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Entropically Driven Self-Assembly of Colloidal Crystals on Templates in Space

机译:空间模板上胶体晶体的熵驱动自组装

摘要

These experiments aim to create new colloidal crystalline materials, to study the assembly and thermodynamics of these materials, to measure the optical properties of these materials. and to fix the resulting structures so that they can be brought back and studied on earth. In microgravity, the elimination of particle sedimentation effects creates a purely "thermodynamic" environment for colloidal suspensions wherein particle size, volume fraction, and interparticle interactions are the primary determinants of the assembled structures. We will control the colloidal assembly process using attractive, entropic particle interactions brought about by the depletion effect. By using attractive interactions for colloidal assembly we create conditions for growth that resemble those associated with "conventional" microscopic systems such as atoms and molecules. This approach differs qualitatively from the more common "space-filling" mode of colloidal crystal growth that is driven purely by packing constraints. It is anticipated that at least some of the solidified structures will survive reentry to earth's gravitational field, and that their optical, magnetic, and electrical properties can then be studied in detail upon return.
机译:这些实验旨在创建新的胶态晶体材料,以研究这些材料的组装和热力学,以测量这些材料的光学性质。并修复由此产生的结构,以便可以将其带回地球并进行研究。在微重力下,消除颗粒沉降效应为胶体悬浮液创造了一个纯粹的“热力学”环境,其中粒径,体积分数和颗粒间相互作用是组装结构的主要决定因素。我们将使用由耗尽效应带来的有吸引力的熵粒子相互作用来控制胶体组装过程。通过使用吸引人的相互作用进行胶体组装,我们创造了类似于“常规”微观系统(例如原子和分子)的生长条件。这种方法在质量上与胶体晶体生长的更普遍的“空间填充”模式不同,后者仅由堆积约束驱动。可以预料,至少有一些凝固的结构会在折返地球重力场后幸存下来,然后可以在返回时详细研究它们的光学,磁性和电学性质。

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