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C. Hebert

Publications and source records attributed to C. Hebert.

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Precipitation in lean Mg-Zn-Ca alloys

While lean Mg-Zn-Ca alloys are promising materials for temporary implants, questions remain on the impact of Zn and Ca. In this context, the precipitation in Mg-1.5Zn-0.25Ca (ZX20, in wt.%) was investigated upon linear heating from about room temperature to 400 C, with a particular focus on the debated ternary precipitate phase. Three exothermic differential scanning calorimetry (DSC) peaks were observed at 125, 250 and 320 C. The microstructure at the end of these peaks (205, 260 and 350 C) was probed in a multiscale correlative approach using atom probe tomography (APT) and transmission electron microscopy (TEM). At 205 C, APT analysis revealed Ca-rich, Zn-rich and Zn-Ca-rich clusters of about 3 nm in size and with a number density of 5.7 x 10^23 m^-3. At 260 C, APT and TEM showed mono-layered Zn-Ca-rich Guinier-Preston (GP) zones of about 8 nm in size and with a number density of 1.3 x 10^23 m^-3. At 350 C, there are larger, highly coherent elongated precipitates of about 50 nm in size, in a lower number density, and of two types: either binary Mg2Ca precipitates or less numerous ternary Ca2Mg6Zn3 precipitates, as deduced from scanning TEM-based energy dispersive X-ray spectrometry (EDS) and nanodiffraction in TEM. The highest hardening, probed by Vickers testing, relates to the end of the 125 C DSC peak and thus to GP zones, which outperform the hardening induced by the nanoscale clusters and the larger intermetallic particles. Precipitation in ZX20 upon linear heating was compared to the one induced by hot extrusion at 330 C. Here, ternary precipitates outnumber the binary ones and are larger, incoherent, and in a much lower number density. They are unequivocally made of hexagonal Ca2Mg5Zn5, as deduced by atomically resolved EDS mapping and scanning TEM imaging, and supported by simulations. Precipitation complexity of in lean Mg-Zn-Ca alloys and its kinetic path are discussed.

cond-mat.mtrl-sci

Insights into image contrast from dislocations in ADF-STEM

Competitive mechanisms contribute to image contrast from dislocations in annular dark field scanning transmission electron microscopy ADF STEM. A clear theoretical understanding of the mechanisms underlying the ADF STEM contrast is therefore essential for correct interpretation of dislocation images. This paper reports on a systematic study of the ADF STEM contrast from dislocations in a GaN specimen, both experimentally and computationally. Systematic experimental ADF STEM images of the edge character dislocations revealed a number of characteristic contrast features that are shown to depend on both the angular detection range and specific position of the dislocation in the sample. A theoretical model based on electron channelling and Bloch wave scattering theories, supported by multislice simulations using Grillo s strain channelling equation, is proposed to elucidate the physical origin of such complex contrast phenomena.

cond-mat.mtrl-sci

Quantitative imaging of flux vortices in type-II superconductor MgB$_2$ using Cryo-Lorentz Transmission Electron Microscopy

Imaging of flux vortices in high quality MgB$_2$ single crystals has been successfully performed in a commercial Field Emission Gun-based Transmission Electron Microscope. In Cryo-Lorentz Microscopy, the sample quality and the vortex lattice can be monitored simultaneously, allowing one to relate microscopically the surface quality and the vortex dynamics. Such a vortex motion ultimately determines the flow resistivity, $\rho_{f}$, the knowledge of which is indispensable for practical applications such as superconducting magnets or wires for Magnetic Resonance Imaging. The observed patterns have been analyzed and compared with other studies by Cryo-Lorentz Microscopy or Bitter decoration. We find that the vortex lattice arrangement depends strongly on the surface quality obtained during the specimen preparation, and tends to form an hexagonal Abrikosov lattice at a relatively low magnetic field. Stripes or gossamer-like patterns, recently suggested as potential signatures of an unconventional behavior of MgB$_2$, were not observed.

cond-mat.supr-con

New Limits on the Ultra-high Energy Cosmic Neutrino Flux from the ANITA Experiment

We report initial results of the first flight of the Antarctic Impulsive Transient Antenna (ANITA-1) 2006-2007 Long Duration Balloon flight, which searched for evidence of a diffuse flux of cosmic neutrinos above energies of 3 EeV. ANITA-1 flew for 35 days looking for radio impulses due to the Askaryan effect in neutrino-induced electromagnetic showers within the Antarctic ice sheets. We report here on our initial analysis, which was performed as a blind search of the data. No neutrino candidates are seen, with no detected physics background. We set model-independent limits based on this result. Upper limits derived from our analysis rule out the highest cosmogenic neutrino models. In a background horizontal-polarization channel, we also detect six events consistent with radio impulses from ultra-high energy extensive air showers.

astro-ph

The Antarctic Impulsive Transient Antenna Ultra-high Energy Neutrino Detector Design, Performance, and Sensitivity for 2006-2007 Balloon Flight

We present a detailed report on the experimental details of the Antarctic Impulsive Transient Antenna (ANITA) long duration balloon payload, including the design philosophy and realization, physics simulations, performance of the instrument during its first Antarctic flight completed in January of 2007, and expectations for the limiting neutrino detection sensitivity. Neutrino physics results will be reported separately.

astro-ph