4.5 Article

Rapid ascent conditions of diamond-bearing kimberlitic magmas: Findings from high pressure-temperature experiments and finite element modeling

Journal

TECTONOPHYSICS
Volume 594, Issue -, Pages 13-26

Publisher

ELSEVIER
DOI: 10.1016/j.tecto.2013.03.006

Keywords

Multi-anvil experiments; Diamond-graphite transition; Electrical resistivity; Mantle xenoliths; Finite element model; Tensile failure

Funding

  1. Department of Science and Technology, Govt. of India
  2. Atomic Energy Commission
  3. Council of Scientific and Industrial Research, Govt. of India
  4. INSA
  5. SERB, Govt. of India

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This paper deals with the problem of rapid ascent mechanism of kimberlite magmas with a multi-directional approach: 1) the kinetics of diamond-graphite transition; 2) settling velocity of diamond phenocrysts in magmas and 3) formation of ruptures required for magma ascent with a high speed. Based on the diamond-graphite transition, we present an estimate of the ascent rates from high pressure and temperature experiments using Walker-type multi-anvil apparatus. The experiments were conducted with diamond, placed within a synthetic kimberlitic assemblage, keeping an initial pressure and temperature of 6 GPa and 1350 degrees C, respectively. It was observed that the volume fraction of diamond to graphite conversion strongly depended on the ascent rates. Using electrical resistivity and X-ray diffraction studies, we measured the degree of graphitization as a function of the ascent rate (u). For u < 3 m/s, diamond underwent almost complete graphitization (conversion > 90%), whereas it remained nearly intact (conversion < 10%) when u > 10 m/s. Our theoretical calculations of the settling velocity of mantle xenoliths again confirm that diamond can exist when u > 3 m/s. We performed numerical experiments with finite element (visco-elastic) models to analyze the dynamics of tensile failure at the tip of magma pools, leading to dilatational vertical fractures for magma transport. Considering the tensile strength of mantle in the order of 0.5 kb, our models show this failure process as a function of the critical shape (A(r): ratio of vertical and horizontal dimensions) and density contrast (Delta rho) of magma pools. The critical Delta rho is estimated nearly 200 kg/m(3) when A(r) is very large (>4). (C) 2013 Elsevier B.V. All rights reserved.

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