posted on 2024-07-12, 22:12authored byAndrea Elizabeth Garing
In this thesis we presented a comprehensive investigation of the thermodynamic behaviour of several astrophysically interesting crystalline phases. Then, for the first time, we derived a 2-dimensional distribution of gas and crystalline grains within a protoplanetary disc, and applied analytical calculations to study the possible chemistry and dynamics of grains and predict their evolution. Our results provide vital clues and new insights on the possible mechanisms that produced the observed crystalline grain distribution in protoplanetary discs, and the bulk material which likely formed meteorites and the planets in our Solar System.
History
Thesis type
Thesis (PhD)
Thesis note
Thesis submitted in fulfilment of the requirements of the degree of Doctor of Philosophy, Swinburne University of Technology, 2013.