Hanbury Brown and Twiss effect

The Hanbury Brown and Twiss (HBT) effect is any of a variety of correlation and anti-correlation effects in the intensities received by two detectors from a beam of particles. HBT effects can generally be attributed to the dual wave-particle nature of the beam, and the results of a given experiment depend on whether the beam is composed of fermions or bosons. Devices which utilize the effect are commonly called intensity interferometers and were originally used in astronomy, although they are also heavily used in the field of quantum optics.

History

In 1956, Robert Hanbury Brown and Richard Q. Twiss published A test of a new type of stellar interferometer on Sirius, in which two photomultiplier tubes (PMTs), separated by about 6 meters, were aimed at the star Sirius. Light was collected into the PMTs using mirrors from searchlights. An interference effect was observed between the two intensities, revealing a positive correlation between the two signals, despite the fact that no phase information was collected. Hanbury Brown and Twiss used the interference signal to determine the apparent angular size of Sirius, claiming excellent resolution.

Also, in the field of particle physics, Goldhaber et al. performed an experiment in 1959 in Berkeley and found an unexpected angular correlation among identical pions, in order to discover the ρ⁰ resonance (by means of $\rho ^{0}\rightarrow \pi ^{-}\pi ^{+}$) [Phys.Rev.Lett.3,181(1959)]. From then on, the HBT technique started to be used in particular by the heavy-ion community to determine the space-time dimensions of the particle emission source for heavy ion collisions. For recent developments in this field, cf. for example the review article by Lisa [M.Lisa,et al., Ann.Rev.Nucl.Part.Sci 55, 357(2005), or, [1].

An example of an intensity interferometer that would observe no correlation if the light source is a coherent laser beam, and positive correlation if the light source is a filtered one-mode thermal radiation. The theoretical explanation of the difference between the correlations of photon pairs in thermal and in laser beams was first given by Roy J. Glauber, who was awarded the 2005 Nobel Prize in Physics "for his contribution to the quantum theory of optical coherence".

The original HBT result met with much skepticism in the physics community. Although intensity interferometry had been widely used in radio astronomy where Maxwell's equations are valid, at optical wavelengths the light would be quantised into a relatively small number of photons. Many physicists worried that the correlation was inconsistent with the laws of thermodynamics. Some even claimed that the effect violated the uncertainty principle. Hanbury Brown and Twiss resolved the dispute in a neat series of papers (see References below) which demonstrated first that wave transmission in quantum optics had exactly the same mathematical form as Maxwell's equations albeit with an additional noise term due to quantisation at the detector, and secondly that according to Maxwell's equations, intensity interferometry should work. Others, such as Edward Mills Purcell immediately supported the technique, pointing out that the clumping of bosons was simply a manifestation of an effect already known in statistical mechanics. After a number of experiments, the whole physics community agreed that the observed effect was real.

The original experiment used the fact that two bosons tend to arrive at two separate detectors at the same time. Morgan and Mandel used a thermal photon source to create a dim beam of photons and observed the tendency of the photons to arrive at the same time on a single detector. Both of these effects used the wave nature of light to create a correlation in arrival time - if a single photon beam is split into two beams, then the particle nature of light requires that each photon is only observed at a single detector, and so an anti-correlation was observed in 1986. Finally, bosons have a tendency to clump together, giving rise to Bose–Einstein correlations, while fermions due to the Pauli exclusion principle, tend to spread apart leading to Fermi–Dirac (anti)correlations. Bose–Einstein correlations have been observed between pions, kaons and photons, and Fermi–Dirac (anti)correlations between protons, neutrons and electrons. For a general introduction in this field cf. the textbook on Bose–Einstein correlations by Richard M. Weiner It must be noted, that a difference in repulsion of BECs in the "trap-and-free fall" analogy of the HBT effect affects comparison.

