Method of and device for measuring the nonlinear refractive index in a single mode optical fibre

Abstract: A train of transform-limited optical pulses with wavelength close to the zero-dispersion wavelength of the fibre (2) and high and variable peak power, such as to give rise to self-phase modulation, is sent into a fibre (2); the spectral broadening of the signal exiting the fibre (2) is measured for a number of values of the peak power of the pulses and the nonlinear refractive index is obtained from the angular coefficient of the straight line representing spectral broadening versus peak power. The device for carrying out the method is also provided.

Description: The invention described herein relates to the characterisation of optical fibres and in particular its object is to provide a method and a device for measuring the Kerr non-linearity coefficient (or nonlinear refractive index coefficient) in a single mode optical fibre. In most materials of interest for optical communications, one of the main nonlinear phenomena is the Kerr optical effect, which acts on the refractive index making it depend on optical intensity I according to the formula: n(I) = n 0 + n 2 I where n(I) is the refractive index as a function of the intensity (and therefore of the power) of the radiation sent into the fibre, n 0 is the linear refractive index, whilst n 2 is the so-called nonlinear coefficient of the refractive index (also called simply nonlinear refractive index). Due to the introduction of optical amplifiers in optical communication systems, the powers transmitted along a fibre make nonlinear effects linked to n 2 no longer negligible: since these effects can cause significant degradation in the performance of a system or, conversely, they can be exploited for new technical solutions, it is important to know them with precision. In the case of optical fibres, the nonlinear refractive index n 2 in general is obtained indirectly, through a measurement of the so-called Kerr non-linearity coefficient γ, which is proportional to n 2 and also takes into account the confinement of light in the fibre, thus providing more complete information, from the operational point of view, than does n 2 , which is a parameter depending only on the material. Coefficient γ is given by relation: γ = (2π/λ p )·(n 2 /A eff ) = (ω p /c)·(n 2 /A eff ) where λ p and ω p are respectively the wavelength and the angularfrequency ofthe radiation sent into the fibre, c is the velocity of light and A eff is the effective area of the core of the fibre. which is a parameter providing a measure of the optical confinement of light inside the fibre. From the value of γ it is therefore possible to obtain the value of n 2 , once A eff , which needs to be obtained with an independent measurement, is known. Several methods of determining γ or n 2 are known. The most commonly used ones entail sending high power optical pulses into the fibre and analysing the spectrum of the pulses exiting the fibre in order to measure the nonlinear phase shift  NL induced by each pulse on itself (self-phase modulation). This phase shift is due to the fact that the pulse changes the refractive index of the fibre, as indicated by relationship (1), and it is linked to coefficient γ by relation  NL = γ·P·L, where P is the pulse power and L the length of the fibre. The pulses used are in general very short, to obtain the high peak powers required, since n 2 in silica is very small (order of magnitude: 10 -20 m 2 /W). Examples of such methods are described in the papers: "Measurement of nonlinear index of silica-core and dispersion-shifted fibers", by K.S. Kim et al., Optics Letters, Vol. 19, no. 4,15 February 1994, pp. 257 et seq., "Nonlinear coefficient measurement for dispersion shifted fibres using self-phase modulation method at 1.55 µm", by Y. Namihira et al., Electronics Letters, Vot. 30, No. 14, 7 July 1994, pp. 1171-1172, and in the paper "Nonlinear-index measurement by SPM at 1.55 µm", by R.H. Stolen et al., presented at OFC'95, San Diego (USA), 26 February - 2 March 1995, paper FD1. From these papers, it is known that the spectrum of the pulse at the output of the fibre is broadened and presents a succession of maxima and minima. According to the paper by Kim et al., the nonlinear index is obtained from the phase shift the transmitted light is subjected to, which phase shift is measured by obtaining identifiable shapes at particular phase shifts using a Fabry-Perot interferometer. As stated in the paper, such method is affected by various uncertainties. According