Rydberg atom

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A Rydberg atom is an excited atom with one or more electrons that have a very high principal quantum number. These atoms have a number of peculiar properties including an exaggerated response to electric and magnetic fields, long decay periods and electron wavefunctions that approximate under some conditions classical orbits of electrons about the nuclei.

In spite of its shortcomings, the Bohr model of the atom is useful in explaining these properties. Classically an electron in a circular orbit of radius r, about a nucleus of charge Ze, obeys Newton's second law:

\mathbf{F}=m\mathbf{a} \Rightarrow {kZe^2 \over r^2}={mv^2 \over r}

where k = 1/(4πε0).

Orbital momentum is quantised in units of \hbar:

mvr=n\hbar

Combining these two equations leads to Bohr's expression for the orbital radius in terms of the principal quantum number n:

r={n^2\hbar^2 \over kZe^2m}

It is now apparent why Rydberg atoms have such peculiar properties; the radius of the orbit scales as n2 (the n = 137 state of hydrogen has an atomic radius ~1µm) and the geometric cross-section as n4. Thus Rydberg atoms are extremely large with loosely bound valence electrons, easily perturbed or ionised by collisions or external fields.

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[edit] The classical view of Rydberg atoms

An atom in a Rydberg state has a valence electron in a large orbit far from the ion core; in such an orbit the outermost electron feels an almost hydrogenic, 1/r coulomb potential from a compact ion core consisting of a nucleus with Z protons and the lower electron shells filled with Z−1 electrons.

Coulombic 1/r potential.
Coulombic 1/r potential.

The similarity of the effective potential ‘seen’ by the outer electron to the hydrogen potential is a defining characteristic of Rydberg states and explains why the electron wavefunctions approximate to classical orbits. There are three notable exceptions:

  • An atom may have two (or more) electrons in highly excited states with comparable orbital radii. In this case the electron-electron interaction gives rise to a significant deviation from the hydrogen potential.
  • If the valence electron has very low angular momentum (interpreted classically as an extremely eccentric elliptical orbit) then it may pass close enough to polarise the ion core, giving rise to a 1/r3 dipole term in the potential:
V \propto {A \over r} + {B \over r^3}

where A & B are constants.

  • If the outer electron penetrates the inner electron shells, it will 'see' more of the charge of the nucleus and hence experience a greater force.

[edit] The quantum mechanical picture

Quantum mechanically a state of high n refers to an atom in which the valence electron(s) have been excited into a formerly unpopulated electron orbital with higher energy and lower binding energy:

E_B \propto {1 \over n^2}

This explains why Rydberg states are susceptible to ionisation.

The long lifetimes of Rydberg states with high orbital angular momentum can be explained in terms of the overlapping of wavefunctions. The wavefunction of an electron in a high l state (high angular momentum) has very little overlap with the wavefunctions of the inner electrons and hence remains relatively unperturbed.

The three exceptions to the definition of a Rydberg atom as an atom with a hydrogenic potential, have an alternative, quantum mechanical explanation:

  • If a second electron is excited into a state ni, energetically close to the state of the outer electron no, then its wavefunction become almost as large as the first (a double Rydberg state). This occurs as ni approaches no and leads to a condition where the size of the two electron’s orbits are related; a condition referred to as radial correlation[1].
  • Polarization of the ion core produces an anisotropic dipole potential that causes an angular correlation[2] between the motions of the two outermost electrons. This can be thought of as a tidal locking effect due to a non-spherically symmetric potential.
  • The wavefunction of the outer electron in states with low orbital angular momentum l, is periodically localised within the shells of inner electrons and interacts with the full charge of the nucleus.

[edit] What makes Rydberg atoms worth studying?

