取自V. Grib金伯利岩管的钻石:形态和光谱特征

E. A. Vasilev, V. N. Ustinov, S. I. Leshukov, R. N. Pendeliak, E. V. Nikolaeva
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引用次数: 0

摘要

研究课题。本文介绍了对V. Grib金伯利岩管上部陨石坑和双气孔相勘探钻孔岩心500颗金刚石晶体的研究结果。分别分析了凝灰岩和凝灰岩(火山口)、凝灰岩角砾岩、自长岩金伯利岩角砾岩和斑岩金伯利岩(斑岩)的结晶。的目标。对V. Grib管中金刚石进行了形态学和光谱学研究。材料与方法。采用VERTEX-70光谱仪和Hyperion 1000显微镜测定了样品中总氮浓度和以B型缺陷形式存在的氮(NBS)的比例,以及“血小板”B′带(3107 cm-1)的吸收系数。利用ALROSA VIEW PRO设备记录了360 nm激发下的光致发光(PL)图像,以检测PL的不均匀性和颜色。用Horiba FL-3光谱仪在300 K下激发350和450 nm,用InVia Renishaw光谱仪在77 K下激发405、488和787 nm记录了PL光谱。结果。钻石在氮浓度和NBS方面的分布是特定的;约50%的晶体沿一条等温线分布,低氮晶体占5%。25%的晶体的PL谱线为883/885 nm的含镍缺陷线。大多数具有这种缺陷的晶体的氮含量低于400ppm,但根据NBS,它们占据了整个范围。该系统存在于76%的双胞胎和共生体的光谱中;后者占钻石的36%,线条为883/885 nm。所研究的钻石与M.V. Lomonosov矿床中发现的钻石的不同之处在于,立方结构晶体含量低得多(2和15%),溶解程度低(八面体,分别为33和15%),彩色宝石比例低,氮浓度和NBS范围广。结论。揭示的特征表明,V. Grib矿床的钻石生长条件与东欧、西伯利亚地台和乌拉尔地区其他金伯利岩体的钻石生长条件不同。低氮晶体和含镍钻石的高比例可能表明存在较大的clippir型晶体。
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Diamonds from V. Grib kimberlite pipe: Morphology and spectroscopic features
Research subject. The article presents the results of studying 500 diamond crystals from the core of exploration boreholes of crater and diatreme facies of the upper part of V. Grib kimberlite pipe. Crystals from tuffs and tuffites (crater), tufobreccia, autolith kimberlite breccia and porphyry kimberlite (diatreme) were analyzed separately. aim. To carry out a morphological and spectroscopic study of diamonds from V. Grib pipe. Materials and Methods. An VERTEX-70 spectrometer with a Hyperion 1000 microscope was used to determine the total nitrogen concentration and the share of nitrogen in the form of B defects (NBS), the absorption coefficients of the “platelet” bands B', 3107 cm-1. Images of photoluminescence (PL) were recorded at 360 nm excitation by an ALROSA VIEW PRO device, in order to detect inhomogeneities and color of PL. The PL spectra were recorded by a Horiba FL-3 spectrometer with an excitation of 350 and 450 nm at 300 K and by an InVia Renishaw spectrometer with an excitation of 405, 488 and 787 nm at 77 K. Results. The distribution of diamonds in terms of nitrogen concentration and NBS is specific; about 50% of the crystals are located along one isotherm, the proportion of low-nitrogen crystals is 5%. The PL spectra of 25% of crystals showed the lines of 883/885 nm of an elementary Ni-containing defect. Most crystals with this defect have less than 400 ppm of nitrogen, but they occupy the entire range according to NBS. This system is found in the spectra of 76% of twins and intergrowth; the latter are of 36% of diamonds with the lines 883/885 nm. The studied diamonds differ from those found in M.V. Lomonosov deposit in terms of a much lower content of crystals of cubic habitus (2 and 15%), a lower degree of dissolution (octahedra, respectively, 33 and 15%), a low proportion of colored stones, as well as a wide range of nitrogen concentration and NBS. Conclusion. The revealed features indicate the specific growth conditions of diamonds from V. Grib deposit, which differed from those of diamonds from other kimberlitic bodies of the East European, Siberian platforms and the Urals. The high proportion of low-nitrogen crystals and Ni-containing diamonds is a possible indicator for the presence of large CLIPPIR-type crystals.
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