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Phase Transitions: Vaporization and Condensation02:39

Phase Transitions: Vaporization and Condensation

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The physical form of a substance changes on changing its temperature. For example, raising the temperature of a liquid causes the liquid to vaporize (convert into vapor). The process is called vaporization—a surface phenomenon. Vaporization occurs when the thermal motion of the molecules overcome the intermolecular forces, and the molecules (at the surface) escape into the gaseous state. When a liquid vaporizes in a closed container, gas molecules cannot escape. As these gas phase...
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Phase Transitions: Sublimation and Deposition02:33

Phase Transitions: Sublimation and Deposition

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Some solids can transition directly into the gaseous state, bypassing the liquid state, via a process known as sublimation. At room temperature and standard pressure, a piece of dry ice (solid CO2) sublimes, appearing to gradually disappear without ever forming any liquid. Snow and ice sublimate at temperatures below the melting point of water, a slow process that may be accelerated by winds and the reduced atmospheric pressures at high altitudes. When solid iodine is warmed, the solid sublimes...
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States of Matter and Phase Changes00:59

States of Matter and Phase Changes

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The internal energy of a substance—the total kinetic energy of all its molecules and the potential energy of their associated forces—depends on the strength of the intermolecular forces in the condensed phases and the pressure exerted on the substance. The internal energy of a substance is the highest in the gaseous state, the lowest in the solid state, and intermediate in the liquid state. Phase transitions are caused by changes in physical conditions, such as temperature and...
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Phase Transitions02:31

Phase Transitions

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Whether solid, liquid, or gas, a substance's state depends on the order and arrangement of its particles (atoms, molecules, or ions). Particles in the solid pack closely together, generally in a pattern. The particles vibrate about their fixed positions but do not move or squeeze past their neighbors. In liquids, although the particles are closely spaced, they are randomly arranged. The position of the particles are not fixed—that is, they are free to move past their neighbors to...
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Phase Transitions: Melting and Freezing02:39

Phase Transitions: Melting and Freezing

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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...
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Phase Changes01:19

Phase Changes

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Phase transitions play an important theoretical and practical role in the study of heat flow. In melting or fusion, a solid turns into a liquid; the opposite process is freezing. In evaporation, a liquid turns into a gas; the opposite process is condensation.
A substance melts or freezes at a temperature called its melting point and boils or condenses at its boiling point. These temperatures depend on pressure. High pressure favors the denser form of the substance, so typically, high pressure...
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扩张的介质中的相位过渡:热残留物.

Romuald A Janik1, Matti Järvinen2,3, Jacob Sonnenschein4

  • 1Jagiellonian University, Institute of Theoretical Physics and Mark Kac Center for Complex Systems Research, Łojasiewicza 11, 30-348 Kraków, Poland.

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概括

我们研究了膨胀宇宙中的相位过渡. 热等离子体残留物持续存在,抵御冷却和泡核形成,即使在宇宙膨胀下.

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科学领域:

  • 高能物理 高能物理
  • 宇宙学的宇宙学是什么?
  • 量子场理论 量子场理论

背景情况:

  • 了解早期宇宙需要研究不断膨胀的介质中的相位过渡.
  • 全息模型为强合的量子场理论提供了洞察力.

研究的目的:

  • 分析扩张系统中封闭-解封阶段过渡的动态.
  • 为了研究在膨胀过程中热等离子体残余的行为.

主要方法:

  • 使用有效的边界描述.
  • 将描述与全息Witten模型相匹配.
  • 在提升不变和宇宙膨胀场景中模拟动态.

主要成果:

  • 观察到持久的热血残留物没有降温.
  • 尽管系统扩张,这些残留物抵御了泡核形成.
  • 在不同的膨胀模型中,残留物收缩,溶解和重新加热的动力学是强大的.

结论:

  • 热等离子体残留物在膨胀过程中表现出稳定的行为,挑战了典型的相位过渡期望.
  • 这些发现在Minkowski和Friedmann-Robertson-Walker时空中都是一致的.
  • 这种强度表明,在不断膨胀的宇宙中,这些残留物具有基本的特性.