Related Experiment Video
Updated: Jun 12, 2026

16:20
Hyperpolarized Xenon for NMR and MRI Applications
Published on: September 6, 2012
Stabilization of helium in intense xuv laser fields
T Birkeland1, R Nepstad, M Førre
1Department of Mathematics, University of Bergen, N-5007 Bergen, Norway.
Physical Review Letters
|May 21, 2010
Summary
Electron-electron repulsion in helium atoms negatively impacts atomic stabilization in intense laser fields, especially with short pulses. Double ionization shows the clearest stabilization signature, unlike simplified models.
Area of Science:
- Quantum mechanics
- Atomic physics
- Strong-field laser physics
Background:
- Atomic stabilization is a phenomenon where atoms exposed to intense laser fields become less likely to ionize.
- Electron-electron correlation, the interaction between electrons, is crucial in multi-electron systems like helium.
Purpose of the Study:
- To investigate the influence of electron-electron correlation on helium ionization dynamics in high-frequency laser fields.
- To analyze the effect of electron repulsion on atomic stabilization, particularly for short laser pulses.
Main Methods:
- Solving the time-dependent Schrödinger equation from first principles for helium atoms.
- Simulating ionization dynamics under intense, high-frequency laser fields.
Main Results:
- Observed a decrease in total ionization yield at high field strengths, indicating atomic stabilization.
- Found that electron-electron repulsion detrimentally affects the degree of stabilization, especially for short pulses.
- Double ionization channels showed a more distinct stabilization signature, being less affected by two-electron effects.
Conclusions:
- Electron-electron correlation significantly modifies ionization dynamics and stabilization in helium.
- One-dimensional models commonly used to study correlation effects tend to overestimate their impact.
- Double ionization is a more robust indicator of stabilization in the presence of electron correlation.
More Related Videos
Related Concept Videos
Nuclear Fusion
The process of converting very light nuclei into heavier nuclei is also accompanied by the conversion of mass into large amounts of energy, a process called fusion. The principal source of energy in the sun is a net fusion reaction in which four hydrogen nuclei fuse and ultimately produce one helium nucleus and two positrons.
A helium nucleus has a mass that is 0.7% less than that of four hydrogen nuclei; this lost mass is converted into energy during the fusion. This reaction produces about...
A helium nucleus has a mass that is 0.7% less than that of four hydrogen nuclei; this lost mass is converted into energy during the fusion. This reaction produces about...
Noble Gases
The elements in group 18 are noble gases (helium, neon, argon, krypton, xenon, and radon). They earned the name “noble” because they were assumed to be nonreactive since they have filled valence shells. In 1962, Dr. Neil Bartlett at the University of British Columbia proved this assumption to be false.
Nuclear Binding Energy
The difference between the calculated and experimentally measured masses is known as the mass defect of the atom. In the case of helium-4, the mass defect indicates a “loss” in mass of 4.0331 amu – 4.0026 amu = 0.0305 amu. The loss in mass accompanying the formation of an atom from protons, neutrons, and electrons is due to the conversion of that mass into energy that is evolved as the atom forms. The nuclear binding energy is the energy produced when the atoms’ nucleons are bound together;...

