Modelling the Growth of Tyndall Stars
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If you have a question about this talk, please contact Mustapha Amrani.
Free Boundary Problems and Related Topics
A “liquid snowflake” or “Tyndall star” is a small, thin, star-shaped region of liquid
water produced when ice is melted by absorption of light. In the early stages of its growth,
the liquid inclusion appears as a small, approximately axially symmetric, lens-like object. We investigate some models, based on having a highly anisotropic kinetic-undercooling
condition on the ice/water boundary, to try to understand the morphology of such a “Tyndall shape”.
This talk is part of the Isaac Newton Institute Seminar Series series.
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