OSA's Digital Library

Optics Express

Optics Express

  • Editor: Michael Duncan
  • Vol. 13, Iss. 4 — Feb. 21, 2005
  • pp: 1138–1143
« Show journal navigation

Ultrafast optical delay line using soliton propagation between a time-prism pair

James van Howe and Chris Xu  »View Author Affiliations


Optics Express, Vol. 13, Issue 4, pp. 1138-1143 (2005)
http://dx.doi.org/10.1364/OPEX.13.001138


View Full Text Article

Acrobat PDF (194 KB)





Browse Journals / Lookup Meetings

Browse by Journal and Year


   


Lookup Conference Papers

Close Browse Journals / Lookup Meetings

Article Tools

Share
Citations

Abstract

Through theoretical analysis and experiment, we show that the performance of an ultrafast optical delay line using a time-prism pair is significantly improved when solition propagation is used between time-prisms. The enhancement is most dramatic for short pulses where dispersive pulse broadening in a linear propagation regime between time-prisms is large and limits perfomance. Experimentally, we demonstrate an optical delay line using soliton propagation in an all-fiber configuration allowing us to achieve a scan rate of 0.5 GHz, a delay range of 33.0 ps, no pre- and post-dispersion compensation, and a delay-to-pulse-width ratio of 6.0.

© 2005 Optical Society of America

1. Introduction

2. Theoretical analysis

The figure of merit for any delay line is the delay-to-pulse-width ratio which we define as Rτ/TFWHM, where TFWHM is the intensity full width at half maximum for the input pulse and Δτ is the maximum time delay at the output of the device, given by [5

5. J. van Howe and Chris Xu, “Ultrafast optical delay line by use of a time-prism pair,” Opt. Lett. 30, 99–101 (2005). [CrossRef] [PubMed]

] as

Δτ=Δλ·D=(π2λ22πcVppVπ1Tm)·D.
(1)

σ=1+(λ22πcD2To2)2,
(2)

where To is the intensity 1/e half-width of the Gaussian input pulse.

Fig. 1. Optical path of previous ultrafast delay line using linear propagation and pre- and post-dispersion compensation (pre- and post-comp). Evolution of the optical pulse and carrier frequency is shown above. The black curves represent the linear portion of the sinusoidal phase profile imposed by the time-prisms; PM: phase modulator.

In order to have complete reversible frequency conversion, the broadened pulse plus the full delay is restricted to the linear portion (TLin) of the sinusoidal modulation drive,

Toσ+Δτ<TLin.
(3)

The linear portion of the modulation drive depends on the fractional nonlinearity that can be tolerated in an experiment. Here we define the fractional nonlinearity, NL, as the ratio of the cubic term to the linear term in the Taylor expansion of the sinusoidal modulation. The fractional nonlinearity determines the amount of spectral and temporal distortion of output pulses and the linear portion for a given NL can be solved as TLin=βTm, where β=2π(1.5)NL.

Fig 2. Delay-to-pulse-width ratio, R as a function of input pulse width for two contours of fractional nonlinearity, NL=5% (blue curves) and NL=30% (red curves). The linear propagation regime is shown by the dashed curve, and the soliton propagation regime is shown by the solid curves. The peak-to-peak drive voltage and modulation frequency are fixed to 5.24 Vπ and 10 GHz respectively.

We use Eqs. (13) to solve for the delay-to-pulse-width ratio, R, as a function of input pulse width for linear and soliton propagation (Fig. 2). Each contour in Fig. 2 gives the upper bound for R for the corresponding NL. In the linear propagation regime (dashed curves), dispersive pulse broadening dominates for short pulses where the optical pulse bandwidth (Δλopt) is much greater than the wavelength shift produced by the phase modulator, i.e. Δλopt≫Δλ. The asymptotic behavior for short pulses at a given NL approaches

R=π2VppVπβln2[1+2π2VppVπToTm]1.
(4)

For long input pulse widths, Δλ opt≪Δλ, pulse broadening is negligible (σ→1) and the asymptotic behavior for long pulses approaches

R=12ln2(βTmTo1),
(5)

reaching zero for To=βTm, the maximum input pulse width allowed for a given NL. For soliton propagation between time-prisms (solid curves), however, dispersive pulse broadening is completely balanced by self-phase modulation, i.e., σ=1in Eq. (3). Thus, the expression for R at any pulse width is given by Eq. (5). Although linear and solitonic propagation are the same in the long pulse limit, soliton propagation is far superior for short pulses (Fig. 2), eliminating the finite limit on R at short pulse widths. The enhanced ratio using soliton propagation between time-prisms can be understood intuitively in terms the spatial analogy, Fig. 3(a). It is well known that the analog to narrow-band dispersion in the time domain is paraxial diffraction in space [6

6. B. Kolner, “Space-time duality and the theory of temporal imaging,” IEEE J. Quantum. Electron. 30, 1951–1963 (1994). [CrossRef]

]. Here we further extend this spatial-temporal analogy to include optical nonlinearity, where soliton propagation is just the temporal analog of spatial self-trapping. In the absence of self-trapping between a spatial prism pair (linear propagation), the spatially translated beam is also expanded by diffraction, requiring a balance between the input beam diameter and prism separation in order to have successful k̄ vector conversion. Compensating diffraction with self-focusing eliminates such a constraint and therefore improves performance.

