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Ru‐P Nanoalloy from Elemental Phosphorus as P‐Source
Matteo Vanni, Giacomo Provinciali, Fuencisla Delgado Calvo, Elisa Carignani, Sébastien Dreyfuss, Nicolas Mézailles, Antonio Massimiliano Mio, Giuseppe Nicotra, Stefano Caporali, Silvia Borsacchi, Maurizio Peruzzini, Maria Caporali

Ru‐P Nanoalloy from Elemental Phosphorus as P‐Source

Science & Mathematics Published 2022 Verification Pending

Overview & Synopsis

Binary ruthenium-phosphorus nanoparticles (NPs) with different Ru/P ratio were prepared in mild conditions using white phosphorus (P4) as phosphorus source. Accurate study of both their morphology and structure at the atomic level by TEM and HAADF-STEM, respectively, showed that Ru2P and RuP have a narrow size distribution (ca. 3.3 nm) and are lacking an ordered ruthenium phosphide lattice. 31 P Solid State NMR highlighted the existence of three different phosphorus species consistently with the lack of a metal phosphide lattice and finally XPS revealed that the true nature of these nanoparticles can be better described as a ruthenium-phosphorus alloy. As a benchmark test, the selective hydrogenation of nitroarenes to primary aromatic amines was studied and evidenced how the P-alloying imparts a surface modification resulting in a higher catalytic activity and excellent chemoselectivity of Ru2P in comparison to Ru(0) and RuP.

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Document Information

Document Title Ru‐P Nanoalloy from Elemental Phosphorus as P‐Source
Author / Organization Matteo Vanni, Giacomo Provinciali, Fuencisla Delgado Calvo, Elisa Carignani, Sébastien Dreyfuss, Nicolas Mézailles, Antonio Massimiliano Mio, Giuseppe Nicotra, Stefano Caporali, Silvia Borsacchi, Maurizio Peruzzini, Maria Caporali
Subject & Discipline Multidisciplinary Academic Open Research
Categories Science & Mathematics
Publication Year 2022
License / Rights Open Access / Creative Commons
Resource Verification Listed PDF (Verification Pending)
Original Host Website HAL Open Science (hal.science)
File Format application/pdf (Portable Document Format)
Language EN
Catalog ID DOC-254659
Original Source Link Visit Source Page on hal.science »