Challenges
Datasets
Workspaces
Papers
Discussions
Leaderboard
Log inSign up
Challenges
Datasets
Workspaces
Papers
Discussions
Leaderboard
Blog
Job Board
Q3AS

© 2026 Aqora Quantum S.A.S.

TermsPrivacyLegal Notice

Physics Letters A

About a possibility of a decrease in the radiative width of excited levels of atoms and nuclei

И. Д. Феранчук

Published May 1, 1981• 3 citations
Publisher
DOI
10.1016/0375-9601(81)90514-4

Related papers

Two-photon excitation of nuclei

I. V. Krasnov, N. Ya. Shaparev

An analysis is made of the two-photon absorption of radiation by nuclei subjected to two opposed $gamma$-ray fluxes. The absorption cross section has two maxima separated by the recoil energy. The higher maximum, of width GAMMA governed by the radiative damping, is associated with the recoilless absorption; the lower maximum, of width governed by the Doppler effect, describes the absorption in the presence of recoil. The low maximum makes it possible to attain low values of the parameter GAMMA/$omega$. (AIP)

Soviet Journal of Quantum Electronics•Dec 31, 1975•0 citations

Probabilities of radiative transitions between highly excited atomic states

S. P. Goreslavskiǐ, Nikolai B. Delone, В. П. Крайнов

Journal of Experimental and Theoretical Physics•Jun 1, 1982•5 citations

Rates of Radiative Transitions and Atomic Spectra

Boris Michailovich Smirnov

Springer series on atomic, optical, and plasma physics•Jan 1, 2018•0 citations

On the super-narrow gamma lines of nuclei in a Bose—Einstein condensate

Лев Абрамович Ривлин

It is shown that due to the quantum coherence of atoms in a Bose—Einstein condensate, the width of gamma lines of the long-lived metastable states of isomeric nuclei in these atoms can be close to the natural radiative width. This opens up the possibility of observing super-narrow gamma lines, which are narrower by a few orders of magnitude than the Mössbauer gamma line.

Quantum Electronics•Apr 30, 2005•3 citations

On the Width of γ-Line and the Photon Structure

Vladimir V Koltsov

The well-known narrowing of the Mössbaur γ-line with increasing age of the excited energy state ℏω0 of the emitter nucleus (the half-life is T1/2) and broadening of the γ-line with decreasing irradiation time of the absorber nucleus are analyzed. Taking into account the short time of emission of quantum transition energy – much less than T1/2, which can be seen, for example, from the duration of the γ-signal on the scintillator, the analysis leads to the idea of the structure of the γ-quantum (photon) as an electromagnetic wave of frequency ω0 that does not carry energy (0-wave), which is emitted by the nucleus from the moment of formation of the excited state to the quantum transition, with the energy quantum ℏω0 in the form of a short-term singularity on the “tail” of this 0-wave. A possible source of 0-waves can be virtual transitions of the nucleus from the excited state to the ground state and back before the emission of an energy quantum. Detection of 0-waves is possible due to changing the width of the γ‑line with additional irradiation of the absorber nuclei by resonant 0-waves. The possibility of predicting the future decay of an excited state by 0-waves detecting and the prospects of using 0-waves for information transmission are noted. The principle of a 0-wave generator without energy radiation is proposed.

Physics of Atomic Nuclei•Dec 1, 2022•2 citations

Approximate calculation of the radiative lifetimes of excited states of atoms and ions

Pavel Bogdanovich, G. L. Zhukauskas, Alina Momkauskaitė

OptSp•Apr 1, 1988•0 citations
An analysis is made of the two-photon absorption of radiation by nuclei subjected to two opposed gammagammagamma-ray fluxes. The absorption cross section has two maxima separated by the recoil energy. The higher maximum, of width GAMMA governed by the radiative damping, is associated with the recoilless absorption; the lower maximum, of width governed by the Doppler effect, describes the absorption in the presence of recoil. The low maximum makes it possible to attain low values of the parameter GAMMA/omegaomegaomega. (AIP)
The well-known narrowing of the Mössbaur γ-line with increasing age of the excited energy state ℏω0 of the emitter nucleus (the half-life is T1/2) and broadening of the γ-line with decreasing irradiation time of the absorber nucleus are analyzed. Taking into account the short time of emission of quantum transition energy – much less than T1/2, which can be seen, for example, from the duration of the γ-signal on the scintillator, the analysis leads to the idea of the structure of the γ-quantum (photon) as an electromagnetic wave of frequency ω0 that does not carry energy (0-wave), which is emitted by the nucleus from the moment of formation of the excited state to the quantum transition, with the energy quantum ℏω0 in the form of a short-term singularity on the “tail” of this 0-wave. A possible source of 0-waves can be virtual transitions of the nucleus from the excited state to the ground state and back before the emission of an energy quantum. Detection of 0-waves is possible due to changing the width of the γ‑line with additional irradiation of the absorber nuclei by resonant 0-waves. The possibility of predicting the future decay of an excited state by 0-waves detecting and the prospects of using 0-waves for information transmission are noted. The principle of a 0-wave generator without energy radiation is proposed.