Low‐energy helium ion irradiation‐induced amorphization and chemical changes in olivine: Insights for silicate dust evolution in the interstellar medium

By P. Carrez, K. Demyk, P. Cordier, L. Gengembre, J. Grimblot, L. D'hendecourt, A. Jones, H. Leroux. 2002

133 citations recorded by the source corpus.

Subfields: Computational Mechanics, Geophysics, Materials Chemistry

View Paper: https://www.semanticscholar.org/paper/790be6eab68841c48a2fcfe2d732e3dadb882ef9

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In Materials Chemistry

1. A. Tielens

Citations in the corpus

• The Absence of Crystalline Silicates in the Diffuse Interstellar Medium (2004, background): “…studies have investigated the effect of ion bombardments on crystalline grains (e.g., Day 1977; Bradley 1994; Wang et al. 1998; Demyk et al. 2001; Carrez et al. 2002; Jäger et al. 2003b; Brucato et al. 2004), measuring the required dose for amorphization as a function of energy and element used.”
• Ion irradiation of carbonaceous chondrites: A new view of space weathering on primitive asteroids (2017, methodology): “…CCs or terrestrial olivine sample; corresponding to band number 3) exceeds the position of a crystalline olivine with a forsterite number of 0 (no Mg content = 100 % fayalite) [Hamilton, 2010]: this is because Mg loss is also accompanied by amorphization [Demyk et al., 2001; Carrez et al., 2002].”