Quantum physics

A ménage à trois laid bare

Quantum bodies that can't settle down together in pairs get on fine in a cosy threesome. This startling claim about the private life of particles has just seen its first experimental confirmation.

In 1970, Vitaly Efimov, possessor of a freshly minted Russian PhD in theoretical nuclear physics, predicted a bizarre quantum-mechanical effect1: a system consisting of three particles, none of whose two-particle subsystems is stable, can, under certain circumstances, produce an infinite number of bound energy levels. That prediction has been a source of concern for theorists ever since. Yet time and again, attempts to disprove the ‘Efimov effect’ have only verified its existence, albeit — until now — purely theoretically. In this issue, more than 35 years on from the initial prediction, Kraemer et al. (page 315)2 present the first convincing experimental evidence for the effect.

The question explored by Efimov was simple: if each possible pair of particles in a three-particle system is just shy of binding (so there are no bound states), what is the nature of the energy spectrum of the three particles? The answer, that the number of bound states in which the three particles can exist is infinite, is initially surprising. But it can be rationalized by noting that if two particles are already infinitesimally close to forming a bound state, just the faintest whiff of an additional attraction will be sufficient to push them over the edge to confederation. A third attracting particle accomplishes precisely that, no matter how far away from the other two it may roam, or how weak its additional attraction may be. Unsurprisingly, given this qualitative argument, three-body Efimov states have been theoretically found3 to be extremely ‘floppy’, with all imaginable triangular shapes — equilateral, isosceles, scalene (Fig. 1) — and even linear configurations being comparably probable.

Figure 1: Floppy triangles.
figure1

The Efimov-state probability density as a function of two ‘hyperangles’ that control the shape of the three-particle triangle. In this representation, the radius in any direction from the centre of the object measures the probability density of a particular triangular shape; the spikes indicate a somewhat higher probability for the system to exist in configurations where two of the three atoms are close to each other, whereas the near-spherical part of this object shows that all other triangle shapes occur with very comparable probabilities.

The Efimov effect is distantly related to Llewellyn Hilleth Thomas's 1935 proof4 that, in its ground state, a system of three particles that interact only within a vanishingly small range collapses to an infinitely small size, and its binding energy becomes infinitely large. Efimov discussed the link particularly clearly in a 1971 article5 that derived an effective potential-energy curve for such a system as a function of a three-particle ‘hyperradius’, R, which is proportional to the root-mean-square distance of the three particles from their centre of mass. The three-body potential-energy function turns out to be proportional to R−2, and it has a universal, negative coefficient of proportionality. The properties of such a potential are well known, because a similar form governs the motion of a charged particle in the field of a permanent dipole (where two charges of equal and opposite sign are separated by a small distance).

The allowed energy levels of a quantum system can be determined by solving the radial, time-independent Schrödinger equation (which yields the energy levels, En, of a quantum system). When the equation is solved for a system with an R−2 potential, the allowed energy levels that result follow on iteratively from each other according to the rule En+1=En exp(−2π/s0), where s0 is a constant related to the strength of the so-called effective dipole moment with a value slightly greater than one. Thus, as n increases, the binding energies of successive levels decrease exponentially. This scaling also carries over to other observable parameters, such as the size of the state. Thomas's collapsed states are the infinitely tightly bound states that occur as n approaches −, whereas the Efimov states are those states that are only just bound, arising as n approaches +. In real physical systems, the fact that the range of interparticle interactions can never be zero prevents a Thomas collapse, so this effect will, one presumes, never be observed. There is, however, no similar obstacle to observing the Efimov effect.

The strength of the interparticle interaction is described in terms of a parameter known as the scattering length, a. In a system consisting of two atoms, if a is large and positive, a weakly bound state of the diatomic molecule exists. If a is negative, the atoms experience an attraction but are not quite bound together. Kraemer and colleagues' experimental work2 relied on manipulating the atom–atom scattering length of caesium atoms by the now almost routine technique of tuning a magnetic field to a value very close to a ‘Feshbach resonance’ — a short-lived, low-energy, two-body molecular state6. Controlling the scattering length is crucial, as the formation of Efimov states is only expected for scattering lengths much greater in magnitude than the range of two-body interactions.

Kraemer and colleagues did not actually measure bound states at all, so the simplest ‘smoking gun’ evidence for Efimov states — a pattern of energy levels that fits the characteristic exponential formula — has yet to be observed. The authors studied instead the low-energy interactions of three ultracold caesium atoms, measuring the three-body recombination process Cs+Cs+Cs → Cs2+Cs, which had already been tackled theoretically7,8,9,10. Crucially, in 1999, Efimov states were predicted8 to show up as an infinite series of resonances in the rate of recombination at negative values of the scattering length, a link confirmed independently10 two years later.

Kraemer et al.2 saw only one such resonance (Fig. 2), at a scattering length of −850a0, where a0=0.53Å is the Bohr radius, a standard unit of distance in atomic physics. The fact that they did not see more (according to the theory, the next resonance should appear at a scattering length 22.7 times more negative, near a scattering length of −19,000a0) leaves them open to the charge that the effect could be some unrelated, non-Efimov three-body resonance effect, or even just a two-body effect.

