Effects of Hydrostatic Pressure on the Surface Plasmon Resonance of Gold Nanocrystals.

bulk modulus gold nanoparticles hydrostatic pressure optical absorption refractive index surface plasmon resonance

Journal

ACS nano
ISSN: 1936-086X
Titre abrégé: ACS Nano
Pays: United States
ID NLM: 101313589

Informations de publication

Date de publication:
22 Jan 2019
Historique:
pubmed: 20 12 2018
medline: 20 12 2018
entrez: 20 12 2018
Statut: ppublish

Résumé

The surface plasmon resonances of gold nanospheres and nanorods have been measured as a function of hydrostatic pressure up to 17 GPa in methanol-ethanol 4:1 solvent and up to 10 GPa in paraffin. Both the sphere resonance and the longitudinal rod resonance exhibit redshifts, whereas the transverse rod mode shows an extremely weak redshift or blueshift depending on the nanorod aspect ratio. Solidification of the solvent around 11 GPa causes some aggregation of the particles, readily identified through broadening of the surface plasmon band and further redshifting. Spectra collected during loading and unloading cycles exhibit only minimal hysteresis if the pressure remains below 11 GPa. The surface plasmon shifts are the result of two competing effects. Compression of the conduction electrons in the metals increases the bulk plasma frequency, which causes a blueshift. However, the increase in the solvent density under hydrostatic load leads to an increase in the solvent refractive index, which in turn leads to a redshift. We find that after accounting for the solvent contribution, we can spectroscopically determine the bulk modulus of the gold nanoparticles with a precision of 10%. The value obtained of K

Identifiants

pubmed: 30563343
doi: 10.1021/acsnano.8b07104
doi:

Types de publication

Journal Article

Langues

eng

Pagination

498-504

Auteurs

Camino Martín-Sánchez (C)

Malta Consolider Team, DCITIMAC, Facultad de Ciencias , University of Cantabria , Santander 39005 , Spain.

José Antonio Barreda-Argüeso (JA)

Malta Consolider Team, DCITIMAC, Facultad de Ciencias , University of Cantabria , Santander 39005 , Spain.

Susanne Seibt (S)

ARC Centre of Excellence in Exciton Science, School of Chemistry , University of Melbourne , Parkville , Victoria 3010 , Australia.

Paul Mulvaney (P)

ARC Centre of Excellence in Exciton Science, School of Chemistry , University of Melbourne , Parkville , Victoria 3010 , Australia.

Fernando Rodríguez (F)

Malta Consolider Team, DCITIMAC, Facultad de Ciencias , University of Cantabria , Santander 39005 , Spain.

Classifications MeSH