Relationships between textural and photoluminescence spectral features of carbonado (natural polycrystalline diamond) and implications for its origin
- Authors: Ishibashi H.1, Kagi H.2, Odake S.3, Ohfuji H.4, Kitawaki H.5
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Affiliations:
- Department of Geoscience, Faculty of Science
- Geochemical Research Center, Graduate School of Science
- Gemological Institute of America (GIA)
- Geodynamics Research Center
- Central Gem Laboratory
- Issue: Vol 54, No 10 (2016)
- Pages: 882-889
- Section: Article
- URL: https://journals.rcsi.science/0016-7029/article/view/155314
- DOI: https://doi.org/10.1134/S0016702916100050
- ID: 155314
Cite item
Abstract
Field Emission SEM (FESEM) textural observations, crystal size distribution (CSD) analyses, UV-excited luminescence imaging, and photoluminescence (PL) microspectroscopy excited by 488 nm laser were conducted on two texturally contrasting samples of carbonado, a kind of natural polycrystalline diamond from the Central African Republic (CAR). The investigated carbonado samples A and B show extremely different textures: sample A is made up of faceted crystals accompanied by abundant, small rectangular pores, whereas sample B has a granular texture with coarser crystals and scarce, large pores. Diamond crystals smaller than 2–3 µm are enriched in sample A but depleted in sample B. These textural features indicate that sample B diamonds were annealed under thermodynamically stable P–T conditions. The pore characteristics indicate that fluid permeability was higher for sample A than sample B. Photoluminescence (PL) spectra indicate that samples A and B correspond to Group A and B carbonados in the classification of Kagi et al. (1994), respectively, so that sample A reveals emissions from the H3 center without any N–V0 derived emission at 575 nm, whereas sample B shows emissions from the 3H center and the N–V0 defect. In addition, UV-excited luminescence images and photoluminescence spectra for sample B indicate that the rims of diamond crystals within several microns of a pore show luminescence features similar to those of Group AB carbonados (Kagi et al., 1994), indicating that this Group AB material was formed from Group B by irradiation from pore-filling, radioactive-element-bearing materials at a low temperature. The extent of the low-temperature irradiation is considered to depend on fluid permeability, and the Group A material was strongly irradiated due to its permeable texture whereas the Group B material was not significantly irradiated due to its less permeable granular texture. These results indicate that Group B carbonados have retained their original PL spectral features produced under high pressures and temperatures at mantle depths.
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About the authors
Hidemi Ishibashi
Department of Geoscience, Faculty of Science
Author for correspondence.
Email: shishib@ipc.shizuoka.ac.jp
Japan, Ohya 836, Suruga-ku, Shizuoka, 422-8529
Hiroyuki Kagi
Geochemical Research Center, Graduate School of Science
Email: shishib@ipc.shizuoka.ac.jp
Japan, Tokyo, 113-0033
Shoko Odake
Gemological Institute of America (GIA)
Email: shishib@ipc.shizuoka.ac.jp
Japan, Tokyo, 113-0016
Hiroyuki Ohfuji
Geodynamics Research Center
Email: shishib@ipc.shizuoka.ac.jp
Japan, Tokyo, 790-8577
Hiroshi Kitawaki
Central Gem Laboratory
Email: shishib@ipc.shizuoka.ac.jp
Japan, Tokyo, 110-0005
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