DOPED OPTICAL WAVEGUIDE AMPLIFIER

Abstract: The core of a low phonon energy glass optical fibre is doped with trivalent Dysprosium ions (Dy<3+>) for application as an efficient optical fibre amplifier operating around 1.3 mu m. The device utilises the transition <6>H9/2-<6>F11/2 to <6>H15/2. The low phonon energy (high quantum efficiency) glasses include mixed halides, chalcogenides and chalcohalides. Improvements in efficiency can be achieved by co-doping of the fibre core with Eu<3+> and/or Tb<3+> ions.

Description: DOPED OPTICAL WAVEGUIDE AMPLIFIER This invention relates to doped optical waveguide amplifiers. Optical waveguide amplifiers, and in particular optical fibre amplifiers, are used widely in the telecommunications industry. An example of an optical fibre amplifier is the erbium doped fibre amplifier (EDFA) which operates in the so-called third telecoms window (wavelengths around 1500 nanometres (nm) ) . These devices are characterised by their high gain (around 30 decibels (dB)) achieved with limited pump power (less than 50 milliwatts (mW)), which means that pumping can be performed using a single laser diode unit. However, in the important second telecoms window (wavelengths around 1300 nm) , known optical fibre amplifiers operate with a much lower efficiency. The best performance reported so far has been obtained using trivalent Praseodymium (Pr 3* ) doped fluoride fibre amplifiers (PDFFAs), which achieve a small signal gain of about 23dB with about 120mW of pump from a single semiconductor laser diode unit. Operating the pump diode at high drive current to achieve this pump power can severely curtail the lifetime of the diode. This problem has limited the application of this amplifier unit. Application of PDFFAs as high output power amplifiers using solid state neodymium-yttrium-lanthanum-fluoride (Nd:YLF) lasers as the pump source have achieved a higher operating efficiency than the diode pumped device. However, the use of an expensive solid state laser for pumping the fibre amplifier is far from ideal for many applications such as in-line optical fibre amplifiers. It has been proposed to use dysprosium as a dopant in optical waveguide amplifiers. In EP-A-0570743 fluoride or silica (Si0 2 ) glass fibres are doped with dysprosium (Dy 3* ) ions to provide a 1300nm optical amplifier. This invention provides an optical waveguide amplifier comprising a glass optical waveguide doped with dysprosium ions, the glass having a maximum phonon energy of less than 4 0 cm "1 , (cm is an abbreviation for centimetre) . This invention also provides an optical waveguide amplifier comprising a glass optical waveguide doped with dysprosium ions, such that the quantum efficiency of the H g/2 - F u/2 doublet of dysprosium ions in the waveguide is at least 5% - This invention also provides an optical waveguide amplifier comprising a glass optical waveguide doped with dysprosium ions, the doped glass providing a quantum efficiency of greater than 5« for emission at wavelengths of about 1300 nanometres. This invention also provides an optical waveguide amplifier comprising a glass optical waveguide doped with dysprosium ions, the glass not being a fluoride or silica glass. The invention recognises that the nature of the glasses previously proposed in dysprosium doped optical waveguide amplifiers can dramatically limit the performance of those amplifiers. By using glasses having either a low phonon energy or glasses having a high quantum efficiency (a quantity related to the phonon energy and/or type of glass), the efficiency of the Dy 3* dopant can be greatly improved. Embodiments of amplifiers according to the invention can operate in the second telecoms window between 1280 and 1350nm and can be easily pumped by a single semiconductor laser diode unit with a typical small signal gain in excess of 20dB for 50mW of pump power. Further claims involve the incorporation of another trivalent rare earth ion (example Ytterbium) as