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Geology

Article: pp. 83–86 | Full Text | PDF (852K)

Using phosphorescence as a fingerprint for the Hope and other blue diamonds

Sally Eaton-Magaña1, Jeffrey E. Post2, Peter J. Heaney3, Jaime Freitas4, Paul Klein4, Roy Walters5, and James E. Butler6

1. Naval Research Laboratory, 4555 Overlook Ave. SW, Washington, DC 20375, USA, 2. Department of Mineral Sciences, Smithsonian Institution, Washington, DC 20560, USA, 3. Department of Geosciences, Pennsylvania State University, University Park, Pennsylvania 16802, USA, 4. Naval Research Laboratory, 4555 Overlook Ave. SW, Washington, DC 20375, USA, 5. Ocean Optics Inc., 830 Douglas Avenue, Dunedin, Florida 34698, USA, 6. Naval Research Laboratory, 4555 Overlook Ave. SW, Washington, DC 20375, USA

Sixty-seven natural blue diamonds, including the two largest such gemstones known (the Hope and the Blue Heart), were probed by ultraviolet radiation, and their luminescence was analyzed using a novel spectrometer system. Prior to this study, the fiery red phosphorescence of the Hope Diamond was regarded as quite rare compared to greenish-blue phosphorescence. However, our results demonstrated that virtually all blue diamonds phosphoresce at 660 nm (orange-red) but that this emission often is obscured by a concomitant luminescence at 500 nm (green-blue). Although both bands were nearly always present, the relative intensities of these emissions and their decay kinetics varied dramatically. Consequently, phosphorescence analysis provides a method to discriminate among individual blue diamonds. Treated and synthetic blue diamonds showed behavior distinct from natural stones. Temperature-dependent phosphorescence revealed that the 660 nm emission has an activation energy of 0.4 eV, close to the 0.37 eV acceptor energy for boron, suggesting that the phosphorescence is caused by donor-acceptor pair recombination.

Keywords: phosphorescence, type-IIb diamond, donor-acceptor pair recombination, fingerprinting

Received: 11 June 2007; Revised: 5 September 2007; Accepted: 6 September 2007

DOI: 10.1130/G24170A.1

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