Fig. 3. (a) A schematic of a spatial prism-pair demonstrating the space-time analogy [6,7]. (b) Experimental setup. The phase modulators (PM1) and (PM2) are each driven with a 10 GHz sinusoid whose amplitude is modulated by a 0.5 GHz sinusoid through an RF modulator. The operation of the time-prisms and the evolution of the carrier frequency are indicated. Both Δτ and the pulse width are small portions of the phase modulation period so that the phase modulation can be approximated by a linear phase ramp.

3. Experimental setup and results

The experimental setup is shown in Fig. 3(b). The pulsed source (Calmar Optcom; PSL-10) emits a 5.5 ps FWHM (3dB bandwidth ~0.48 nm), chirp-free, 10 GHz pulse train at a center wavelength of 1549.3 nm. The pulse train is divided down to a 5 GHz repetition rate using a Mach-Zehnder LiNbO3 modulator as a pulse picker. The carrier wavelength of the pulse train is then up-shifted by a time-prism, a 10 GHz sinusoidally driven LiNbO3 phase modulator (PM1). An erbium doped fiber amplifier (EDFA) and a variable attenuator are used to adjust the optical power to satisfy the soliton condition for propagation in the following 2.88 km of SMF-28 fiber (total dispersion 49 ps/nm). After propagating as a soliton pulse train through the dispersive delay, the carrier wavelength is down-shifted back to its original value by a second time-prism (PM2), driven with the same sine wave, but π out of phase. The amount of wavelength shift, and therefore the amount of time delay, is controlled by adjusting the drive voltage into the phase modulators through a broadband RF modulator (Miteq; BMA0218LA1MD). Since V p-pV RF_mod, where V RF_mod is the modulation input into the RF modulator, Δτ becomes a function of VRF _mod, Eq. (1). Thus, ultrafast programmable time delays can be obtained by controlling the modulation waveform V RF_mod.

To demonstrate the concept, we first verified soliton propagation by showing that for the proper input power, the spectrum and the pulse remain unchanged after propagating through the 2.88 km of fiber. For a 5.5 ps Sech pulse at 5 GHz repetition rate, we expected the fundamental soliton to be obtained between 18 to 19 dBm average input power into the SMF- 28. Figure 4 shows the various spectra and time traces for different propagation regimes. The blue dashed curves in Figs. 4(a) and 4(b) denote the original spectrum and time trace of the source before propagation. The spectral characteristics and pulse width at various input powers into the SMF fiber is typical for nonlinear propagation in the anomalous dispersion region and is in agreement with our numerical simulations. The 18.3-ps pulse width of the source as measured by the sampling scope is consistent with the impulse response of the oscilloscope (~17.0 ps) and a 5.5-ps input pulse. The spectral features in Fig. 4(a) are indicative of a small deviation from the ideal Sech input pulse. Figure 4(b) shows the contrast between soliton propagation and linear propagation (-10.0 dBm into the fiber).

Fig. 4. (a) Spectra corresponding to different amounts of average power into the 2.88 km of SMF-28. The average power and corresponding temporal pulse widths are written on the respective curves. The dashed blue curve corresponds to the original spectrum. All spectra are taken at 0.05 nm resolution bandwidth (RBW). (b) Oscilloscope time traces for different propagation regimes. The dashed blue curve corresponds to the time trace of the input pulse.
Fig. 5. Evolution of optical spectra through the ultrafast delay-line using soliton propagation: original spectra (dashed blue curves); after PM1 (solid black curves); after PM2 (solid red curves). All spectra were taken at 0.05 nm RBW.

To demonstrate ultrafast scanning capability of our delay line and the improved performance using soliton propagation, we modulate the 10 GHz RF sine wave with a 0.5 GHz sinusoid. The maximum RF output into the wavelength up-shifting phase modulator was approximately 5.24Vπ, corresponding to a maximum wavelength shift of 0.66 nm. Figure 5 shows the evolution of the optical spectrum through the ultrafast delay-line: 1) before phase-modulation; 2) after wavelength up-shifting (after PM1); and 3) after wavelength down-shifting (after PM2).

