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

Annals of Physics

Number of bound states of three-body systems and Efimov's effect

Yu. N. Ovchinnikov, Israel Michael Sigal

Published Dec 1, 1979• 144 citations
Publisher
DOI
10.1016/0003-4916(79)90339-7

Related papers

Number of bound states of three-body systems and Efimov's effect

Theoretical Physics

Annals of Physics•Oct 1, 1979•2 citations

Efimov states and bound state properties in selected nuclear and molecular three-body systems

Harvey Stephen Huber

•Jan 1, 1978•0 citations

Efimov Physics in Heteronuclear Four-Body Systems

Yujun Wang, W. Blake Laing, Javier von Stecher +1 more

We study three- and four-body Efimov physics in a heteronuclear atomic system with three identical heavy bosonic atoms and one light atom. We show that exchange of the light atom between the heavy atoms leads to both three- and four-body features in the low-energy inelastic rate constants that trace to the Efimov effect. Further, the effective interaction generated by this exchange can provide an additional mechanism for control in ultracold experiments. Finally, we find that there is no true four-body Efimov effect-that is, no infinite number of four-body states in the absence of two- and three-body bound states-resolving a decades-long controversy.

arXiv:1109.1581•Physical Review Letters•Feb 15, 2012•29 citations

Number of eigenvalues of many-body Hamiltonians and Efimov's effect

Israel Michael Sigal

Springer eBooks•Apr 6, 2008•4 citations

Universal equation for Efimov states

Eric Braaten, H.‐W. Hammer, Masaoki Kusunoki

Efimov states are a sequence of shallow three-body bound states that arise when the two-body scattering length is large. Efimov showed that the binding energies of these states can be calculated in terms of the scattering length and a three-body parameter by solving a transcendental equation involving a universal function of one variable. We calculate this universal function using effective field theory and use it to describe the three-body system of ${}^{4}\mathrm{He}$ atoms. We also extend Efimov's theory to include the effects of deep two-body bound states, which give widths to the Efimov states.

arXiv:cond-mat/0201281•Physical Review A•Feb 28, 2003•54 citations

Efimov states: what are they and why are they important?

J. H. Macek

The interaction of two atoms at energies in the microkelvin range is mainly characterized by one parameter, namely, the s-wave scattering length. Efimov showed that when the scattering length was effectively infinite, i.e. much larger than the natural length scale of the atoms, a large number of three-body bound states could form even when the two-body system supported only one weakly bound state, or possibly none at all. The states are bound in an effective 1/ R 2 potential and therefore form a series with a characteristic energy spacing. These states are called Efimov states and are conceptually important since they indicate a new way to form aggregates of particles. They bear some relation to vibrationally bound states of three atoms. The theory of these states and their relation to vibrational binding is reviewed in light of recent experimental measurements.

Physica Scripta•Jul 13, 2007•6 citations
We study three- and four-body Efimov physics in a heteronuclear atomic system with three identical heavy bosonic atoms and one light atom. We show that exchange of the light atom between the heavy atoms leads to both three- and four-body features in the low-energy inelastic rate constants that trace to the Efimov effect. Further, the effective interaction generated by this exchange can provide an additional mechanism for control in ultracold experiments. Finally, we find that there is no true four-body Efimov effect-that is, no infinite number of four-body states in the absence of two- and three-body bound states-resolving a decades-long controversy.
Efimov states are a sequence of shallow three-body bound states that arise when the two-body scattering length is large. Efimov showed that the binding energies of these states can be calculated in terms of the scattering length and a three-body parameter by solving a transcendental equation involving a universal function of one variable. We calculate this universal function using effective field theory and use it to describe the three-body system of 4He{}^{4}\mathrm{He}4He atoms. We also extend Efimov's theory to include the effects of deep two-body bound states, which give widths to the Efimov states.
The interaction of two atoms at energies in the microkelvin range is mainly characterized by one parameter, namely, the s-wave scattering length. Efimov showed that when the scattering length was effectively infinite, i.e. much larger than the natural length scale of the atoms, a large number of three-body bound states could form even when the two-body system supported only one weakly bound state, or possibly none at all. The states are bound in an effective 1/ R 2 potential and therefore form a series with a characteristic energy spacing. These states are called Efimov states and are conceptually important since they indicate a new way to form aggregates of particles. They bear some relation to vibrationally bound states of three atoms. The theory of these states and their relation to vibrational binding is reviewed in light of recent experimental measurements.