of thionylimide, HNSO, in space: the first N-, S- and O-bearing interstellar molecule
First interstellar detection of HNSO with column density (8 ± 1)×10^13 cm^{-2} and abundance ~6×10^{-10} relative to H2, proposed to form via NSO + H on icy grains.
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Fully Analytic Nuclear Gradients for the Bethe--Salpeter Equation
First analytic nuclear gradients derived and implemented for BSE@G0W0, validated on excited-state geometries and adiabatic energies against wavefunction benchmarks.
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Reduction of finite-size effects for second-order M{\o}ller-Plesset perturbation theory with singularity subtraction
MP2SS reduces finite-size errors in periodic MP2 to millihartree accuracy at coarser k-point meshes for gapped systems via auxiliary function subtraction.
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The Significant Role of Hydrogen in the Formation of Silicon Carbide in Evolved Stars
Experiments reveal that hydrogen plays a central role in forming SiC2, the key precursor to silicon carbide nanodust in carbon-rich stars.
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Ternary liquid crystalline mixture showing broad antiferroelectric smectic C$_A$* and glassy hexatic smectic X$_A$* phases
The designed ternary liquid crystal mixture stabilizes a broad antiferroelectric SmC_A* phase, vitrifies the hexatic SmX_A* phase, and shows evidence of altered molecular organization between SmC* and SmC_A* phases based on X-ray, dielectric, and calorimetric data.
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Rotational Spectroscopy as a Tool to Study Vibration-Rotation Interaction: Investigations of $^{13}$CH$_3$CN and CH$_3$$^{13}$CN up to $v_8 = 2$ and a Search for $v_8 = 2$ Transitions toward Sagittarius B2(N)
New spectroscopic measurements of 13CH3CN and CH3^13CN up to v8=2 yield precise l-component energy spacings of 22.93 and 21.79 cm^{-1} from perturbations and enable targeted searches in star-forming regions.
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Electron enrichment of zigzag edges of armchair-oriented graphene nano-ribbons increases their stability and induces pinning of Fermi level
Electron capture at zigzag edges stabilizes armchair GNRs, eliminates spin polarization in the ground state, and induces Fermi level pinning with valence and conduction band slopes of approximately 0.1 and 0.9.
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Competing crystallization pathways and cold crystallization kinetics in 10OS5 liquid crystal
Cooling rate controls whether 10OS5 forms glass or crystallizes into conformationally disordered Cr1/Cr2 phases whose cold-crystallization energy output can be tuned by thermal history.