On crystallization at the inner core boundary

Details On crystallization at the inner core boundary On crystallization at the inner core boundary

Jul 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005pepi..151...37s&link_type=abstract

Physics of the Earth and Planetary Interiors, Volume 151, Issue 1-2, p. 37-51.

Physics

7

Scientific paper

It is widely believed that a mushy layer develops at the inner core boundary (ICB) while the outer core material freezes onto the inner core. This view is obtained in reference to metallurgical or analog experiments on solidification carried out in the laboratory where morphological instability almost always follows constitutional supercooling. However, morphological instability is not an automatic consequence of supercooling: supercooling and stable solid liquid interface may coexist under certain conditions such as might perhaps occur at the ICB. If these conditions are realized, there could be both solidification on the ICB and crystallization of small solid particles in the supercooled layer (slurry layer). We made a linear stability analysis of a unidirectionally advancing solid liquid interface under the ICB conditions. Several values of the liquidus slope as a function of the concentration of light material (mC) were used for the stability analysis. It was confirmed that supercooling and stability may coexist if |mC| is low enough, although too low to be realistic. The estimated amount of supercooling in the layer is of order 0.1 K, and this provides an estimate of the size and population of solid particles in the slurry layer. However, even if |mC| were small enough, the existence of a slurry layer at the ICB would be unlikely due to (i) the difficulty of continuously supplying enough nuclei in the layer and (ii) the Rayleigh Taylor instability due to the compositional buoyancy. It is, therefore, most probable that a mushy layer exists at the ICB.

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