Soft X-ray Irradiation of Silicates: Implications on Dust Evolution in Protoplanetary Disks
Authors:
Ciaravelli et al
Abstract:
The processing of energetic photons on bare silicate grains was simulated experimentally on silicate ?lms submitted to soft X-rays of energies up to 1.25 keV. The silicate material was prepared by means of a microwave assisted solgel technique. Its chemical composition reflects the Mg2SiO4 stoichiometry with residual impurities due to the synthesis method. The experiments were performed using the spherical grating monochromator beamline at the National Synchrotron Radiation Research Center in Taiwan. We found that soft X-ray irradiation induces structural changes that can be interpreted as an amorphization of the processed silicate material. The present results may have relevant implications in the evolution of silicate materials in X-ray irradiated protoplanetary disks.
Saturday, October 22, 2016
Soft X-ray Irradiation of Silicates: Implications on Dust Evolution in Protoplanetary Disks
Labels:
dust,
protoplanetary disks,
silicon,
x ray astronomy
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