Isabelle Daniel

Isabelle Daniel

orcid

Research Focus & Metrics

Academic Career Length

36Years (1991-Present)

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

Representative Publications

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21 December 2007 in Science
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NHNadege Hilairet
Nadege Hilairet
BRBruno Reynard
Bruno Reynard
YWYanbin Wang
Yanbin Wang
IDIsabelle Daniel
Isabelle Daniel
SMSébastien Merkel
Sébastien Merkel
SPSylvain Petitgirard
Sylvain Petitgirard
The supposed low viscosity of serpentine may strongly influence subduction-zone dynamics at all time scales, but until now its role could not be quantified because measurements relevant to intermediate-depth settings were lacking. Deformation experiments on the serpentine antigorite at high pressures and temperatures (1 to 4 gigapascals, 200° to 500°C) showed that the viscosity of serpentine is much lower than that of the major mantle-forming minerals. Regardless of the temperature, low-viscosity serpentinized mantle at the slab surface can localize deformation, impede stress buildup, and limit the downdip propagation of large earthquakes at subduction zones. Antigorite enables viscous relaxation with characteristic times comparable to those of long-term postseismic deformations after large earthquakes and slow earthquakes. Antigorite viscosity is sufficiently low to make serpentinized faults in the oceanic lithosphere a site for subduction initiation.

29 August 2006 in Chemical Society Reviews
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IDIsabelle Daniel
Isabelle Daniel
POPhilippe M Oger
Philippe M Oger
RWRoland Winter
Roland Winter
Life on Earth can be traced back to as far as 3.8 billion years (Ga) ago. The catastrophic meteoritic bombardment ended between 4.2 and 3.9 Ga ago. Therefore, if life emerged, and we know it did, it must have emerged from nothingness in less than 400 million years. The most recent scenarios of Earth accretion predict some very unstable physico-chemical conditions at the surface of Earth, which, in such a short time period, would impede the emergence of life from a proto-biotic soup. A possible alternative would be that life originated in the depth of the proto-ocean of the Hadean Earth, under high hydrostatic pressure. The large body of water would filter harmful radiation and buffer physico-chemical variations, and therefore would provide a more stable radiation-free environment for pre-biotic chemistry. After a short introduction to Earth history, the current tutorial review presents biological and physico-chemical arguments in support of high-pressure origin for life on Earth.

1 June 2004 in Physics and Chemistry of Minerals
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AAA.-L. Auzende
A.-L. Auzende
IDIsabelle Daniel
Isabelle Daniel
BRB. Reynard
B. Reynard
CLC. Lemaire
C. Lemaire
FGF. Guyot
F. Guyot

7 August 2010 in Journal of Geophysical Research
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ARAngèle Ricolleau
Angèle Ricolleau
JPJean-Philippe Perrillat
Jean-Philippe Perrillat
GFGuillaume Fiquet
Guillaume Fiquet
IDIsabelle Daniel
Isabelle Daniel
JMJan Matas
Jan Matas
NGNicolas Guignot
Nicolas Guignot


1 May 2014 in Geochimica et Cosmochimica Acta
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Journal Article
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SFSébastien Facq
Sébastien Facq
IDIsabelle Daniel
Isabelle Daniel
GMGilles Montagnac
Gilles Montagnac
HCHervé Cardon
Hervé Cardon
DSDimitri A. Sverjensky
Dimitri A. Sverjensky