a sensitising agent, allowing the possibility of efficient 98θnm pumping. Although the invention is applicable to bulk optical or planar waveguides, it is preferred that the waveguide is an optical fibre. This can improve the spatial overlap between the dopant, the signal to be amplified and the pump signal. In particular, it is preferred that the optical fibre is a single mode optical fibre. The dopant may be applied only or primarily to the fibre core, or may also be applied to the fibre cladding. Preferably the waveguide is formed of a glass selected from the group consisting of: (i) heavy metal mixed halide glasses; (ii) chloride glasses (iii) chalcogenide glasses; and (iv) chalcohalide glasses. The.performance of the amplifier may be improved by the inclusion of at least one rare earth co-dopant to decrease the lifetime of the H 11/2 and/or H 13/2 energy levels of the dysprosium ion. This can improve the efficiency of the amplifier. Preferably the or a co-dopant is europium. Also, preferably the or a co-dopant is terbium. The lifetime of certain of the relevant energy levels in the dopant ions can be decreased (increasing the performance of the amplifier) by promoting lasing within the amplifier. To this end, it is preferred that the amplifier comprises reflector means for promoting lasing in the waveguide. Preferably, the reflector means comprises mirrors disposed at each end of the waveguide. Alternatively, it is preferred that the reflector means comprises gratings disposed at each end of the waveguide. Preferably the amplifier comprises means for pumping the amplifier at a pump wavelength selected from the group consisting of: about 810 nanometres, about 910 nanometres and about 1240 nanometres. Alternatively, it is preferred that the amplifier comprises a neodymium-yttrium-aluminium-garnet laser for pumping the amplifier at a pump wavelength of about 1064 nanometres or a neodymium-yttrium- lanthanum-fluoride laser for pumping the amplifier at a pump wavelength of about 1047 nanometres. In order to improve the amplifier performance further, it is preferred that the glass waveguide is doped with a sensitising agent to increase the absorption at the pump wavelength. In a preferred embodiment, the sensitising agent is ytterbium. In this case, it is particularly appropriate to employ means for pumping the amplifier at a pump wavelength of about 98O nm. An amplifier according to the invention is particularly suitable for use in a laser. Alternatively, an amplifier according to the invention is particularly suitable for use in telecommunications equipment. This invention also provides a method of manufacture of an optical waveguide amplifier, the method comprising the step of doping a glass optical waveguide with dysprosium ions, the glass having a maximum phonon energy of less than 450 cm "1 . This invention also provides a method of manufacture of an optical waveguide amplifier, the method comprising the step of doping a glass optical waveguide with dysprosium ions, such that the quantum efficiency of the 6 H 9/2 - 6 F 11/2 doublet of dysprosium ions in the waveguide is at least 5% . The invention will now be described by way of example with reference to the accompanying drawings, throughout which like parts are referred to by like references, and in which: Figure 1 is a schematic diagram illustrating the energy levels of the Dysprosium ion; Figure 2 is a graph showing the absorption spectrum for Dy 3* -doped Gallium-Lanthanum-Sulphide (Ga:La:S) glass; Figure 3 is a graph of a fluorescence spectrum corresponding to emission from the metastable H g/2 - F 11/2 doublet to the H 15/2 ground level in Dy 3* -doped Ga:La:S glass; Figures 4a to 4d are schematic diagrams of Dy * -doped low phonon energy glass amplifiers, using various pump configurations; Figure 5 is a graph of small signal gain against fibre length for a co-directional pumped Dy 3 "-doped Ga:La:S glass optical fibre amplifier; Figure 6 is a