By using soliton propagation between time-prisms, dispersive broadening no longer occurs, gaining an additional 10 ps in time delay. The improved performance is demonstrated by the excellent match between the original soliton spectrum (blue dashed curve) and the spectrum after wavelength down-shifting (solid red curve) in Fig. 5. The broadened spectrum after wavelength up-shifting (solid black curve) represents the superposition of the spectra of five pulse trains, whose center wavelengths are successively up-shifted. We also note that much of the oscillatory structure in the down-shifted spectrum has vanished. This agrees with simulation results and is due to the fact that a good portion of the dispersive non-solitonic waves have been shifted out of band by the time-prisms.

Fig. 6. (a) Oscilloscope time trace demonstrating rapid scanning of delays. The dashed grid lines represent the original position of pulses with no phase modulation. (b) Delay Δτ as a function time obtained from (a). The solid curve is the 0.5 GHz modulation. The impulse response of the scope is ~17.0 ps.

Scanning of the optical delay in the soliton propagation regime is shown by the oscilloscope time trace in Fig. 6(a). The corresponding delays are plotted in 6(b), with the 0.5 GHz modulation (V RF_mod) plotted on top of the measured data points. The excellent agreement in Fig. 6(b) demonstrates the precise mapping of the modulation input to the time delay. Here the measured maximum time delay is 33.0 ps, giving a delay-to-pulse-width ratio of 6.0. This matches well to what is expected given the 0.66 nm wavelength shift and 49 ps/nm dispersion. While additional measurements on the spectral phase will uniquely match the pulse shape before and after the delay, the nearly identical pulse spectra and time traces are very good indications that the output pulse train is simply a delayed replica of the input.

4. Conclusion

Through theoretical analysis and experiment, we show that the performance of an ultrafast optical delay line using a time-prism pair is significantly improved when solition propagation is used between time-prisms. The enhancement becomes most dramatic in the case of short pulses where the optical bandwidth greatly exceeds the frequency shift of the time-prisms. For the purposes of demonstration, we show ultrafast scanning for an input pulse width of 5.5 ps and obtain a delay-to-pulse-width ratio of 6.0. Although standard SMF was used to achieve the dispersive delay in our experiment, other fiber types, such as those with much smaller mode field diameters can be used to reduce the power requirement for solitons, making our technique applicable for a sub-picosecond pulse train.

References and links

1.

W. Yang, D. Keusters, D. Goswami, and W.S. Warren, “Rapid ultrafine-tunable optical delay line at the 1.55-µm wavelength,” Opt. Lett. 23, 1843–1845 (1998). [CrossRef]

2.

R. Piyaket, S. Hunter, J.E. Ford, and S. Esener, “Programmable ultrashort optical pulse delay using an acousto-optic deflector,” Appl. Opt. 34, 1445–1453 (1995). [CrossRef] [PubMed]

3.

I. Frigyes and A. J. Seeds, “Optically generated true-time delay in phased-array antennas,” IEEE Trans. Microwave Theory Technol. 43, 2378–2386 (1995). [CrossRef]

4.

X. Liu, M. J. Cobb, and X. Li, “Rapid scanning all-reflective optical delay line for real-time optical coherence tomography,” Opt. Lett. 29, 80–82 (2004). [CrossRef] [PubMed]

5.

J. van Howe and Chris Xu, “Ultrafast optical delay line by use of a time-prism pair,” Opt. Lett. 30, 99–101 (2005). [CrossRef] [PubMed]

6.

B. Kolner, “Space-time duality and the theory of temporal imaging,” IEEE J. Quantum. Electron. 30, 1951–1963 (1994). [CrossRef]

OCIS Codes
(060.5530) Fiber optics and optical communications : Pulse propagation and temporal solitons
(070.2580) Fourier optics and signal processing : Paraxial wave optics
(320.7080) Ultrafast optics : Ultrafast devices

ToC Category:
Research Papers

History
Original Manuscript: January 10, 2005
Revised Manuscript: January 10, 2005
Published: February 21, 2005

Citation
James van Howe and Chris Xu, "Ultrafast optical delay line using soliton propagation between a time-prism pair," Opt. Express 13, 1138-1143 (2005)
http://www.opticsinfobase.org/oe/abstract.cfm?URI=oe-13-4-1138


Sort:  Journal  |  Reset  

References

Cited By

Alert me when this paper is cited

OSA is able to provide readers links to articles that cite this paper by participating in CrossRef's Cited-By Linking service. CrossRef includes content from more than 3000 publishers and societies. In addition to listing OSA journal articles that cite this paper, citing articles from other participating publishers will also be listed.


« Previous Article  |  Next Article »

OSA is a member of CrossRef.

CrossCheck Deposited