1944
DOI: 10.1007/bf03173450
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The fluorescence and absorption spectra of diamond in the visible region

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Cited by 33 publications
(7 citation statements)
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“…The best estimate of the energy and wavelength at its maximum is 2.396 eV (518 nm), which is 65 meV lower in energy than the zero-phonon line. The diffuse phononassisted peaks resolved on the long wavelength side of the 504 nm line in figure 12, on the other hand, have the spacing of about 40 meV that is a well documented feature of the H3 system (Mani 1944a;Dyer & Matthews 1957;Dean et al i960). A further distinction between these two emission systems is that whereas the H3 system (at least when associated with platelets and dislocations) saturates at high specimen current densities (as already described in §4 (a) and §4(£)) the system shown in figure 13 presented no obvious signs of saturating, even at current densities as high as 1 mA mm-2.…”
Section: (D) Regions Contiguous With External Surfacesmentioning
confidence: 89%
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“…The best estimate of the energy and wavelength at its maximum is 2.396 eV (518 nm), which is 65 meV lower in energy than the zero-phonon line. The diffuse phononassisted peaks resolved on the long wavelength side of the 504 nm line in figure 12, on the other hand, have the spacing of about 40 meV that is a well documented feature of the H3 system (Mani 1944a;Dyer & Matthews 1957;Dean et al i960). A further distinction between these two emission systems is that whereas the H3 system (at least when associated with platelets and dislocations) saturates at high specimen current densities (as already described in §4 (a) and §4(£)) the system shown in figure 13 presented no obvious signs of saturating, even at current densities as high as 1 mA mm-2.…”
Section: (D) Regions Contiguous With External Surfacesmentioning
confidence: 89%
“…( a) Lines associated with slip traces Two line emissions registered on spectra from H3 system-emitting regions of specimen GH2 appear at 2.55 eV (485 nm) and 2.30 eV (540 nm). Since the work of Mani (1944a) the latter line has been several times reported as accompanying the H3 system, for example by Dean et al (i960) in low-temperature cathodoluminescence studies. During the present observations it was often noted by visual spectroscopy when it accompanied the H3 emission in various crystals; and it sometimes appeared with sufficient strength to stand out sharply above the strong background given at room temperature by the phonon-assisted peaks of the H3 system.…”
Section: O Ther Spectral Lines With Topographically Defined Associationsmentioning
confidence: 91%
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“…The same N3 center is also responsible for blue long-wave ultraviolet fluorescence when seen in type Ia diamonds (Nayar, 1941;Mani, 1944;Dyer and Matthews, 1957). Based largely on observations with the prism spectroscope, Anderson (1943aAnderson ( ,b, 1962 noted the general correlation between the intensity of the 415 nm absorption band and the strength of the diamond's yellow color (also see Anderson and Payne, 1956).…”
Section: Introductionmentioning
confidence: 97%
“…Fluorescence in diamonds has been studied for nearly a century (e.g., Becquerel, 1868;Mani, 1944;Shipley, 1947;Wild and Biegel, 1947;Cotty, 1956;Dyer and Matthews, 1958;Collins, 1974Collins, , 1982Fritsch and Waychunas, 1994;Eaton-Magaña et al, 2007;Holloway, 2009;Shigley and Breeding, 2013). While much is known and published about diamond defects and fluorescence, most gemologists do not have ready access to this information.…”
mentioning
confidence: 99%