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

Bulletin of the American Physical Society

Observation of quantum accelerator modes in Rb atoms

Vijayashankar Ramareddy, Brian P. Timmons, G. Behinaein, Peyman Ahmadi, Gil S. Summy

Published May 19, 2006• 0 citations
OpenAlex

Related papers

Acceleration of cold Rb atoms by frequency modulated light pulses

Jozsef S. Bakos, Gagik P. Djotyan, P.N. Ignácz +5 more

The European Physical Journal D•May 3, 2007•10 citations

Laser Cooling and Trapping of Rb Atoms

S. Chakraborty, A. Banerjee, Ayan Ray +4 more

•Dec 1, 2006•0 citations

Effect of a magnetic field gradient and gravitational acceleration on a time-domain grating-echo interferometer

M. Weel, I. Y. Chan, Scott Beattie +3 more

We have observed the effects of magnetic field gradients and gravitational acceleration on grating echoes in a time-domain single state atom interferometer that uses laser cooled Rb atoms. These observations are compared to theoretical predictions based on a simplified model. The oscillatory dependence of the echo amplitude due to the magnetic field gradient is in agreement with the predicted quadratic scaling as a function of the time between excitation pulses. We also observe a linear dependence of this oscillation frequency as a function of the magnetic field gradient which is predicted by theory. In the presence of gravity, the calculations predict a quadratic dependence for the echo phase on the time between excitation pulses as well as a change in the shape of the echo envelope. We have observed both of these effects in the experiment, and we find that the change in shape is qualitatively consistent with our prediction. It is necessary to understand these effects in order to carry out high precision studies of the atomic fine-structure constant and gravitational acceleration using this interferometric technique. We also present an improved measurement of gravitational acceleration using this technique that is precise to $\ensuremath{\sim}15\phantom{\rule{0.3em}{0ex}}\mathrm{ppm}$ by exploiting the quadratic phase dependence.

Physical Review A•Jun 28, 2006•19 citations

Double resonance spectroscopy of laser-cooled Rb atoms

Alastair G. Sinclair, Barry D. McDonald, Erling Riis +1 more

Optics Communications•Mar 1, 1994•27 citations

Quantum Accelerator Modes Near Higher-Order Resonances

Italo Guarneri, Laura Rebuzzini

Quantum accelerator modes have been experimentally observed, and theoretically explained, in the dynamics of kicked cold atoms in the presence of gravity, when the kicking period is close to a half-integer multiple of the Talbot time. We generalize the theory to the case when the kicking period is sufficiently close to any rational multiple of the Talbot time, and thus predict new rich families of experimentally observable quantum accelerator modes.

arXiv:0805.2040•Physical Review Letters•Jun 13, 2008•11 citations

Ultracold collisions between Rb atoms and a Sr + ion

Tomáš Šikorský, Ziv Meir, Ruti Ben-shlomi +2 more

Bulletin of the American Physical Society•Jun 11, 2015•0 citations
We have observed the effects of magnetic field gradients and gravitational acceleration on grating echoes in a time-domain single state atom interferometer that uses laser cooled Rb atoms. These observations are compared to theoretical predictions based on a simplified model. The oscillatory dependence of the echo amplitude due to the magnetic field gradient is in agreement with the predicted quadratic scaling as a function of the time between excitation pulses. We also observe a linear dependence of this oscillation frequency as a function of the magnetic field gradient which is predicted by theory. In the presence of gravity, the calculations predict a quadratic dependence for the echo phase on the time between excitation pulses as well as a change in the shape of the echo envelope. We have observed both of these effects in the experiment, and we find that the change in shape is qualitatively consistent with our prediction. It is necessary to understand these effects in order to carry out high precision studies of the atomic fine-structure constant and gravitational acceleration using this interferometric technique. We also present an improved measurement of gravitational acceleration using this technique that is precise to $\ensuremath{\sim}15\phantom{\rule{0.3em}{0ex}}\mathrm{ppm}$ by exploiting the quadratic phase dependence.