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Featured researches published by V. M. Malavergne.


Geochimica et Cosmochimica Acta | 2001

Transition elements in water-bearing silicate glasses/melts. Part II. Ni in water-bearing glasses

François Farges; Manuel Munoz; Ralf Siewert; V. M. Malavergne; Gordon E. Brown; Harald Behrens; Marcus Nowak; Pierre-Emmanuel Petit

Abstract The local coordination environment around Ni(II) in a series of sodium trisilicate (NS3) and albitic (ALB) glasses has been evaluated by using high-resolution XANES and anharmonic EXAFS spectroscopies. The glasses contain ∼1000 to 4000 ppm of Ni and from 0 to 8.2 wt.% water. They were synthesized at pressures between 2.2 and 5 kbars and temperatures between 1050 and 1350 K. The bulk glasses were characterized by using X-ray diffraction, transmission electron microscopy, Raman, and ultraviolet-Vis-NIR spectroscopies. Both hydrous NS3 and ALB glasses show dominant amounts of Ni(II) in relatively regular 6-coordinated environments, in contrast with their anhydrous counterparts, where 5-coordinated Ni dominates. There are also significant differences in the average medium-range environment (2–3.5 A) around Ni between the anhydrous and hydrous glasses. In the ALB glasses, the presence of water in amounts >2 wt.% induces the formation of nanocrystallites, with an average diameter of ∼40 A and an atomic arrangement similar to that of nepouite ([6]Ni3Si2O5(OH)4) or Ni-talc ([6]Ni3Si4O10(OH)2) or a related hydrous Ni-silicate. The presence of Ni-bearing nanocrystallites is thought to be due to the relatively slow quench rate of the high-temperature–high-pressure synthesis apparatus used. These nanophases are difficult to detect by using conventional characterization methods and can cause misleading interpretations of the glass structure if not detected. In contrast, there is no evidence for Ni-rich, nanocrystalline domains in NS3 glasses containing high water contents (up to 8.2 wt.%); instead, two to three Si second neighbors are observed around Ni in all NS3 glasses (and in ALB glasses with water contents Our results for Ni combined with results from other studies of 3-d divalent transition metal cations in hydrous silicate glasses suggest that water in silicate melts helps these cations form their preferred coordination environments [6-coordinated for Mn(II), Fe(II), and Ni(II)]. Ni(II) may occur in natural hydrous silicate melts dominantly in 6-coordinated environments, rather than dominantly in 4-coordinated environments, as in anhydrous melts and supercritical aqueous fluids, explaining the compatible behavior of Ni in magmas. However, in situ experiments are required to test this suggestion.


High Pressure Research | 2007

In situ mapping of high-pressure fluids using hydrothermal diamond anvil cells

H. Bureau; B. Ménez; V. M. Malavergne; Andrea Somogyi; A. Simionovici; Dominique Massare; H. Khodja; Laurent Daudin; J.-P. Gallien; Cliff S. J. Shaw; M. Bonnin-Mosbah

We present new results combining high pressures and temperatures attainable in a diamond anvil cell with in situ synchrotron radiation induced micro-X-ray fluorescence measurements. Hydrothermal diamond anvil cells experiments have been performed by measuring the partitioning of Pb between aqueous fluids (pure water or NaCl-enriched water) and hydrous silicate melts of haplogranite composition using synchrotron X-ray fluorescence. The in situ measurements were performed in the range 0.3–1.2 GPa and 730–850 °C both in the aqueous fluid and in the silicate melts being in equilibrium. Pb is strongly partitioned into high-pressure–temperature hydrous melts when Cl is present in either the hydrous melt or the aqueous fluid. Moreover, our comparisons of in situ results with post-mortem results show that significant changes take place during rapid quenching especially when samples are small (few hundred of microns in diameter). Water exsolution is induced by the quench in the silicate melt showing the high mobility of Pb which immediately partitions into the water vapor phase during the quench. The current in situ approach offers thus a pertinent complementary method to the classical experimental petrology investigations.


