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

Ionization and recombination dynamics of an expanding ultracold Rydberg gas

Thomas Pohl, Thomas Pattard, Jan Michael Rost

Published Jan 1, 2003• 0 citations
OpenAlex

Related papers

Ionization processes induced by ultralong-range interactions in an ultracold Rydberg gas [Kurzvortrag]

Thomas Amthor, M. Reetz‐Lamour, Sebastian Westermann +4 more

•Jan 1, 2006•0 citations

Plasma formation from ultracold Rydberg gases

Thomas Pohl, Thomas Pattard, Jan Michael Rost

Recent experiments have demonstrated the spontaneous evolution of a gas of ultracold Rydberg atoms into an expanding ultracold plasma, as well as the reverse process of plasma recombination into highly excited atomic states. Treating the evolution of the plasma on the basis of kinetic equations, while ionization/excitation and recombination are incorporated using rate equations, we have investigated theoretically the Rydberg-to-plasma transition. Including the influence of spatial correlations on the plasma dynamics in an approximate way, we find that ionic correlations change the results quantitatively but not qualitatively.

arXiv:physics/0303052•Physical Review A•Jul 25, 2003•67 citations

Highly excited state Rydberg recombination and consequences for ultracold neutral plasmas

H. R. Sadeghpour, Thomas Pohl, D. Vrinceanu

Bulletin of the American Physical Society•May 30, 2008•0 citations

Correlated excitation dynamics in an ultracold Rydberg gas

Cristiano Simonelli, María Martínez Valado, Raffaele Faoro +6 more

•Jan 1, 2015•0 citations

Recombination in an expanding ultracold plasma

M. J. Lim, T. C. Killian, S. A. Kulin +3 more

Summary form only given. We have observed recombination into a large range of Rydberg levels in an ultracold plasma. The plasma is created by two-photon ionization of laser-trapped and -cooled metastable xenon atoms. By changing the intensity and detuning of the ionizing laser pulse, the initial temperature and density of the plasma can be varied. This allows us to access plasma coupling parameters (???) between 0.1 and 5. In this range of values, we previously reported unexplained heating of the expanding cloud, between 10 and 100 ???s after creation of the plasma. The recently observed recombination appears to provide much of the extra energy responsible for this behavior. The recombined atoms, up to 20% of the created plasma, populate energy levels down to n=40. They survive for /spl sim/1 ms indicating that high angular momentum states are present. However, standard scaling laws for three-body recombination do not agree with the observed dynamics. Furthermore, Rydberg atom formation is incomplete at the time when the plasma expansion velocity has reached its maximum value. Various effects are under consideration as possible remedies to these inconsistencies.

Quantum Electronics and Laser Science Conference•Nov 13, 2002•0 citations

Theoretical study of half-cycle pulse assisted ionization and recombination in Rydberg atoms

Julietta V. Rau

Bulletin of the American Physical Society•May 29, 2008•0 citations
Recent experiments have demonstrated the spontaneous evolution of a gas of ultracold Rydberg atoms into an expanding ultracold plasma, as well as the reverse process of plasma recombination into highly excited atomic states. Treating the evolution of the plasma on the basis of kinetic equations, while ionization/excitation and recombination are incorporated using rate equations, we have investigated theoretically the Rydberg-to-plasma transition. Including the influence of spatial correlations on the plasma dynamics in an approximate way, we find that ionic correlations change the results quantitatively but not qualitatively.
Summary form only given. We have observed recombination into a large range of Rydberg levels in an ultracold plasma. The plasma is created by two-photon ionization of laser-trapped and -cooled metastable xenon atoms. By changing the intensity and detuning of the ionizing laser pulse, the initial temperature and density of the plasma can be varied. This allows us to access plasma coupling parameters (???) between 0.1 and 5. In this range of values, we previously reported unexplained heating of the expanding cloud, between 10 and 100 ???s after creation of the plasma. The recently observed recombination appears to provide much of the extra energy responsible for this behavior. The recombined atoms, up to 20% of the created plasma, populate energy levels down to n=40. They survive for /spl sim/1 ms indicating that high angular momentum states are present. However, standard scaling laws for three-body recombination do not agree with the observed dynamics. Furthermore, Rydberg atom formation is incomplete at the time when the plasma expansion velocity has reached its maximum value. Various effects are under consideration as possible remedies to these inconsistencies.