INO
CNR
vai_a_storia   vai_a_organizzazione   vai_a_sedi   vai_a_personale   Area Riservata
    English English Version  
 
 

Melting dynamics of ice in the mesoscopic regime

  Articoli su Riviste JCR/ISI  (anno 2017)

Autori:  Citroni M., Fanetti S., Falsini N., Foggi P., Bini R

Affiliazione Autori:  aLENS–European Laboratory for Non-Linear Spectroscopy, 50019 Sesto, Florence, Italy; bDipartimento di Chimica Ugo Schiff, University of Florence, 50019 Sesto, Florence, Italy; cIstituto di Chimica dei Composti Organo Metallici, Consiglio Nazionale delle Ricerche, 50019 Sesto, Florence, Italy; dIstituto Nazionale di Ottica, Consiglio Nazionale delle Ricerche, 50125 Florence, Italy; and eDipartimento di Chimica, University of Perugia, I-06123 Perugia, Italy

Riassunto:  How does a crystal melt? How long does it take for melt nuclei to grow? The melting mechanisms have been addressed by several theoretical and experimental works, covering a subnanosecond time window with sample sizes of tens of nanometers and thus suitable to determine the onset of the process but unable to unveil the following dynamics. On the other hand, macroscopic observations of phase transitions, with millisecond or longer time resolution, account for processes occurring at surfaces and time limited by thermal contact with the environment. Here, we fill the gap between these two extremes, investigating the melting of ice in the entire mesoscopic regime. A bulk ice I-h or ice VI sample is homogeneously heated by a picosecond infrared pulse, which delivers all of the energy necessary for complete melting. The evolution of melt/ice interfaces thereafter is monitored by Mie scattering with nanosecond resolution, for all of the time needed for the sample to reequilibrate. The growth of the liquid domains, over distances of micrometers, takes hundreds of nanoseconds, a time orders of magnitude larger than expected from simple H-bond dynamics.

Rivista/Giornale:  PROCEEDINGS OF THE NATIONAL ACADEMY OF SCIENCES OF THE UNITED STATES OF AMERICA
Volume n.:  114 (23)      Pagine da: 5935  a: 5940
Ulteriori informazioni:  This work was supported by the Deep Carbon Observatory initiative (Extreme Physics and Chemistry of Carbon: Forms, Transformations, and Movements in Planetary Interiors, from the Alfred P. Sloan Foundation); by the Grant Futuro in Ricerca 2010 RBFR109ZHQ funded by the Italian Ministero dell
DOI: 10.1073/pnas.1620039114

*Impact Factor della Rivista: (2017) 9.504
data tratti da "WEB OF SCIENCE" (marchio registrato di Thomson Reuters) ed aggiornati a:  19/05/2019

Riferimenti visionabili in IsiWeb of Knowledge: (solo per sottoscrittori)
Per visualizzare la scheda dell'articolo su IsiWeb: Clicca qui

INO © Istituto Nazionale di Ottica - Largo Fermi 6, 50125 Firenze | Tel. 05523081 Fax 0552337755 - P.IVA 02118311006     P.E.C.    Info