- Rydberg constant - Wikipedia
In spectroscopy, the Rydberg constant, symbol for heavy atoms or for hydrogen, named after the Swedish physicist Johannes Rydberg, is a physical constant relating to the electromagnetic spectra of an atom
- 量子光学 | 里德堡原子简介 - 知乎
Rydberg state：Rydberg atom指有一个电子被激发至high-n的系统，我们称这些系统处于Rydberg state。 这里之所以使用“系统”，是因为处于高激发的束缚态原子、分子以及其他相似系统均可以用modified Rydberg formula描述，因为high-n电子波函数被localized在距离离子实束缚能
- 里德伯常量_百度百科
后来，波尔引入 约化质量，计算出理论值R=10967757 8m -1 中文名 里德伯常量 外文名 Rydberg constant 理论值 R=1 097373157×10^7 m^-1 实验值 R=1 0967758×10^7m^-1
- Realization of a Rydberg-dressed extended Bose-Hubbard model
Ultracold atoms in optical lattices have been used extensively to simulate the behavior of the Hubbard model, which describes the physics of interacting particles on a lattice However, past studies focused largely on on-site interactions, which are easier to implement experimentally Weckesser et al used the so-called Rydberg dressing technique to create extended-range interactions between
- Rydberg Physics - Book - IOPscience
Rydberg physics is the land of gentle giants—highly-excited electronic states where an electron is, on average, far from the nucleus They are created with a lot of energy, have unusually large size and live relatively long
- Rydberg state of atoms - Nature
Excited atoms under a high energy level, termed as Rydberg atoms, possess exceptional characteristics (e g , size and dipole moment), which are contingent on their principal quantum numbers
- 里德伯常量 - 维基百科，自由的百科全书
里德伯常量 里德伯常量（英語： Rydberg constant）是物理学中经常用到的常數。 根据2014年 CODATA 的结果，它的值是 R ∞ = 1 0973731568508 ( 65 ) × 10 7 m − 1 {\displaystyle R_ {\infty }=1 0973731568508 (65)\times 10^ {7}\,\mathrm {m} ^ {-1}} [1]
- Rydberg constant | Definition, Formula, Value, Facts - Britannica
Rydberg constant, fundamental constant of atomic physics that appears in the formulas developed (1890) by the Swedish physicist Johannes Rydberg, describing the wavelengths or frequencies of light in various series of related spectral lines, most notably those emitted by hydrogen atoms in the Balmer series
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