非经典性和一个光子的影响.
Christopher C Gerry1, Richard J Birrittella2, Paul M Alsing3
1Department of Physics and Astronomy, Lehman College, The City University of New York, Bronx, NY 10468-1589, USA.
概括
调查量子干扰,这项研究表明,一个单一的光子如何产生量子干扰.
科学领域:
- 量子光学就是量子光学.
- 量子信息科学是一种量子信息科学.
背景情况:
- 光的量子状态表现出各种各样的特性,从高度非经典的 (数值状态) 到类似经典的 (连贯状态).
- 了解这些不同的量子状态之间的干扰效应对于推进量子技术至关重要.
研究的目的:
- 为了研究混合数态与相干的光态时的量子干扰效应.
- 分析单个光子的非经典性如何影响输出场的统计性质.
- 为了确定输出纠对连贯状态的幅度的依赖.
主要方法:
- 对数态和连贯态之间的量子干扰进行理论分析.
- 由于单光子混合而导致的统计性质转换的数学建模.
- 调查输出场中的纠性质.
主要成果:
- 将单个光子与一个连贯状态混合会显著改变输出的统计性质.
- 输出场的纠保持不变,无论相干状态的幅度如何.
- 量子干扰效应被证明可以改变光的非经典特征.
结论:
- 单个光子的非经典性在与连贯场混合时改变光的统计性质方面发挥着关键作用.
- 输出中的纠对于连贯状态振幅的变化是坚固的.
- 这项研究为量子信息处理中的潜在应用提供了对控制光的量子状态的见解.
相关概念视频
Photoelectric Effect
29.0K
When light of a particular wavelength strikes a metal surface, electrons are emitted. This is called the photoelectric effect. The minimum frequency of light that can cause such emission of electrons is called the threshold frequency, which is specific to the metal. Light with a frequency lower than the threshold frequency, even if it is of high intensity, cannot initiate the emission of electrons. However, when the frequency is higher than the threshold value, the number of electrons ejected...
29.0K
The de Broglie Wavelength
25.1K
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...
25.1K
The Wave Nature of Light
47.9K
The nature of light has been a subject of inquiry since antiquity. In the seventeenth century, Isaac Newton performed experiments with lenses and prisms and was able to demonstrate that white light consists of the individual colors of the rainbow combined together. Newton explained his optics findings in terms of a "corpuscular" view of light, in which light was composed of streams of extremely tiny particles traveling at high speeds according to Newton's laws of motion.
47.9K
The Bohr Model
49.4K
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...
49.4K
The Pauli Exclusion Principle
33.3K
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:
33.3K
The Uncertainty Principle
22.8K
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...
22.8K


