Monica Pozzo

Dr. Monica Pozzo

Department of Earth Sciences, University College London, Gower Street, London WC1E 6BT, UK
orcid

Research Focus & Metrics

Academic Career Length

31Years (1996-Present)

(Calculated once Scilit publication data is synced: current year − year of first publication + 1)

Representative Publications

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11 April 2012 in Nature
Verified
Journal Article
Closed access
MPMonica Pozzo
Monica Pozzo
CDChris Davies
Chris Davies
DGDavid Gubbins
David Gubbins
DADario Alfè
Dario Alfè

1 February 2009 in International Journal of Hydrogen Energy
Verified
Journal Article
Closed access
MPMonica Pozzo
Monica Pozzo
DAD. Alfè
D. Alfè

22 September 2009 in The Astrophysical Journal
Verified
Journal Article
Closed access
RKRubina Kotak
Rubina Kotak
WMW. P. S. Meikle
W. P. S. Meikle
DFD. Farrah
D. Farrah
CGC. L. Gerardy
C. L. Gerardy
RFR. J. Foley
R. J. Foley
JWJ. C. Wheeler
J. C. Wheeler

12 October 2009 in Physical Review Letters
Verified
Journal Article
Closed access
PDF file
PLPaolo Lacovig
Paolo Lacovig
MPMonica Pozzo
Monica Pozzo
DADario Alfè
Dario Alfè
PVPaolo Vilmercati
Paolo Vilmercati
ABAlessandro Baraldi
Alessandro Baraldi
SLSilvano Lizzit
Silvano Lizzit
By combining high-resolution photoelectron spectroscopy and ab initio calculations, we show that carbon nanoislands formed during the growth of a long-range ordered graphene layer on Ir(111) assume a peculiar domelike shape. The understanding of the unusual growth mechanism of these C clusters, which represent an intermediate phase between the strongly coupled carbidic carbon and a quasi-free-standing graphene layer, can provide information for a rational design of graphenelike systems at the nanoscale.

22 January 2013 in Physical Review B
Verified
Journal Article
Closed access
MPMonica Pozzo
Monica Pozzo
CDChris Davies
Chris Davies
DGDavid Gubbins
David Gubbins
DADario Alfè
Dario Alfè
We report on the thermal and electrical conductivities of two liquid silicon-oxygen-iron mixtures (Fe${}_{0.82}$Si${}_{0.10}$O${}_{0.08}$ and Fe${}_{0.79}$Si${}_{0.08}$O${}_{0.13}$), representative of the composition of the Earth's outer core at the relevant pressure-temperature conditions, obtained from density functional theory calculations with the Kubo-Greenwood formulation. We find thermal conductivities $k=100(160)$ W m${}^{$-${}1}$ K${}^{$-${}1}$, and electrical conductivities $$\sigma${}=1.1(1.3)\ifmmode\times\else\texttimes\fi{}{10}^{6}\phantom{\rule{0.28em}{0ex}}{$\Omega${}}^{$-${}1}$ m${}^{$-${}1}$ at the top (bottom) of the outer core. These values are between two and three times higher than previous estimates, and have important implications for our understanding of the Earth's thermal history and the functioning of the Earth's magnetic field, including rapid cooling rate for the whole core or high level of radiogenic elements in the core. We also show results for a number of structural and dynamic properties of the mixtures, including the partial radial distribution functions, mean square displacements, viscosities, and speeds of sound.

1 August 2004 in Monthly Notices of the Royal Astronomical Society
Verified
Journal Article
Open access
PDF file
MPMonica Pozzo
Monica Pozzo
WMW. P. S. Meikle
W. P. S. Meikle
AFA. Fassia
A. Fassia
TGT. Geballe
T. Geballe
PLP. Lundqvist
P. Lundqvist
JSJ. Sollerman
J. Sollerman
We present late-time near-infrared (NIR) and optical observations of the Type IIn SN 1998S. The NIR photometry spans 333–1242 d after explosion, whil