Centrosymmetric to noncentrosymmetric structure transition of the RbREP2Se6 (RE = La–Nd, Sm, Ho–Yb) series: crystal growth, magnetic and optical properties

Abstract

Rare-earth (RE) chalcophosphates have attracted considerable attention as infrared nonlinear optical (NLO) materials. Herein, nine single crystals of quaternary rare-earth containing selenophosphates, RbREP2Se6 (RE = La–Nd, Sm, Ho–Yb) were synthesized using the RbI flux assisted boron chalcogen mixture (BCM) method. The compounds RbREP2Se6 (RE = La–Pr) crystallize in the monoclinic crystal system with the P21/c space group, whereas RbREP2Se6 (RE = Nd, Sm, Ho–Yb) crystallize in the orthorhombic crystal system with the P212121 space group. In the RbREP2Se6 (RE = La–Pr) series, the structure is composed of [REP2Se6] layers formed by interconnected RESe9 distorted capped square antiprism and P2Se6 dimers, while in the RbREP2Se6 (RE = Nd, Sm, Ho–Yb) series, [REP2Se6] layers consist of RESe8 bicapped trigonal prisms and P2Se6 dimers. Polycrystalline powders of all the title compounds were also obtained for property measurements. Magnetic property measurements of RbREP2Se6 (RE = Nd, Er, and Yb), were collected over the 2–300 K temperature range, which revealed paramagnetic behavior with small negative Weiss constants. The bandgaps of RbREP2Se6 (RE = Nd, and Sm) were determined from UV-vis diffuse reflectance measurements. Second Harmonic Generation (SHG) measurements of RbREP2Se6 (RE = Nd, and Sm) polycrystalline samples exhibited an efficiency of ∼0.67 × AgGaS2, and ∼3.65 × AgGaS2 respectively.

Graphical abstract: Centrosymmetric to noncentrosymmetric structure transition of the RbREP2Se6 (RE = La–Nd, Sm, Ho–Yb) series: crystal growth, magnetic and optical properties

Supplementary files

Article information

Article type
Paper
Submitted
30 Jan 2026
Accepted
05 Mar 2026
First published
06 Mar 2026

Dalton Trans., 2026, Advance Article

Centrosymmetric to noncentrosymmetric structure transition of the RbREP2Se6 (RE = La–Nd, Sm, Ho–Yb) series: crystal growth, magnetic and optical properties

H. B. Kashem, M. A. A. Muhit, H. E. Smith, E. A. Gabilondo, P. S. Halasyamani and H. zur Loye, Dalton Trans., 2026, Advance Article , DOI: 10.1039/D6DT00254D

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