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The Quantum-Mechanical Model of an Atom02:45

The Quantum-Mechanical Model of an Atom

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Shortly after de Broglie published his ideas that the electron in a hydrogen atom could be better thought of as being a circular standing wave instead of a particle moving in quantized circular orbits, Erwin Schrödinger extended de Broglie’s work by deriving what is now known as the Schrödinger equation. When Schrödinger applied his equation to hydrogen-like atoms, he was able to reproduce Bohr’s expression for the energy and, thus, the Rydberg formula governing...
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The de Broglie Wavelength02:32

The de Broglie Wavelength

25.2K
In the macroscopic world, objects that are large enough to be seen by the naked eye follow the rules of classical physics. A billiard ball moving on a table will behave like a particle; it will continue traveling in a straight line unless it collides with another ball, or it is acted on by some other force, such as friction. The ball has a well-defined position and velocity or well-defined momentum, p = mv, which is defined by mass m and velocity v at any given moment. This is the typical...
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The Uncertainty Principle04:08

The Uncertainty Principle

22.9K
Werner Heisenberg considered the limits of how accurately one can measure properties of an electron or other microscopic particles. He determined that there is a fundamental limit to how accurately one can measure both a particle’s position and its momentum simultaneously. The more accurate the measurement of the momentum of a particle is known, the less accurate the position at that time is known and vice versa. This is what is now called the Heisenberg uncertainty principle. He...
22.9K
The Pauli Exclusion Principle03:06

The Pauli Exclusion Principle

33.6K
The arrangement of electrons in the orbitals of an atom is called its electron configuration. We describe an electron configuration with a symbol that contains three pieces of information:
33.6K
The Bohr Model02:18

The Bohr Model

49.7K
Following the work of Ernest Rutherford and his colleagues in the early twentieth century, the picture of atoms consisting of tiny dense nuclei surrounded by lighter and even tinier electrons continually moving about the nucleus was well established. This picture was called the planetary model since it pictured the atom as a miniature “solar system” with the electrons orbiting the nucleus like planets orbiting the sun. The simplest atom is hydrogen, consisting of a single proton as...
49.7K
Quantum Numbers02:43

Quantum Numbers

34.1K
It is said that the energy of an electron in an atom is quantized; that is, it can be equal only to certain specific values and can jump from one energy level to another but not transition smoothly or stay between these levels.
34.1K

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相关实验视频

Updated: May 15, 2025

Scalable Quantum Integrated Circuits on Superconducting Two-Dimensional Electron Gas Platform
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Scalable Quantum Integrated Circuits on Superconducting Two-Dimensional Electron Gas Platform

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量子和经典制度之间微妙的细微差别.

Karin Wittmann Wilsmann1, Erick R Castro2, Itzhak Roditi2

  • 1Instituto de Física, Universidade do Rio Grande do Sul, RS 91501-970, Brazil.

Chaos (Woodbury, N.Y.)
|April 8, 2025
PubMed
概括
此摘要是机器生成的。

这项研究研究了许多玻色子的量子系统,揭示了经典和量子行为如何在不同的相互作用模式中对齐. 研究结果显示了经典轨迹和量子状态之间的联系,类似于已知的模式.

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科学领域:

  • 量子物理学的量子物理学
  • 多体系统是多体系统.
  • 这是量子混沌.

背景情况:

  • 了解半古典极限对于弥合量子力学和古典物理学至关重要.
  • 玻色的多体系统在潜力中表现出不同的行为,从可整合到混乱.
  • 之前的工作已经探索了各种物理系统中的量子-经典对应.

研究的目的:

  • 探索一个可整合的混沌玻色多体量子系统的半经典极限.
  • 检查不同相互作用模式 (可整合,自我陷,混乱) 中的经典-量子对应.
  • 为了研究经典相空间投影和量子维格纳函数之间的关系.

主要方法:

  • 分析三井潜力中的玻色子多体系统.
  • 经典轨迹的相空间平均投影与量子胡西米分布的比较.
  • 在可整合,自我陷和混乱的相互作用制度中进行调查.

主要成果:

  • 在古典轨迹的相位空间平均投影和Husimi分布之间观察到非常相似.
  • 这种相似之处支持了对自态的维格纳函数的一致半古典凝聚的原理.
  • 结果中观察到的模式让人想起了杰森·加拉斯的""形状.

结论:

  • 该研究提供了对可整合混沌玻色子系统半经典行为的细微见解.
  • 经典-量子对应在不同的相互作用模式中是明显的.
  • 这些发现突出了经典动力学和半经典极限中的量子状态分布之间的联系.