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SYNTHESIS, STRUCTURAL CHARACTERIZATION, AND HIRSHFELD SURFACE ANALYSIS OF AgCd2InSe4: A NEW MEMBER OF THE I-II2-III-VI4 CHALCOGENIDE FAMILY

  • Gerzon E. Delgado
  • , Jonathan Cisterna
  • , Eugenio Quintero
  • , Rosmary Guillén-Guillén
  • , Cecilia Chacón
  • , Gustavo Marroquin
  • , Gerson Márquez

Producción científica: Artículo CientíficoArtículo originalrevisión exhaustiva

Resumen

A new quaternary chalcogenide compound, AgCd2InSe4, belonging to the I-II2-III-VI4 family of diamond-like semiconductors, has been synthesized using the melt and annealing technique. The stoichiometric composition was confirmed by energy-dispersive X-ray spectroscopy (EDS), yielding elemental ratios consistent with the nominal 1:2:1:4 proportions. Powder X-ray diffraction (PXRD) data revealed a single-phase material with an orthorhombic crystal structure and successfully refined using the Rietveld method in the Pmn21 space group with unit cell parameters a = 8.5817(6) Å, b = 7.4099(9) Å, c = 6.9953(6) Å, and V = 444.83(7)(5) Å3. This quaternary compound crystallizes in a wurtzite-stannite structure where tetrahedrally coordinated cations (Ag+, Cd2+, In3+) and anions (Se2–) form a three-dimensional honeycomb structure. Interatomic distances suggest enhanced ionic contributions to bonding, consistent with other related chalcogenides. A Hirshfeld surface analysis (HSA) indicates that the most important contributions to the crystal packing are from Cd-Se (39.4%), In-Se (31.93%), and Ag-Se (19.9%) interactions, suggesting that the Ag+ ion is the most labile species and making this material a promising candidate for applications requiring fast ion transport. Additionally, Debye temperature and heat capacity estimations point to soft lattice dynamics, indicating potential for use in thermoelectric and optoelectronic devices.

Idioma originalInglés estadounidense
-607
PublicaciónRomanian Journal of Physics
Volumen71
N.º3-4
DOI
EstadoIndizado - 2026
Publicado de forma externa

Nota bibliográfica

Publisher Copyright:
© 2026, Publishing House of the Romanian Academy. All rights reserved.

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