新加坡南洋理工大学Simon Redfern教授研究组招收2021秋季博士生
研究课题:高压下材料结构预测
Pressure-driven routes to materials discovery and planetary formation - abundant element compounds at high pressures.
We are familiar with the fact that matter changes state, due to driving free energy changes, as a function of temperature or pressure - solid ice transforms to liquid water to gaseous steam as we heat it, or, transforms from solid to liquid as we add sodium chloride. The influence of pressure on matter is less-well studied, but is a much stronger effect. The discovery of room temperature superconductivity in mixtures of carbon, sulfur and hydrogen recently* is a consequence of the high-density conditions of the mixture, held at more than two million atmospheres’ pressure. Such extraordinary physical phenomena and physical conditions can be achieved in laboratory experiments, and in computer simulations of materials, but they are also the conditions found deep in planetary interiors. When pressure is applied, the interatomic distances in materials may change significantly, modifying bonding and electronic structure. Pressure is now recognized as an important, if sometimes brutal, force for modifying the structures and properties of materials, so it also offers new opportunities for creating new materials, for materials discovery, and for unveiling novel physical and chemical properties of materials. It is also important for understanding how planets and their moon satellites form, and ultimately how dense matter in the universe behaves. The ten most abundant elements in our galaxy are H, He, O, C, Ne, Fe, N, Si, Mg and S. This project will take simple mixtures of light elements from this group (similar to the C-H-S superconductors mentioned above) up to high pressure to explore the new physics and chemistry that their combinations result in, to shed new light on materials discovery, as well as on planetary formation, geophysical and geochemical processes, and planetary evolution.
*Snider, E., Dasenbrock-Gammon, N., McBride, R. et al. Room-temperature superconductivity in a carbonaceous sulfur hydride. Nature 586, 373–377 (2020).
GPA:3.2/4.0(最好3.5+),TOEFL 100/IELTS 6.5,最好有GRE成绩,两封推荐信,申请截止日期可根据情况延后,具体项目要求见NTU ASE PhD项目官网
导师简介:
Simon Redfern目前为南洋理工亚洲环境学院教授,理学院院长。Simon博士毕业于英国剑桥大学,曾任剑桥大学地球科学系教授,系主任,和英国,欧洲,北美,中国的学术圈都有较多联系。Simon的研究兴趣很广泛,包括矿物学,晶体学,材料学,地球科学,目前主要研究高温高压下物质的原子结构和物理化学性质,以及行星内部的物质构造。Simon是一个非常随和,易于沟通交流的导师,曾成功培养过24个博士,对学生非常耐心。课题组经常组织烧烤,麻将等团建活动,氛围良好。