to the paper by Namihira et al., the number of the maxima and minima of the output spectrum is detected, which number depends on the instantaneous power of the pulse, and the positions of the maxima and minima correspond to values of  NL that are odd multiples of π/2. By measuring power P in these points, one obtains  NL and therefore y. Also a measurement of this kind has limited accuracy, since it is difficult to exactly determine the points of maximum and minimum, and therefore, given the small size of the peaks, the power value measured can be affected by even quite large errors. The invention provides instead a method and a device which do not require the evaluation of the phases and of power maxima and minima and hence allow an accurate measurement of n 2 or γ. More specifically, the invention is based on a measurement of the spectral broadening undergone by a high power pulse because of the Kerr effect. It has been demonstrated (see Q.Z. Wang et al.: "Supercontinuum Generation in Condensed Matter", in "The Supercontinuum Laser", edited by R.R. Alfano, Springer-Verlag 1989, Ch. 2, par. 2, pp. 34-40) that, when operating under conditions in which the group velocity dispersion in the fibre, the absorption and the Raman effect can be ignored, the pulse has such characteristics as to give rise only to self-phase modulation. In this case the electric field in each time position τ along the pulse has an instantaneous frequency ω(τ) = ω p + δω(τ) with δω(τ) = -(γ/2)[∂F 2 (τ)/∂τ]·z·P where F(τ) is the envelope of the pulse launched into the fibre, z is the distance from the fibre launching end and P is the peak power of the pulse. At the output from the fibre, the spectrum of the pulse will have undergone an overall broadening given by the maximum of function (4) which, as can easily be deduced by deriving function (4) and setting the derivative to 0, is given by Δω M = (γ/2)[∂ 1 - ∂ 2 ]·z·P where ∂ 1 , ∂ 2 indicate the values of ∂F 2 (τ)/∂τ in the two inflection points of intensity F 2 (τ). The broadening therefore is a linear function of pulse power through a constant which depends on the characteristics of the pulse, on parameter γ and on the length of the fibre. From the measurement of the spectral broadening, it is easy to obtain γ and n 2 . Note that the relations given above are valid for power values at least as high as to give rise to a doubling of the peak in the spectrum of the pulse. Therefore, according to the invention a method is provided in which a signal comprising a train of transform-limited optical pulses is sent into the fibre, the pulses having a wavelength close to the zero-dispersion wavelength of the fibre and a high and variable power, so as to give rise to self-phase modulation, and the spectrum of the pulses exiting the fibre is analysed. The spectral broadening of the signal exiting the fibre is measured for a number of values of the peak power of the pulses, such spectral broadening being a linear function of peak power according to a factor which depends on the nonlinear refractive index; the angular coefficient of the line representing said function is determined and the nonlinear refractive index is obtained from such angular coefficient. Note that the pulses must have a short duration (e.g. 5 - 8 ps) but they must not be too short, as in that case they would occupy a very wide spectrum which could involve spectral regions of the fibre with high group velocity dispersion, thus voiding one of the conditions for the validity of relations (3) - (5). As stated above, the self-phase modulation gives rise to a number of peaks in the spectrum of the pulse at the output of the fibre and the number of those peaks depends on the instant power of the pulse. The measurement of the spectral broadening is carried out either measuring the full width at half maximum (FWHM) of the spectrum or the distance between extreme peaks. According to the invention, the first quantity is preferably measured, since such a measurement has been proved to result in a better agreement between experimental data and the theoretical behaviour of the spectral broadening versus the peak power, expressed by relation (5). The invention concerns also the device carrying out the method, which comprises: means to generate and send into the fibre a sequence of transform-limited optical pulses, with a high power such as to give rise to self-phase modulation and with wavelength close to the zero-dispersion wavelength of the fibre; means to vary the power of the pulses sent into the fibre and to measure