graph of small signal gain against pump power for a co-directional pumped Dy 3* -doped Ga:La:S glass optical fibre amplifier; Figure 7 is a schematic energy level diagram for Eu 3* , Tb 3* and Dy 3* ions; Figure 8 is a graph of gain against fibre length for a Tb 3* /Eu 3+ /Dy 3* co-doped Ga:La:S glass optical fibre amplifier; Figure 9 is a graph of gain against pump power for a Tb 3* /Eu 3* /Dy 3+ co-doped Ga:La:S glass optical fibre amplifier; Figure 10 is a graph of gain against pump power for a Eu 3 VTb 3* /Dy 3* co-doped Ga:La:S glass fibre amplifier, pumped at three different pump wavelengths; Figure 11 is a graph of gain against pump power for a Nd:YAG pumped Eu 3+ /Tb 3* /Dy 3* co-doped fibre amplifier; Figure 12 is a graph of gain against output power for a Nd:YAG pumped Eu 3* /Tb 3* /Dy 3* co-doped fibre amplifier; and Figure 13 is a graph of gain against Yb concentration for a Yb 3 7Eu 3 7Tb 3 7Dy 3* co-doped fibre amplifier. Figure 1 is a schematic diagram illustrating the energy levels of the Dysprosium (Dy 3+ ) ion. When the Dy 3* ion is added as a dopant to glass, the Dy 3* ion has a characteristic set of absorption lines. The wavelength and magnitude of the absorption lines are dependant on the host glass. If the Dy 3* -doped glass is to be used as an optical amplifying element, the wavelength and magnitude of the various absorption lines can significantly affect the efficiency and performance of the amplifying element. An example of an absorption spectrum for Dy 3* -doped Gallium- Lanthanum-Sulphide (Ga:La:S) glass is shown in Figure 2. As shown in Figure 2, there are a number of absorption "peaks", centred around the following approximate wavelengths: 800nm, 900nm, 1050 to llOOnm, and 1240 to 1290nm. The wavelengths of the absorption peaks form the possible amplifier pump wavelengths when the doped glass is used as an optical amplifying element. After a Dy 3* ion has absorbed a pump photon, the ion 'relaxes' via non-radiative (multi-phonon) decay within a short time to the metastable doublet 6H g/2 - F 11/2 , where it stays for a characteristic time which is strongly dependant on the host glass. An excited ion in the metastable doublet may decay non- radiatively to the underlying H 11/2 energy level at a rate (W NR ) determined predominantly by the maximum phonon energy of the host glass, and to a lesser extent by a host dependant electron-phonon coupling coefficient. These physical effects mean that for a given energy gap (example "1700cm "1 for the 6 H 9/2 - 6 F u/2 to 6 H 11/2 energy gap in Dy 3 -doped Ga:La:S), a "low phonon energy" glass has a lower non-radiative decay rate than a high phonon energy glass such as silica. Since this non-radiative decay process is in competition with that of spontaneous or stimulated emission from the metastable doublet, the non-radiative decay can dominate over spontaneous or stimulated emission in high phonon energy glasses. Thus little spontaneous emission is observed from the H g/2 - F 11/2 doublet in high phonon energy glasses. The spontaneous emission is characterised by a radiative decay rate (W rad ) which is also dependant on the glass host and ideally should be large. In other words, a low phonon energy glass, doped with Dy 3+ ions, provides a more efficient optical amplifying element than a higher phonon energy glass. One way of quantatively defining low phonon energy glasses is to quantify the radiative quantum efficiency of the H g/2 - F u/2 doublet as follows: QE ( % ) =100 rad W z, ad ■ w N, R This definition is related to the glass phonon energy, since a reduction in the glass phonon energy reduces the non-radiative decay rate, and hence increases the radiative quantum efficiency. A "low phonon energy glass" is defined as one in which the non- radiative decay rate is at such a low level that when the glass is doped with a low concentration of Dy 3* ions (for example O.Olmoi;. or lOOppm) the radiative quantum efficiency of the H g/2 - F 11/2 