[edit] Experimental atomic physics

Although the interesting nature of Rydberg atoms has been understood since the development of the Bohr model in 1913, for a long time there was no efficient method for producing large, single-state, mono-energetic populations. There were a number of interesting experiments done in the 1950s and 1960s using electron impact excitation:

e^- + A \rarr A^* + e^-

and charge exchange excitation:

A^+ + B \rarr A^* + B^+

but these techniques both produce populations with a very broad spread of energies.

The arrival of tunable dye lasers in the 1970s allowed a much greater level of control over populations of excited atoms. In optical excitation the incident photon is absorbed by the atom, thus absolutely specifying the energy of the state produced.

The precise control over atomic states allowed by optical excitation has played a significant role in advancing our understanding of atomic Rydberg states.

[edit] Investigating diamagnetic effects

The large sizes and low binding energies of Rydberg atoms lead to a high magnetic susceptibility Χ. As diamagnetic effects scale with the area of the orbit and the area is proportional to the radius squared \Rightarrow A \propto n^4, effects impossible to detect in ground state atoms become obvious in Rydberg atoms, which demonstrate very large diamagnetic shifts.

[edit] Rydberg atoms in plasmas

Rydberg atoms form commonly in plasmas due to the recombination of electrons and positive ions; low energy recombination results in fairly stable Rydberg atoms, while recombination of electrons and positive ions with high kinetic energy often form autoionising Rydberg states. Rydberg atoms’ large sizes and susceptibility to perturbation and ionisation by electric and magnetic fields, are an important factor determining the properties of plasmas.

[edit] Rydberg atoms in astrophysics

In the time between the early absorption spectroscopy experiments and the arrival of tunable lasers, interest in Rydberg atoms was kept alive by the realisation that they are common in interstellar space, and as such are an important radiation source for astronomers.

The density within interstellar gas clouds is typically many orders of magnitude lower than the best laboratory vacuums attainable on Earth, allowing Rydberg atoms to persist for long periods of time without being ionised by collisions or electric and magnetic fields. As a result of this longevity and the abundance of hydrogen it is particularly common for astronomers to observe radiation from the heavens at a frequency of 2.4 GHz, now known to correspond to the hydrogen n = 109 to n = 108 transition. Such a highly excited hydrogen atom on Earth would be ionised almost immediately as the binding energy would be significantly below thermal energies.

[edit] Classical simulation of a Rydberg atom

A simple 1/r potential results in a closed Keplerian elliptical orbit, however the large electric dipole moment of a Rydberg atom makes them extremely susceptible to electric fields.

Stark - Coulomb potential for a Rydberg atom in a static electric field.
Stark - Coulomb potential for a Rydberg atom in a static electric field.

Application of an external electric field (known in atomic physics as a Stark field) changes the geometry of the potential and dramatically changes the behaviour of the electron.

A Coulombic potential does not apply any torque as the force is always antiparallel to the position vector (i.e. always pointing along a line running between the electron and the nucleus):

\mathbf{\tau}=\mathbf{r} \times \mathbf{F}=|\mathbf{r}||\mathbf{F}|\sin\theta
\theta=\pi \Rightarrow \mathbf{\tau}=0

With the application of a static electric field, the electron feels a continuously changing torque. The resulting trajectory becomes progressively more distorted over time, eventually going through the full range of angular momentum from [L=LMAX], to a straight line [L=0], to the initial orbit in the opposite sense [L= —LMAX].

The time period of the oscillation in angular momentum (the time to complete the trajectory in the figure below), almost exactly matches the quantum mechanically predicted period for the wavefunction to return to its initial state, demonstrating the classical nature of the Rydberg atom.

Trajectory of the outer electron of a Rydberg atom in a static electric field.
Trajectory of the outer electron of a Rydberg atom in a static electric field.

[edit] See also

[edit] References

  • ↑ Gallagher, Thomas F. (1994). in A. Dalgarno, F. H. Read, R. N. Zare: Rydberg Atoms. Cambridge: Cambridge University Press. ISBN 0-521-38531-8. 

[edit] External links

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