Wave mechanics

The HBT effect can in fact be predicted solely by treating the incident electromagnetic radiation as a classical wave. Suppose we have a single incident wave with frequency $\omega$ on two detectors. Since the detectors are separated, say the second detector gets the signal delayed by a phase of $\phi$. Since the intensity at a single detector is just the square of the wave amplitude, we have for the intensities at the two detectors

$i_{1}=E^{2}\sin ^{2}(\omega t)\,$

$i_{2}=E^{2}\sin ^{2}(\omega t+\phi )=E^{2}(\sin(\omega t)\cos(\phi )+\sin(\phi )\cos(\omega t))^{2}\,$

which makes the correlation

$\langle i_{1}i_{2}\rangle =\lim _{T\rightarrow \infty }{\frac {E^{4}}{T}}\int _{0}^{T}\sin ^{2}(\omega t)(\sin(\omega t)\cos(\phi )+\sin(\phi )\cos(\omega t))^{2}\,dt$

$={\frac {E^{4}}{4}}+{\frac {E^{4}}{8}}\cos(2\phi ),$

a constant plus a phase dependent component. Most modern schemes actually measure the correlation in intensity fluctuations at the two detectors, but it is not too difficult to see that if the intensities are correlated then the fluctuations $\Delta i=i-\langle i\rangle$, where $\langle i\rangle$ is the average intensity, ought to be correlated. In general

$\langle \Delta i_{1}\Delta i_{2}\rangle =\langle (i_{1}-\langle i_{1}\rangle )(i_{2}-\langle i_{2}\rangle )\rangle =\langle i_{1}i_{2}\rangle -\langle i_{1}\langle i_{2}\rangle \rangle -\langle i_{2}\langle i_{1}\rangle \rangle +\langle i_{1}\rangle \langle i_{2}\rangle$

$=\langle i_{1}i_{2}\rangle -\langle i_{1}\rangle \langle i_{2}\rangle ,$

and since the average intensity at both detectors in this example is $E^{2}/2$,

$\langle \Delta i_{1}\Delta i_{2}\rangle ={\frac {E^{4}}{8}}\cos(2\phi ),$

so our constant vanishes. The average intensity is $E^{2}/2$ because the time average of $\sin ^{2}(\omega t)$ is 1/2.

An evaluation of a degree of the second-order coherence for complementary (anti-correlated) outputs of an interferometer leads to behaviour like "anti-bunching effect". For example a variation in reflectivity (and thus also in transmittance) of beam splitter, where

$i_{1}=i_{r}\$

$i_{2}=i_{t}=i-i_{r}\,$

results in the negative correlation of fluctuations

$\langle \Delta i_{1}\Delta i_{2}\rangle =-{\frac {E^{4}}{8}}\cos(2\phi ),$

i.e. a dip in the coherence function $g^{(2)}(\tau )$.

Quantum Interpretation

Photon detections as a function of time for a) antibunching (e.g. light emitted from a single atom), b) random (e.g. a coherent state, laser beam), and c) bunching (chaotic light). τ_c is the coherence time (the time scale of photon or intensity fluctuations).

The above discussion makes it clear that the Hanbury Brown and Twiss (or photon bunching) effect can be entirely described by classical optics. The quantum description of the effect is less intuitive: if one supposes that a thermal or chaotic light source such as a star randomly emits photons, then it is not obvious how the photons "know" that they should arrive at a detector in a correlated (bunched) way. A simple argument suggested by Ugo Fano [Fano, 1961] captures the essence of the quantum explanation. Consider two points $a$ and $b$ in a source which emit photons detected by two detectors $A$ and $B$ as in the diagram. A joint detection takes place when the photon emitted by $a$ is detected by $A$ and the photon emitted by $b$ is detected by $B$ (red arrows) or when $a$'s photon is detected by $B$ and $b$'s by $A$ (green arrows). The quantum mechanical probability amplitudes for these two possibilities are denoted by $\langle A|a\rangle \langle B|b\rangle$ and $\langle B|a\rangle \langle A|b\rangle$ respectively. If the photons are indistinguishable, the two amplitudes interfere constructively to give a joint detection probability greater than that for two independent events. The sum over all possible pairs $a$,$b$ in the source washes out the interference unless the distance $AB$ is sufficiently small.

Two source points a and b emit photons detected by detectors A and B. The two colors represent two different ways to detect two photons.

Fano's explanation nicely illustrates the necessity of considering two particle amplitudes, which are not as intuitive as the more familiar single particle amplitudes used to interpret most interference effects. This may help to explain why some physicists in the 1950s had difficulty accepting the Hanbury Brown Twiss result. But the quantum approach is more than just a fancy way to reproduce the classical result: if the photons are replaced by identical fermions such as electrons, the antisymmetry of wavefunctions under exchange of particles renders the interference destructive, leading to zero joint detection probability for small detector separations. This effect is referred to as antibunching of fermions [Henny, 1999]. The above treatment also explains photon antibunching [Kimble, 1977]: if the source consists of a single atom which can only emit one photon at a time, simultaneous detection in two closely spaced detectors is clearly impossible. Antibunching, whether of bosons or of fermions, has no classical wave analog.