doublet is greater than 5»- (>10 " % could give even better results). This definition also covers glasses such as chalcohalides which still have a relatively high quantum efficiency because of their large radiative rates. Examples of low phonon energy glasses are: (i) heavy metal mixed halide glasses (such as CdF 2 -CdCl 2 , ZnCl 2 - ZnF 2 and mixed fluoride/chloride glasses containing Barium, Sodium, Indium, Lead and/or Gallium); (ii) chloride glasses (such as zinc and cadmium chlorides (ZnCl 2 , CdCl 2 )); (iϋ) chalcogenide glasses (such as germanium sulphide, arsenic sulphide and/or gallium sulphide based glasses including the addition of elements caesium, potassium, zirconium, antimony, lanthanum, phosphorus, gallium, indium, silver, calcium, sodium and bismuth and glasses containing Sulphur and/or Selenium and or Tellurium) , this category including Ga:La:S glass; and (iv) Chalcohalide glasses (such as any of the chalcogenide listed glasses with the addition of Chlorine and/or Fluorine). This definition of low phonon energy glass does not include so- called "pure" fluoride glasses (for example zinc fluoride - barium fluoride - lanthanum fluoride - Aluminium fluoride - sodium fluoride (ZBLAN) or indium fluoride (InF)) or oxide glasses (example Si0 2 ) , since the radiative quantum efficiency of the H g/2 - F 11/2 doublet when these glasses are doped with Dy 3+ ions is very low (less than 5%) • Direct measurement of the radiative quantum efficiency of the Dy 3+ -doped glass is carried out using the so-called "integrating sphere" method, described in the book "Physics and Chemistry of Glasses", M J Payne et al, 1991- An excitation wavelength around 124θnm is used for this measurement and (for the measurement process) the Dy 3* ion concentration is made low (~500ppm) in order to avoid ambiguous results due to energy transfer between Dy 3* ions. Examples of the quantum efficiencies for Dy 3* -doped glasses measured using this technique are: 2% for InF glass and 20# for Ga:La:S glass. Alternatively, a low phonon energy glass may be defined in terms of its maximum phonon energy, as measured by Raman spectroscopy. Here, the maximum phonon energy of the glass is defined as the energy of the highest frequency phonon mode of the glass, defined by the peak of the Raman intensity. Examples of phonon energies measured using this technique are: ~580cm "1 for ZBLAN glass, " 510cm "1 for InF glass and "350cm "1 for Ga:La:S glass. Using this definition of the maximum phonon energy of the glass, a low phonon energy glass is defined as one with a maximum phonon energy of less than 450cm "1 . (Better results still could be obtained by glasses in a range of less than e.g. 400 cm "1 ). Radiative emission from the doublet occurs to all the lower lying energy levels (i.e. H 11/2 , H 13/2 and H 15/2 ) and the emission spectrum is dependent on the host glass. An example of the fluorescence spectrum, corresponding to emission from the metastable H g/2 - F 11/2 doublet to the H 15/2 ground level, obtained from Dy 3* -doped Ga:La:S glass, is shown in Figure 3 and shows a peak wavelength of about 1320nm. Although the Dy 3 " ions can be used as a dopant in various types of waveguide such as planar or bulk optical waveguides, in the present embodiments the ions are incorporated into the core of a glass optical fibre. This can provide an efficient spatial overlap between the Dy 3* ions and both the pump and signal radiations. In particular, good results can be obtained with a single mode fibre having a core diameter of less than lOμm and a core/cladding refractive index difference of less than 0.1% . The optical fibre may be made by standard fabrication techniques such as the double crucible method, the rod-in-tube method, extrusion rotational casting or the so-called "solgel" method. Typical Dy 3* - doping levels for such optical fibre cores are within the approximate range 0.01mol%-5mol% (about 100ppm-50000ppm) . The process of amplification