Abstract
The effect of a magnetic field on an atom has been studied for a long time and has played a crucial role in the understanding of atomic physics. The magnetic fields available in the laboratory are small, however; their action in the atom used to be well explained by perturbation theory. The evidence for strong magnetic fields was first found by the astronomers in white dwarfs some twenty years ago, and extremely strong fields are assumed to exist in neutron stars. This discovery led to laboratory experiments that somehow manage to imitate the extraordinary conditions in these exceptional stars.
Keywords
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.
This is a preview of subscription content, log in via an institution.
Buying options
Tax calculation will be finalised at checkout
Purchases are for personal use only
Learn about institutional subscriptionsPreview
Unable to display preview. Download preview PDF.
Author information
Authors and Affiliations
Rights and permissions
Copyright information
© 1990 Springer Science+Business Media New York
About this chapter
Cite this chapter
Gutzwiller, M.C. (1990). The Diamagnetic Kepler Problem. In: Chaos in Classical and Quantum Mechanics. Interdisciplinary Applied Mathematics, vol 1. Springer, New York, NY. https://doi.org/10.1007/978-1-4612-0983-6_19
Download citation
DOI: https://doi.org/10.1007/978-1-4612-0983-6_19
Publisher Name: Springer, New York, NY
Print ISBN: 978-1-4612-6970-0
Online ISBN: 978-1-4612-0983-6
eBook Packages: Springer Book Archive