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

Applied Physics B

Heating of cold cesium atoms by blue-detuned laser radiation

Basrul Bahar, J. Castellanos, Udo Hübner, Carl O. Weiss

Published Mar 1, 1998• 0 citations
Publisher
DOI
10.1007/s003400050401

Related papers

Adiabatic focusing of cold atoms in a blue-detuned laser standing wave

Lev Khaykovich, Nir Davidson

Applied Physics B•May 1, 2000•2 citations

Cold and dense cesium clouds in far-detuned dipole traps

B. Boiron, A. Michaud, J.M. Fournier +4 more

Received 4 November 1997We study the behavior of cesium atoms confined in far-detuned laser traps and submitted to blue Sisyphuscooling. First, in a single focused yttrium aluminum garnet YAG beam, the atomic cloud has a rod shape witha6- 3mtransverse waist radius, a temperature of 2 K, and a transient density of 10

European Quantum Electronics Conference (EQEC)•Aug 24, 2005•0 citations

Laser Cooling and Trapping of Cesium Atoms

Muhammad Naeem Anwar

•Jan 1, 2016•0 citations

Arbitrarily copropagating superluminal and slow light by controllable one-photon detuning in trapped cold atoms

Yanting Zhao, Jie Ma, Xianli Zhang +3 more

Absorption spectra of cold cesium atoms confined in a magneto-optical trap are observed around the D2 transition line (6S(1/2), F=4-->6P(3/2), F'=5) with the probe laser frequency detuned near the trapping laser frequency. We observe the dispersion-like profile resulted from the stimulated Raman processes with the sub-natural linewidth, and study the behavior of the group velocity of light in trapped cold atoms. By only changing the blue and red detuning of the probe frequency from the trapping laser frequency, we are able to arbitrarily control the speed of a light pulse from subluminal to superluminal velocity.

Optics Express•Mar 24, 2008•0 citations

Laser cooling of cesium atoms in far-detuned optical lattices

S. Lukman Winoto

•Nov 1, 1999•0 citations

High-density cooling of cesium atoms in the gravito-optical surface trap

I. Manek, U. Moslener, M. Hammes +1 more

Summary form only given. The gravito-optical surface trap (GOST) confines cesium atoms by a blue-detuned repulsive evanescent wave (EW) in combination with gravity. Horizontal confinement is provided by the conservative optical dipole potential of a hollow, cylindrical laser beam, far blue-detuned from resonance. For preparing a very cold and dense cesium gas in the GOST, we use evanescent wave 'Sisyphus' cooling, which is based on inelastic reflections of the atoms from the EW. Using this method we have obtained a temperature of 3 /spl mu/K, which corresponds to an average distance of the atoms from the surface of 19 /spl mu/m. As a very important feature for attaining very high densities, EW cooling allows one to keep the atoms predominantly in the absolute ground state, thus avoiding trap loss by light assisted collisions.

Quantum Electronics and Laser Science Conference•Jan 20, 2003•0 citations
Absorption spectra of cold cesium atoms confined in a magneto-optical trap are observed around the D2 transition line (6S(1/2), F=4-->6P(3/2), F'=5) with the probe laser frequency detuned near the trapping laser frequency. We observe the dispersion-like profile resulted from the stimulated Raman processes with the sub-natural linewidth, and study the behavior of the group velocity of light in trapped cold atoms. By only changing the blue and red detuning of the probe frequency from the trapping laser frequency, we are able to arbitrarily control the speed of a light pulse from subluminal to superluminal velocity.
Summary form only given. The gravito-optical surface trap (GOST) confines cesium atoms by a blue-detuned repulsive evanescent wave (EW) in combination with gravity. Horizontal confinement is provided by the conservative optical dipole potential of a hollow, cylindrical laser beam, far blue-detuned from resonance. For preparing a very cold and dense cesium gas in the GOST, we use evanescent wave 'Sisyphus' cooling, which is based on inelastic reflections of the atoms from the EW. Using this method we have obtained a temperature of 3 /spl mu/K, which corresponds to an average distance of the atoms from the surface of 19 /spl mu/m. As a very important feature for attaining very high densities, EW cooling allows one to keep the atoms predominantly in the absolute ground state, thus avoiding trap loss by light assisted collisions.