Figure 2: Features predicted7,8,9,10,11 and observed2 in ultracold three-body recombination.
figure2

a, The theoretical rate (in terms of a ‘recombination length’8) of the three-body recombination process Cs+Cs+Cs → Cs2+Cs, obtained from numerical solutions of the three-body Schrödinger equation8,11 and plotted as a function of the two-body scattering length a (in units of the Bohr radius a0). The first interference minimum7,8,9,10,11 at a>0 and the first resonance maximum8,9,10 at a<0 — features predicted by theory — were observed by Kraemer et al.2 in their studies of caesium recombination. Insets b,c, the three-body potentials responsible for these features: the potential before recombination of three incident atoms at energy E (blue line) is shown in red; that after recombination, in black. b, For positive a, the transition between the two potentials takes place at a ‘hyperradius’ R a by one of two paths. First, the system ‘jumps’ into the lower recombined channel when still decreasing in size to R a. The atom then rebounds off the dimer (R increases) but the system remains in the recombined state (blue pathway). Second, the three atoms initially rebound elastically and only recombine in their outward traversal of R a (yellow path). Minima and maxima in the recombination rate arise from quantum-mechanical interference between these two paths in the outgoing channel (green arrow). c, For a<0, the transition occurs at R much smaller than |a|, and the system must tunnel quantum mechanically into the small-R potential well in order to recombine. When there are resonances (an allowed quasi-bound energy state, indicated by the horizontal red line) behind this barrier, the tunnelling probability is effectively enhanced, giving a maximum in the recombination rate. The resonance positions change with the scattering length (shown by the arrow), tuning the system in and out of resonance and yielding a series of peaks in the recombination length.

That interpretation is rendered unlikely, however, by the appearance of an interference minimum (Fig. 2) in the experimental spectrum at a positive scattering length, amin=210a0. Theoretical studies7,8,9,10 agree that, when Efimov physics occurs, a series of such minima in the three-body recombination should appear for large positive values of a. However, one study10 places the first minimum correctly to within 25% of the experimentally observed location2, even though its formula would not be expected to be valid at such low values of a. On the other hand, numerical solutions of the three-body Schrödinger equation8,11 place this minimum at a different location, near amin=1,500a0 (Fig. 2). Resolution of this disagreement will require further work.

Although the evidence is not yet conclusive, the appearance of both predicted phenomena — a resonance maximum8,10,11 and an interference minimum7,8,9,10,11 — implies strongly that Efimov physics has been observed. Developments in the theory are pointing the way to further experiments that would provide even more definitive confirmation11.

The Efimov effect, so long eluding observation, is beginning to yield up its secrets. As our theoretical understanding of Efimov states has deepened, so has our vision of their wider implications, such as those for the recombination physics studied by Kraemer et al.2. We look forward to seeing how the spark provided by this impressive new experiment ignites a new round of exploration into the rich quantum-mechanical world of exotic few-body systems.

References

  1. 1

    Efimov, V. Phys. Lett. B 33, 563–564 (1970).

    ADS  CAS  Article  Google Scholar 

  2. 2

    Kraemer, T. et al. Nature 440, 315–318 (2006).

    ADS  CAS  Article  Google Scholar 

  3. 3

    Esry, B. D., Lin, C. D. & Greene, C. H. Phys. Rev. A 54, 394–401 (1996).

    ADS  CAS  Article  Google Scholar 

  4. 4

    Thomas, L. H. Phys. Rev. 47, 903–909 (1935).

    ADS  CAS  Article  Google Scholar 

  5. 5

    Efimov, V. N. Sov. J. Nucl. Phys. 12, 589–595 (1971).

    Google Scholar 

  6. 6

    Inouye, S. et al. Nature 392, 151–154 (1998).

    ADS  CAS  Article  Google Scholar 

  7. 7

    Nielsen, E. & Macek, J. H. Phys. Rev. Lett. 83, 1566–1569 (1999).

    ADS  CAS  Article  Google Scholar 

  8. 8

    Esry, B. D., Greene, C. H. & Burke, J. P. Jr Phys. Rev. Lett. 83, 1751–1754 (1999).

    ADS  CAS  Article  Google Scholar 

  9. 9

    Bedaque, P. F., Braaten, E. & Hammer, H.-W. Phys. Rev. Lett. 85, 908–911 (2000).

    ADS  CAS  Article  Google Scholar 

  10. 10

    Braaten, E. & Hammer, H.-W. Phys. Rev. Lett. 87, 160407 (2001).

    ADS  CAS  Article  Google Scholar 

  11. 11

    D'Incao, J. P. & Esry, B. D. Phys. Rev. A (in the press); preprint at http://www.arxiv.org/cond-mat/0508474 (2006).

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Esry, B., Greene, C. A ménage à trois laid bare. Nature 440, 289–290 (2006). https://doi.org/10.1038/440289b

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