is similar to that taking place in the EDFA referred to above. As the pump radiation propagates along the fibre length, absorption occurs giving a population in the metastable doublet H g/2 - F 11/2 . Propagation of a weak signal beam (for example, a signal at 1320nm) through the fibre leads to the process of stimulated emission and net gain if the amplification is larger than any losses. The stimulated emission lineshape for Dy 3* in Ga:La:S is similar to the spontaneous emission shown in Figure 3 a d peaks at about 1320nm. Figures 4a to 4d are schematic diagrams of Dy 3* -doped low phonon energy glass fibre amplifiers, using various pump configurations. Each of the configurations uses an angled splice between a high NA low phonon energy glass fibre and a high NA silica fibre, which is tapered. The configurations shown in Figures 4a to 4d are referred to as "co-directional", "counter-directional", "double-pass" and "bi-directional" pumping respectively. In each of Figures 4a to 4d, signal light is input at an input port 10 and output at an output port 20. The pump signal is input at a pump input 30. Figures 4a to 4d also show a number of interconnected optical fibre units, referred to by the following reference numbers: Reference ] Number Hnϋ 40 pump signal multiplexer 50 tapered silica fibre 60 angled splice 70 Dy 3* doped low phonon energy glass fibre 80 mirror having high reflectance at pump and signal wavelengths 90 optical circulator 100 50:50 coupler The performance of a co-directional pumped Dy 3* -doped Ga:La:S glass optical fibre amplifier is shown in Figure 5 and 6. In particular. Figure 5 is a graph of small signal gain against fibre length and Figure 6 is a graph of small signal gain against pump power. In this embodiment, the amplifier operating wavelength is 1320nm, and is pumped at 124θnm by a semiconductor laser diode. The input signal power is lμw. The fibre contains 500ppm Dy 3* ions, and is characterised by a NA=0.4 and cutoff wavelength=900nm. Figure 5 demonstrates that an optimum device length is 10m, for which the peak gain is ~3dB at 50mW of pump power. Figure 6 shows a peak gain of ~5dB for lOOmW of pump power. The skilled man will appreciate that the term 'optimum' does not necessarily refer to an absolute maximum of performance, but instead refers to the result of an engineering process to improve the performance of the device as far as is reasonable given other possible design constraints. The device could also be pumped at any of the other absorption bands (HOOnm, 1050nm, 910nm, 88θnm, 8l0nm 7δθnm, or 76θnm) .although the device length and efficiency will not be the same as those shown in Figures 5 and 6. Although the basic Ga:La:S device described above offers significantly better performance than previous Dy 3* -doped amplifiers using high phonon energy glasses, its performance is limited by two main physical effects. The radiative quantum efficiency for the Dy 3* - doped Ga:La:S glass is ~20#, which indicates that about 80% of the ions in the metastable doublet decay non-radiatively to the lower lying energy level ( H 11/2 ) . When doped into Ga:La:S glass, the lifetime of the Dy 3* energy levels H 11/2 and H 13/2 are " 1msec and ~3.5msec respectively, as compared with ~55us for the H g/2 - F u/2 doublet. Thus, when the glass is used as an amplifying element, a significant number of ions will reside in both of these energy levels rather than returning to the ground level ( 6 H 15/2 ) . The result of this 'bottle- necking' is an increase in the optimum device length and hence the net background loss, thus tending to limit the amplifier efficiency. Furthermore, signal (1.3μm) excited state absorption from both of these levels to the higher lying levels F 3/2 , F- /2 , F ?