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相关概念视频

Polymer Classification: Crystallinity01:21

Polymer Classification: Crystallinity

2.8K
Unlike ionic or small covalent molecules, polymers do not form crystalline solids due to the diffusion limitations of their long-chain structures. However, polymers contain microscopic crystalline domains separated by amorphous domains.
Crystalline domains are the regions where polymer chains are aligned in an orderly manner and held together in proximity by intermolecular forces. For example, chains in the crystalline domains of polyethylene and nylon are bound together by van der Waals...
2.8K
Molecular and Ionic Solids02:54

Molecular and Ionic Solids

17.1K
Crystalline solids are divided into four types: molecular, ionic, metallic, and covalent network based on the type of constituent units and their interparticle interactions.
Molecular Solids
Molecular crystalline solids, such as ice, sucrose (table sugar), and iodine, are solids that are composed of neutral molecules as their constituent units. These molecules are held together by weak intermolecular forces such as London dispersion forces, dipole-dipole interactions, or hydrogen bonds, which...
17.1K
Recrystallization: Solid–Solution Equilibria01:10

Recrystallization: Solid–Solution Equilibria

1.1K
Recrystallization is a purification technique used to separate impurities from solid compounds. In this technique, no chemical reactions occur. Instead, it exploits physical properties only, specifically, the solubility differences between the desired compound and impurities, either at a single temperature or at different temperatures, and under other selected conditions. The solid-solution equilibrium (solubility equilibrium) of each component in the solution represents a binary phase...
1.1K
Crystal Growth: Principles of Crystallization01:25

Crystal Growth: Principles of Crystallization

1.8K
Crystallization is a phase transformation process in which crystals are precipitated from a supersaturated solution or formed from other sources. During crystallization, atoms or molecules arrange themselves into a well-defined, rigid crystal lattice to minimize energy.
Initiating crystallization involves manipulating the concentration of the solute and the temperature of the solution. Since crystal growth occurs when the ratio of concentration and solubility of the solute in the solvent...
1.8K
Metallic Solids02:37

Metallic Solids

18.4K
Metallic solids such as crystals of copper, aluminum, and iron are formed by metal atoms. The structure of metallic crystals is often described as a uniform distribution of atomic nuclei within a “sea” of delocalized electrons. The atoms within such a metallic solid are held together by a unique force known as metallic bonding that gives rise to many useful and varied bulk properties.
All metallic solids exhibit high thermal and electrical conductivity, metallic luster, and malleability....
18.4K
Phase Transitions: Melting and Freezing02:39

Phase Transitions: Melting and Freezing

12.4K
Heating a crystalline solid increases the average energy of its atoms, molecules, or ions, and the solid gets hotter. At some point, the added energy becomes large enough to partially overcome the forces holding the molecules or ions of the solid in their fixed positions, and the solid begins the process of transitioning to the liquid state or melting. At this point, the temperature of the solid stops rising, despite the continual input of heat, and it remains constant until all of the solid is...
12.4K

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相关实验视频

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Simulation of the Planetary Interior Differentiation Processes in the Laboratory
06:04

Simulation of the Planetary Interior Differentiation Processes in the Laboratory

Published on: November 15, 2013

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探索表面特性和水晶中的预化.

Azat O Tipeev1, Alexander L Gurashkin2, Edgar D Zanotto1

  • 1Department of Materials Engineering, Federal University of São Carlos, 13.565-905 São Carlos, SP, Brazil.

The Journal of chemical physics
|June 12, 2024
PubMed
概括

我们计算了LJ,和的晶体表面自由能量. 在LJ晶体中观察到预化,为晶体核和生长提供了洞察力.

科学领域:

  • 材料科学 材料科学 材料科学
  • 表面科学是一门学科.
  • 计算物理 计算物理

背景情况:

  • 晶体表面的特性控制着诸如吸附,核和摩擦等关键过程.
  • 表面自由能量 (γ) 是影响这些现象的关键参数.

研究的目的:

  • 直接计算伦纳德-斯 (LJ),和晶体的低指数面的温度依赖的表面自由能量 (γ(T)).
  • 研究表面预融现象及其与晶体稳定性和融化线的关系.

主要方法:

  • 利用计算分离技术来计算表面自由能量.
  • 采用原子学模拟来分析表面原子的移动性和结构变化.

主要成果:

  • 计算了LJ,Ge和Si晶体的γ{\text{T}},与Si{\text{11}}和Ge{\text{111}的实验数据有很好的一致.
  • 在LJ晶体中确定了从0.75Tm开始的表面预化,与增加的表面原子流动性和在负压下变态稳定的化线相关.
  • 由于化前引起的故障,观察到低于均质结极限的薄LJ晶片中的再结晶.
  • 在Ge和Si模型晶体中没有发现预融的证据,与实验观测一致.

结论:

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  • 计算分离技术准确地预测了真实材料的表面自由能量.
  • 在LJ晶体中的表面预融提供了一个模型来理解负压和深超冷的现象.
  • 该研究提供了对晶体表面行为,核形成和原子尺度上的增长的见解.