such power; means to analyse the optical spectrum of the pulses exiting the fibre; and a processing system to obtain the nonlinear refractive index from the optical spectrum; the means to analyse the optical spectrum of the pulses exiting the fibre are arranged to determine the spectral broadening of the pulses as the peak power varies; and the processing system is arranged to obtain the nonlinear refractive index from the angular coefficient of the straight line representing the spectral broadening versus the peak power. For the sake of further clarification, reference is made to the enclosed drawing, wherein: Figure 1 is a schematic representation of the device which carries out the method; Figures 2A - 2D are graphs of the spectrum, at the output of the fibre, of a hyperbolic secant pulse for different values of the peak power; Figure 3 is a graph of the spectral broadening versus the peak power for the values of power considered in Figure 2; and Figure 4 is a graph showing the theoretical and experimental curves of the spectral broadening versus the peak power. In the drawing thin lines indicate the path of the optical signals and double lines indicate electrical connections. A source 1, e.g. a wavelength tunable colour centre laser, generates a train of pulses with duration Δt and repetition period T, wavelength λ p close to the zero dispersion wavelength λ 0 of a fibre 2 whose Kerr non-linearity coefficient is to be measured and such peak power as to give rise to self-phase modulation. The pulses are transform-limited or quasi transform limited pulses, that is pulses for which the product between the full width at half maximum Δt and the bandwidth Δν must have a certain value, corresponding to the theoretical minimum, which depends on the pulse shape. Pulses with those characteristics are for instance hyperbolic secant pulses (Δt·Δν = 0.314), Gaussian pulses (Δt·Δν = 0.441) or Lorentzian pulses (Δt·Δν = 0.11). The pulse train is launched into the fibre by means of a variable attenuator 3 that allows different values to be selected for average power. A beam splitter 4 placed between the attenuator and the fibre allows a fraction of the power associated with each pulse to be taken and sent to a radiometer 5 or to another power measuring device. The signal exiting fibre 2 is collected by an optical spectrum analyser 6 or other instrument that is arranged to measure the spectral broadening of the pulses as peak power P varies. Advantageously, for the reasons given above, device 6 measures the maximum broadening Δλ M (to which a value Δω M corresponds) as the full width at half maximum of the output spectrum, which width, in a theoretical spectrum, substantially corresponds with the distance between the two extreme inflection points. A processing system 7, connected to analyser 6 and radiometer 5, obtains the values of P (given by the product of the average power by the inverse T/Δt of the duty cycle) from the individual values of the average power, stores the values of Δω M in correspondence with the different values of P, determines the angular coefficient of the straight line representing Δω M versus P and obtains the value of γ, and therefore of n 2 , from such angular coefficient; such a value, taking into account (5) and (2) is given by where ∂ 1 and ∂ 2 are computed analytically for each type of pulse (∂ 1 = -∂ 2 for symmetrical pulses like the ones mentioned above). The values of peak power P must be high enough to give rise to self-phase modulation but not so high as to cause Raman effect in the fibre. The minimum value can be on the order of 1 W, a value for which a doubling of the peak in the spectrum of the pulse starts to occur. Taking into account that the peak power threshold for which the Raman effect occurs is of the order of one hundred Watts, a maximum value for P can be a few tens of Watts, for instance about 20 W. In an exemplary embodiment of the invention, the fibre was a dispersion-shifted fibre with a length of 0.5 km and a zero-dispersion wavelength λ 0 = 1558 nm, the source had a wavelength λ = 1549.5 nm (and therefore an angular frequency ω p = 12.15·10 14 s -1 ) and an effective area A eff = 43·10 -12 m 2 ; the pulses were hyperbolic secant pulses with bandwidth Δν = 55 GHz and full width at half maximum Δt = 5.7 ps (and therefore product Δt·Δν = 0.314), and repetition frequency 76 MHz. For these pulses, it is easy to see that (4) and (6) become respectively Δω M = 8 ch -1 ( 2 ) 3 3 · γ· z Δ t · P n 2 = 3 3 8 ch -1 ( 2 ) · Δ t · A eff · c ω p · z All parameters