/2 can limit further the amplifier efficiency and available peak gain. However, the efficiency of a basic Dy 3* -doped Ga:La:S fibre amplifier can be improved by co-doping the glass with other rare earth ions. In particular, co-doping of the Dy 3* -Ga:La:S fibre with the trivalent rare earth ion Terbium or trivalent Europium (or both) is observed to substantially reduce the lifetime of the H u/2 and H 13/2 energy levels. The energy level diagrams for Eu 3* and Tb 3* ions along with that for the Dy 3* ion are shown in Figure 7- I the co-doped schemes efficient (resonant) energy transfer occurs from the H 11/2 and H 13/2 energy levels of Dy 3* to one of the closely spaced energy levels of Tb 3* or Eu 3* . Fast non-radiative decay of the excited Tb 3* or Eu 3* ions now occurs to the respective ground states via these closely spaced energy levels. The lifetime of the H u/2 and H 13/2 energy levels in a Dy 3* - doped glass, co-doped with suitable concentrations of Tb 3* and/or Eu 3* , is now considerably shorter than that of the metastable doublet H g/2 - Examples of suitable co-doping levels are 0.01-5mol Eu 3* and 0.01-5mol2 Tb 3* ions (~100-50000ppm) . There are other means of decreasing the lifetime of these energy levels. These include the use of one or two high reflectors at the end(s) of the fibre to achieve lasing from either (or both) the H 11/2 and H 13/2 energy levels. The high reflector may be in the form of a external mirrors or gratings (either external or directly written into the fibre). The characteristics of a Tb 3* /Eu 3* /Dy 3* co-doped Ga:La:S glass optical fibre amplifier are shown in Figures 8 and 9> In particular, Figure 8 is a graph of gain against fibre length for a Tb 3* /Eu 3* /Dy 3* co- doped Ga:La:S glass optical fibre amplifier and Figure 9 is a graph of gain against pump power. As in the embodiment described with reference to Figures 5. 6 and 7, the device is co-directionally pumped, the fibre NA is 0.4, the fibre cut-off wavelength is 900nm, the pump wavelength is 124θnm, the signal wavelength is 1320nm and the signal power is lμw. The fibre core contains 500ppm Dy 3* , 5000ppm Eu 3* and 5000ppm Tb 3* . Figure 8 shows that the optimum device length for 50mW of pump power is reduced to ~1.3m (compared to a length of about "10m in the case of no co-doping - see Figure 5) • Figure 9 demonstrates that a substantial increase in the maximum gain (from 5 B to greater than 30dB) can be achieved by co-doping the fibre. In other words, co- doping the fibre can substantially increase the amplifier efficiency. The longevity of high power semiconductor laser diode units operating at 124θnm, based on InGaAs technology, has not been fully established. This is not the case for diodes operating in the wavelength range 750~9δOnm and based on the mature technology of AlGaAs. For this reason, it would be advantageous to be able to pump the optical amplifier at wavelengths in the range 750-98θnm. As already stated, it is in fact possible to pump the Dy 3* -doped low phonon energy glass fibre amplifier at wavelengths other than 124θnm. The most useful of the alternative wavelengths are the 910 and 8l0nm absorption bands. Figure 2 shows that the absorption cross section at these wavelengths is lower than the cross section at 124θnm and 1320nm. One consequence of this is a substantial increase in the pump saturation power of the amplifier and hence a lower efficiency for the device when operated at low pump powers. Figure 10 is a graph illustrating small signal gain of a Eu 3* /Tb 3* /Dy 3* co-doped Ga:La:S glass fibre amplifier, when pumped at any one of 810, 910 and 124θnm wavelengths using high power semiconductor laser diodes. The cut-off wavelengths are 900nm, 800nm and 700nm for 124θnm, 910nm and 8l0nm pumping respectively, whilst the optimum device length varies 1.3 m > 1.5m and 1.7m respectively. When operated at relatively low pump powers (<100mW), the 124θnm pump wavelength provides the most efficient amplification of the group. This can be attributed to the relatively small absorption cross sections at both 910nm and 8l0nm, increasing the pump saturation power of the amplifier. Application of the Dy 3* -doped