short communications
A classical Hanbury Brown–Twiss experiment with hard X-rays
aAdvanced Photon Source, Argonne National Laboratory, 9700 South Cass Avenue, Argonne, IL 60439, USA
*Correspondence e-mail: gluskin@aps.anl.gov
The classical Hanbury Brown–Twiss experiment has been conducted with hard X-ray synchrotron radiation at the Advanced Photon Source. The measured spatial coherence area of the X-ray beam is in good agreement with the prediction based on the vertical positron beam size.
Keywords: Hanbury Brown–Twiss experiment; hard X-rays.
1. Introduction
It has been discussed previously (Gluskin, 1991; Ikonen, 1992) that the high of third-generation synchrotron radiation sources could provide solid ground for measurement of the second degree of coherence of the radiation beams they produce. In recent years, several attempts to observe two photon correlations in synchrotron radiation have been made (Gluskin et al., 1994; Kunimune et al., 1997; Tai et al., 1998). Two of them succeeded, one in the hard X-ray wavelength range and one in the soft X-ray wavelength range. In both cases, sophisticated instrumentation and innovative approaches were applied, but only one significant data point was obtained in each experiment.
In this communication we describe the results of a classical Hanbury Brown–Twiss experiment (Hanbury Brown & Twiss, 1956) conducted at the 3-ID beamline of the Advanced Photon Source (APS). We measured the second degree of coherence, γ(2), in the vertical direction as a function of the distance between two slits, deployed in the X-ray beam, which allowed us to determine the vertical size of the positron beam at the APS storage ring.
2. Experiment
The experimental set-up is shown in Fig. 1. It consists of a double-crystal diamond (111) monochromator, a 3 µm-wide horizontal slit, a high-resolution Si crystal monochromator, an Si(111) crystal beam splitter operating in the Laue geometry, and two avalanche photodiodes (APDs) with vertical slit openings of 8 µm each to detect the split X-ray beams. During the experiment, the position of one detector was fixed while the other was moved vertically across the X-ray beam. The high-resolution monochromator uses Si(422) and Si() channel-cut crystals in a nested energy-dispersive arrangement (Ishikawa et al., 1992; Toellner et al., 1992; Mooney et al., 1994). This system yielded a 5.5 meV bandpass at an energy of 14.413 keV. The beam splitter efficiency was 32% using a 30 µm-thick crystal. The main parameters of the experimental set-up, positron and X-ray beams are summarized in Table 1. The coherence width was calculated by the formula
The coherence time was calculated using τc = λ2/Δλ.
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A schematic of the timing circuits used in the experiment is shown in Fig. 2. Analog pulses from the APDs were converted to proper timing signals by constant-fraction discriminators. The direct coincidence R3, provides random as well as correlated events, whereas the R4, gave only the random uncorrelated events. The delay time was adjusted to precisely one orbit period of the APS (3.683 µs).
The time resolution of the APDs was 1.5 ns, and the deadtime of the electronic delay was 15 ns, which resulted in negligibly small (less than 5 × 10−4) systematic errors for the filling pattern of the storage ring in which the positron bunches were 150 ns apart.
3. Results
Table 2 shows the results of the measurements. The ratio R3/R4 is equal to the value of the second degree of coherence, which was measured as a function of the APDs slits separation over a 48 µm range.
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Fig. 3 shows γ(2) as a function of the vertical slit separation. The HWHM of this function is approximately equal to 15 µm and, according to equation (1), it corresponds to 49 µm of the vertical positron beam size. The total measurement time for all data points was equal to 12.8 h. This was sufficient to obtain an acceptable level of statistical errors, i.e. the value of (1/R3 + 1/R4)1/2 was several times smaller than (R3/R4 − 1) for data points measured within the X-ray beam coherent area. In the future, more precise data may permit an analysis of the shape of the second-order coherence function.
Acknowledgements
We would like to acknowledge E. Trakhtenberg and R. Otto for the design and assembly of the slits, T. Toellner and P. Ilinski for help in conducting the experiment and data analysis. This work was supported by the US Department of Energy, Basic Energy Sciences, Office of Energy Research, under Contract No. W-31-109-ENG-38.
References
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