appearing in relation (8) are constant quantities for a given system configuration: processing system 7 can therefore immediately obtain value n 2 . Figures 2A - 2D represent the output spectra corresponding to four values of peak power (respectively 3.85 W, 5.98 W, 11.19 W and 15.4 W). In those Figures each interval corresponds to 2 nm (x-axis) and 25 µW (y-axis). The Figures clearly show the peaks due to self-phase modulation. Figure 3 shows spectral broadening Δω M (obtained from the full width at half maximum Δλ M ) versus the peak power for a number of values of peak power, including the values corresponding to Figures 2A-2D. The linear behaviour of Δω M is clearly apparent. In order to take into account the fact that the two extreme peaks of the output spectrum have different heights so that the two half-maximum points have different ordinates h s , h d (contrary to what happens in the theoretical spectrum), the distance between the extreme points with ordinate (h s +h d )/2 has been considered as the full width at half maximum. The experimental values, fitted into a straight line, yielded a value of 2.6·10 -20 m 2 /W for n 2 . Such a value is in good agreement with both the theoretical values given by relation (5) (see Fig. 4, where the solid line corresponds with the experimental data and the dotted line with the theoretical behaviour) and the values measured with other methods. Note also that, in the measurement conditions described herein (fibre 0.5 Km long), polarisation remains substantially constant for the whole time taken by the measurement and hence it does not affect the results obtained. Should the effect of the random statistical evolution of polarisation be no longer negligible (as it might happen when using fibre spans of a few tens of kilometres), correcting factor 8/9 should be applied to the value determined by the measurement, as it is well known to the technician -(see S. Γ. Evangelides et al. "Polarization Multiplexing with Solitons", Journal of Lightwave Technology, Vol. 10, No. 1, January 1992, pages 28 and fol.). It is evident that what has been described is given solely by way of non-limiting example and that variations and modifications are possible without departing from the scope of the invention, which is only limited by the wording of the appended claims.

Claims: Method of measuring the nonlinear refractive index in a single-mode optical fibre (2), wherein a signal comprising a train of "transform limited" or "quasi transform limited" optical pulses is sent into fibre (2), such pulses having a wavelength close to the zero-dispersion wavelength of the fibre (2) and a high and variable power, such as to give rise to self-phase modulation, and the spectrum of the pulses exiting the fibre (2) is analysed, wherein the spectral broadening of the signal exiting the fibre (2) is measured for a number of values of the peak power of the pulses by measuring the full width at the half maximum of the spectrum or the distance between extreme peaks, such spectral broadening being a linear function of the peak power according to a factor depending on the nonlinear refractive index; the angular coefficient of the straight line representing said function is determined, and the nonlinear refractive index is obtained from this angular coefficient. Device for measuring the nonlinear refractive index in a single mode fibre (2), comprising: means (1) to generate and send into the fibre (2) a train of transform-limited optical pulses, with such a power as to induce self-phase modulation in the fibre and with wavelength close to the zero-dispersion wavelength of the fibre (2); means (3, 5) to vary the power of the pulses sent into the fibre and to measure such power; means (6) to analyse the optical spectrum of the pulses exiting the fibre; and a processing system (7) to obtain the nonlinear refractive index from the optical spectrum; wherein the means (6) to analyse the optical spectrum of the pulses exiting the fibre are arranged to determine the spectral broadening of the pulses as the peak power varies; and the processing system (7) is arranged to obtain the nonlinear refractive index from the angular coefficient of the straight line representing spectral broadening versus peak power.

Inventors: CALVANI RICCARDO, CAPONI RENATO, NADDEO CLAUDIO, ROCCATO DIEGO, CALVANI, RICCARDO, CAPONI, RENATO, NADDEO, CLAUDIO, ROCCATO, DIEGO
Applicants: AGILENT TECHNOLOGIES INC, AGILENT TECHNOLOGIES, INC. (A DELAWARE CORPORATION)
Application year: 1996
Main classification: G01M11
IPC codes: G01M11