low phonon energy glass fibre amplifier as a power amplifier is best achieved by high power pumping of the device. Direct pumping of the Dy 3* ions is possible at 1064nm, a wavelength corresponding to the output commercial Nd:YAG lasers or at 1047nm (by a neodymium-yttrium-lanthanum-fluoride laser) . These lasers have output powers in excess of 1W. Although the absorption cross section at 1064nm is very much less than that at 124θnm, and indeed lower than those at βlOnm and 910nm, the efficiency of the power amplifier can still be made high due to the large pump powers employed. The small signal gain of a Nd:YAG pumped Eu 3* /Tb 3* /Dy 3* co-doped fibre is shown in Figure 11. The fibre parameters are: NA=0.4, cut-off wavelength=990nm, length=2.5m, signal wavelength=1320nm and signal power=lμw. The fibre core is doped with 500ppm Dy 3* and 5000ppm of both Eu 3* and Tb 3* ions. Figure 12 is a graph of gain against output power for the Nd:YAG pumped Eu 3* /Tb 3* /Dy 3* co-doped fibre amplifier. Figure 12 demonstrates that gain in excess of 30dB is available at output powers in excess of 20dBm (lOOmW). The absorption spectrum for Yb 3* -doped Ga:La:S peaks at ~9δ0nm and shows considerable overlap with the Dy 3* ion absorption within this wavelength region. Incorporation of a suitable doping level of Yb 3* ions into a Dy 3* -doped fibre allows efficient energy transfer between the Yb 3* and Dy 3* ions. Energy transfer occurs from the 2 F 5/2 energy level in Yb 3* to the H 5/2 energy level of Dy 3* from which non-radiative decay occurs to the metastable doublet H g/2 - F u/2 , allowing amplification at 1320nm in a similar manner to that described above for the Dy 3* -doped device. Hence a Yb 3* /Dy 3* /Eu 3* /Tb 3* co-doped amplifier may be efficiently pumped at around 9δ0nm with a substantial increase in the efficiency when compared to a similarly pumped Dy 3* /Eu 3* /Tb 3* -doped device. The Eu 3* /Tb 3* /Dy 3* amplifier described with reference to Figures δ and 9 gives no net gain for lOOmW of pump power at a pump wavelength of 9δ0nm. In contrast, the results obtained for a series of Yb 3* /Eu 3* /Tb * /Dy 3* co-doped amplifiers, pumped with lOOmW, are shown in Figure 13. All these devices are 0.05mol# Dy 3* -doped with varying levels of Yb 3* -added to the fibre core. The fibre NA=0.4 and cut-off wavelength=δ50nm. Figure 13 shows that a Yb 3* /Dy 3* /Eu 3* /Tb 3* co-doped amplifier pumped at 9δOnm can achieve a device performance as good as the 124θnm pumped device, and better than either the δlO or 910nm pumped ones (see Figure 10). An explanation for this is that Yb 3* can act as a "sensitising agent" for a Dy 3* -doped amplifier or laser in order to increase the pump absorption at wavelengths outside the main Dy 3* absorption peaks. The amplifiers described above may be used as lasers at the wavelengths at which amplification is obtained. For example, an amplifier comprising Dy 3* -doped low phonon energy glass may be used as a laser at around 1320nm, using either external mirror(s) or gratings (either external or directly written into the fibre), and either with or without Eu 3* /Tb 3* co-doping. The lasers could make use of a sensitising agent such as Yb 3* as a co-dopant in a Dy 3* -doped low phonon energy glass for operation at around 1320nm, either with or without Eu 3* /Tb 3* -co-doping. In another example, a Dy 3* -doped low phonon energy glass fibre may be operated as a laser at around either 1.7μm or 2.δμm (employing the H u/2 - H 15/2 and H 13/2 - H 15/2 transitions respectively) using mirrors or gratings. A sensitising agent may be used to increase the pump absorption of a Dy 3* -doped fibre laser operating around 1.7μm and/or 2.δμm. Amplifiers and lasers as described above can be used in a variety of applications such as in telecommunication equipment. For example, an optical amplifier as described above could be used in a repeater device forming part of an optical fibre signal transmission link.