From the point of view of the field of quantum optics, the importance of the HBT effect was that it led people (among them Roy J. Glauber and Leonard Mandel) to apply quantum electrodynamics to new situations, many of which had never been experimentally studied, and in which classical and quantum predictions differ.

See also

• Timeline of electromagnetism and classical optics
• Degree of coherence
• Bose–Einstein correlations

References

Note that Hanbury Brown is not hyphenated.

• E. Brannen, H. Ferguson (1956). "The question of correlation between photons in coherent light beams". Nature. 178 (4531): 481. doi:10.1038/178481a0. - paper which (incorrectly) disputed the existence of the Hanbury Brown and Twiss effect

• R. Hanbury Brown and R. Q. Twiss (1956). "A Test of a New Type of Stellar Interferometer on Sirius". Nature. 178 (4541): 1046–1048. doi:10.1038/1781046a0. - experimental demonstration of the effect

• E. Purcell (1956). "The Question of Correlation Between Photons in Coherent Light Rays". Nature. 178 (4548): 1449–1450. doi:10.1038/1781449a0.

• R. Hanbury Brown and R. Q. Twiss (1957). "Interferometry of the intensity fluctuations in light. I. Basic theory: the correlation between photons in coherent beams of radiation". Proc of the Royal Society of London A. 242 (1230): 300–324. doi:10.1098/rspa.1957.0177. download as PDF

• R. Hanbury Brown and R. Q. Twiss (1958). "Interferometry of the intensity fluctuations in light. II. An experimental test of the theory for partially coherent light". Proc of the Royal Society of London A. 243 (1234): 291–319. doi:10.1098/rspa.1958.0001. download as PDF

• Fano, U. (1961). "Quantum theory of interference effects in the mixing of light from phase independent sources". American Journal of Physics. 29 (8): 539. doi:10.1119/1.1937827.

• B. L. Morgan and L. Mandel (1966). "Measurement of Photon Bunching in a Thermal Light Beam". Phys. Rev. Lett. 16 (22): 1012–1014. doi:10.1103/PhysRevLett.16.1012.

• Kimble, H.; Dagenais, M.; Mandel, L. (1977). "Photon antibunching in resonance fluorescence". Physical Review Letters. 39 (11): 691. doi:10.1103/PhysRevLett.39.691.

• P. Grangier, G. Roger, and A. Aspect (1986). "Experimental Evidence for a Photon Anticorrelation Effect on a Beam Splitter: A New Light on Single-Photon Interferences". Europhysics Letters. 1 (4): 173–179. doi:10.1209/0295-5075/1/4/004.{{cite journal}}: CS1 maint: multiple names: authors list (link)

• M. Henny; et al. (1999). "The Fermionic Hanbury Brown and Twiss Experiment". Science. 284 (5412): 296–298. doi:10.1126/science.284.5412.296. PMID 10195890. {{cite journal}}: Explicit use of et al. in: |author= (help)

• R Hanbury Brown (1991). BOFFIN : A Personal Story of the Early Days of Radar, Radio Astronomy and Quantum Optics. Adam Hilger. ISBN 0-7503-0130-9.

• Mark P. Silverman (1995). More Than One Mystery: Explorations in Quantum Interference. Springer. ISBN 0-387-94376-5.

• R Hanbury Brown (1974). The intensity interferometer; its application to astronomy. Wiley. ISBN 0470107979. ASIN B000LZQD3C.

• Y. Bromberg, Y. Lahini, E. Small and Y. Silberberg (2010). "Hanbury Brown and Twiss Interferometry with Interacting Photons". Nature Photonics. 4 (10): 721–726. doi:10.1038/nphoton.2010.195.{{cite journal}}: CS1 maint: multiple names: authors list (link)

External links

• http://adsabs.harvard.edu//full/seri/JApA./0015//0000015.000.html
• http://physicsweb.org/articles/world/15/10/6/1
• http://www.du.edu/~jcalvert/astro/starsiz.htm
• http://www.2physics.com/2010/11/hanbury-brown-and-twiss-interferometry.html