High Pressure Research | 2006

X-ray transmission properties of intelligent anvils in diamond anvil cells

M. Burchard; S. Kubsky; H. Bureau; Andrea Somogyi; V. M. Malavergne; B. Ménez; Manuel Munoz

High-pressure and/or high-temperature analysis of geo- and material science samples routinely employs diamond anvil cells (DACs) as a research instrument. In particular, DACs allow for various in situ characterizations (e.g. Raman and Fourier transform infra red spectroscopies, X-ray diffraction (XRD), X-ray spectroscopy including fluorescence (XRF) and absorption (XAS)) at elevated pressure and temperature. The measurement of pressure (P) and/or temperature (T) in the sample chamber is crucial, but not always accurate, more specifically in the case of low-pressure applications (a few GPa). The development of modified diamonds (intelligent anvils ‘i-anvils’) adapted to a new generation of DACs (intelligent diamond anvil cells: iDAC) can contribute to solve this problem, as the diamond itself serves as the PT sensor, being prepared, for example, by high-energy ion implantation [H. Bureau, M. Burchard, S. Kubsky et al., This volume (2006).] on a micrometric scale. Several most interesting measurement methods used with DACs are based on X-ray techniques (e.g. XRF, XRD, XAS). We present the first results of X-ray transmission measurements with iDACs, performed at the hard-X-ray microfocus beamline ID22 at the ESRF (European Synchrotron Radiation Facility), Grenoble, France. Sensor response to intense irradiation as a function of X-ray energy (E ph∈10;18.1 keV) was investigated. The values of the sensor were found to be independent of the irradiation in the investigated energy range and thus validate the use of these sensors for precise and reliable measurements on a wide range of applications with high-energy synchrotron radiation. No influence of the sensor on the X-ray transmission properties of the anvil has been found.


Meteoritics & Planetary Science | 2001

Description of new shock-induced phases in the Shergotty, Zagami, Nakhla and Chassigny meteorites

V. M. Malavergne; François Guyot; Karim Benzerara; Isabelle Martinez


Chemical Geology | 2006

Structural environment of iron in hydrous aluminosilicate glass and melt-evidence from X-ray absorption spectroscopy

Max Wilke; Christian Schmidt; François Farges; V. M. Malavergne; Laurent Gautron; A. Simionovici; Matthias Hahn; Pierre-Emanuel Petit


Physics of the Earth and Planetary Interiors | 2007

Potassium partitioning into molten iron alloys at high-pressure: Implications for Earth's core

Mohamed Ali Bouhifd; Laurent Gautron; Nathalie Bolfan-Casanova; V. M. Malavergne; T. Hammouda; Denis Andrault; Andrew P. Jephcoat


Physics of the Earth and Planetary Interiors | 2004

The behaviour of sulphur in metal–silicate core segregation experiments under reducing conditions

J. Siebert; V. M. Malavergne; François Guyot; Rossana Combes; Isabelle Martinez


Physica Scripta | 2005

In situ speciation of nickel in hydrous melts exposed to extreme conditions.

Manuel Munoz; H. Bureau; V. M. Malavergne; Benedicte Menez; Max Wilke; Christian Schmidt; A. Simionovici; Andrea Somogyi; François Farges


Archive | 2007

Formation of CaS-MgS in Enstatite Chondrites and Achondrites as a Function of Redox Conditions and Temperature: Constraints on Their Evolution in a Planetesimal and in a Proto-planet

V. M. Malavergne; Sophie Berthet; Kevin Righter


Archive | 2005

Uranium and Lead in the Early Planetary Core Formation: New Insights Given by High Pressure and Temperature Experiments

V. M. Malavergne; M. Tarrida; Robert David Combes; H. Bureau

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Andrea Somogyi

European Synchrotron Radiation Facility

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A. Simionovici

École normale supérieure de Lyon

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Manuel Munoz

University of Marne-la-Vallée

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Dominique Massare

Centre national de la recherche scientifique

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François Farges

Centre national de la recherche scientifique

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François Guyot

Institut de Physique du Globe de Paris

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J. Siebert

Institut de Physique du Globe de Paris

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