Claims: CLAIMS 1. An optical waveguide amplifier comprising a glass optical waveguide doped with dysprosium ions, the glass having a maximum phonon energy of less than 450 cm "1 . 2. An optical waveguide amplifier comprising a glass optical waveguide doped with dysprosium ions, such that the quantum efficiency of the H g/2 - F u/2 doublet of dysprosium ions in the waveguide is at least 5% . 3. An optical waveguide amplifier comprising a glass optical waveguide doped with dysprosium ions, the doped glass providing a quantum efficiency of greater than 5% for emission at wavelengths of about 1300 nanometres. 4. An optical waveguide amplifier comprising a glass optical waveguide doped with dysprosium ions, the glass not being a fluoride or silica glass. 5. An amplifier according to any one of the preceding claims, in which the waveguide is an optical fibre. 6. An amplifier according to claim 5. in which the optical fibre is a single mode optical fibre. 7. An amplifier according to any one of the preceding claims, in which the waveguide is formed of a glass selected from the group consisting of: (i) heavy metal mixed halide glasses; (ii) chloride glasses (iii) chalcogenide glasses; and (iv) chalcohalide glasses. δ. An amplifier according to any one of the preceding claims, in which the glass waveguide is doped with at least one rare earth co- dopant to decrease the lifetime of the 6 H u/2 and/or 6 H 13/2 energy levels of the dysprosium ion . 9. An amplifier according to claim δ , in which the or a co-dopant is europium . 10. An amplifier according to claim δ or claim 9. in which the or a co-dopant is terbium. 11. An amplifier according to any one of the preceding claims, comprising reflector means for promoting lasing in the waveguide. 12. An amplifier according to claim 13, in which the reflector means comprises mirrors disposed at each end of the waveguide. 13- An amplifier according to claim 11, in which the reflector means comprises gratings disposed at each end of the waveguide. 14. An amplifier according to any one of the preceding claims, comprising means for pumping the amplifier at a pump wavelength selected from the group consisting of: about δlO nanometres, about 910 nanometres and about 1240 nanometres. 15. An amplifier according to any one of claims 1 to 13. comprising a neodymium-yttrium-aluminium-garnet laser for pumping the amplifier at a pump wavelength of about 1064 nanometres or a neodymium-yttrium- lanthanum-fluoride laser for pumping the amplifier at a pump wavelength of about 1047 nanometres. 16. An amplifier according to any one of claims 1 to 13. in which the glass waveguide is doped with a sensitising agent to increase the absorption at the pump wavelength. 17. An amplifier according to claim 16, in which the sensitising agent is ytterbium. lδ. An amplifier according to claim 17, comprising means for pumping the amplifier at a pump wavelength of about 9δ0 nanometres. 19. A laser comprising an amplifier according to any one of the preceding claims. 20. Telecommunications equipment comprising an optical waveguide amplifier according to any one of claims 1 to lδ. 21. A method of manufacture of an optical waveguide amplifier, the method comprising the step of doping a glass optical waveguide with dysprosium ions, the glass having a maximum phonon energy of less than 450 cm "1 . 22. A method of manufacture of an optical waveguide amplifier, the method comprising the step of doping a glass optical waveguide with dysprosium ions, such that the quantum efficiency of the H g/2 - F u/2 doublet of dysprosium ions in the waveguide is at least 5% .

Inventors: HEWAK DANIEL WILLIAM, LAMING RICHARD IAN, PAYNE DAVID NEIL, SAMSON BRYCE NEILSON, HEWAK, DANIEL, WILLIAM, LAMING, RICHARD, IAN, PAYNE, DAVID, NEIL, SAMSON, BRYCE, NEILSON
Applicants: HEWAK DANIEL WILLIAM, LAMING RICHARD IAN, PAYNE DAVID NEIL, SAMSON BRYCE NEILSON, UNIV SOUTHAMPTON, HEWAK, DANIEL, WILLIAM, LAMING, RICHARD, IAN, PAYNE, DAVID, NEIL, SAMSON, BRYCE, NEILSON, UNIVERSITY OF SOUTHAMPTON
Application year: 1995
Main classification: H01S3
IPC codes: H01S3