Coverage-dependent structural evolution of CoBr2 at the Au(111) interface
Identifikátory výsledku
Kód výsledku v IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F25%3A00643495" target="_blank" >RIV/68378271:_____/25:00643495 - isvavai.cz</a>
Výsledek na webu
<a href="https://hdl.handle.net/11104/0373433" target="_blank" >https://hdl.handle.net/11104/0373433</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1002/advs.202508262" target="_blank" >10.1002/advs.202508262</a>
Alternativní jazyky
Jazyk výsledku
angličtina
Název v původním jazyce
Coverage-dependent structural evolution of CoBr2 at the Au(111) interface
Popis výsledku v původním jazyce
Unraveling the growth mechanism of van der Waals materials is crucial for their device implementation, as this improves the overall film quality, allowing precise control of their electronic and magnetic properties in nanoscale applications. The initial structure formed on the substrate during growth is often assumed to be bulk-like, thereby neglecting the role of the surface in the assembly. Here, the coverage–dependent growth of CoBr2 on Au(111) from a stoichiometric molecular powder is studied using a combination of experimental techniques, machine–learning-driven molecular dynamics simulations and density functional theory calculations. It is found that CoBr2 molecules initially form a molecular precursor phase characterized by three-molecule clusters arranged in a surface–stabilized structure with long-range order and a periodic coincidence with Au(111). As the surface coverage is increased, this phase subsequently undergoes a transition to form the equilibrium van der Waals crystal layered structure observed for the bulk material. These findings challenge conventional views of direct van der Waals layer formation and provide new insight into the role of the substrate during the growth process.n
Název v anglickém jazyce
Coverage-dependent structural evolution of CoBr2 at the Au(111) interface
Popis výsledku anglicky
Unraveling the growth mechanism of van der Waals materials is crucial for their device implementation, as this improves the overall film quality, allowing precise control of their electronic and magnetic properties in nanoscale applications. The initial structure formed on the substrate during growth is often assumed to be bulk-like, thereby neglecting the role of the surface in the assembly. Here, the coverage–dependent growth of CoBr2 on Au(111) from a stoichiometric molecular powder is studied using a combination of experimental techniques, machine–learning-driven molecular dynamics simulations and density functional theory calculations. It is found that CoBr2 molecules initially form a molecular precursor phase characterized by three-molecule clusters arranged in a surface–stabilized structure with long-range order and a periodic coincidence with Au(111). As the surface coverage is increased, this phase subsequently undergoes a transition to form the equilibrium van der Waals crystal layered structure observed for the bulk material. These findings challenge conventional views of direct van der Waals layer formation and provide new insight into the role of the substrate during the growth process.n
Klasifikace
Druh
J<sub>imp</sub> - Článek v periodiku v databázi Web of Science
CEP obor
—
OECD FORD obor
10302 - Condensed matter physics (including formerly solid state physics, supercond.)
Návaznosti výsledku
Projekt
Výsledek vznikl pri realizaci vícero projektů. Více informací v záložce Projekty.
Návaznosti
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Ostatní
Rok uplatnění
2025
Kód důvěrnosti údajů
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Údaje specifické pro druh výsledku
Název periodika
Advanced Science
ISSN
2198-3844
e-ISSN
2198-3844
Svazek periodika
12
Číslo periodika v rámci svazku
47
Stát vydavatele periodika
US - Spojené státy americké
Počet stran výsledku
8
Strana od-do
e08262
Kód UT WoS článku
001614369800001
EID výsledku v databázi Scopus
2-s2.0-105021805405