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Parabolic Pulses

Definition: pulses with a parabolic intensity profile

More general term: light pulses

German: parabolische Pulse

Categories: nonlinear opticsnonlinear optics, light pulseslight pulses


Cite the article using its DOI: https://doi.org/10.61835/0uc

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A parabolic pulse is a light pulse (usually an ultrashort pulse) that has a temporal intensity profile with a parabolic shape – not only near the pulse center, but also well towards the wings up to the point where the intensity goes to zero. In the ideal case, the pulse would have an intensity profile according to

$$P(t) = \left\{ {\begin{array}{*{20}{c}} {{P_0}\left( {1 - {{\left( {t/\tau } \right)}^2}} \right)\:{\rm{for}}\;\left| t \right| < \tau }\\ {0\; {\rm{otherwise}}} \end{array}} \right.$$

Figure 1 shows an approximately parabolic pulse, as it can result from pulse propagation in a fiber amplifier under certain circumstances. Parabolic pulses have a number of remarkable properties, which have turned out to be particularly important in the context of fiber amplifiers for generating high-energy ultrashort pulses.

parabolic pulse
Figure 1: Temporal profile of a nearly parabolic pulse, such as can be generated in a fiber amplifier fed with Gaussian pulses. Such simulations can be made with the software RP Fiber Power.

Up-chirped parabolic pulses can be generated in a fiber amplifier where the amplified pulses not only experience optical gain, but also the Kerr nonlinearity and normal chromatic dispersion. In this situation, a chirped parabolic pulse is the asymptotic solution for long propagation lengths [3, 8]. After a sufficiently long propagation length, associated with a sufficiently large amplification factor, the shape of the resulting pulses no longer significantly depends on the shape or duration of the seed pulses, and the peak power and duration after a long propagation length depend only on the seed pulse energy. This is a case of self-similar pulse propagation, since the parabolic pulse shape, although not the pulse duration, is preserved. Therefore, such pulses are sometimes called similaritons. The pulse duration parameter is

$$\tau = 3{g^{ - 2/3}}{\left( {\gamma {\beta _2}/2} \right)^{1/3}}{E_{\rm{p}}}^{1/3}$$

where <$g$> is the exponential gain coefficient, and the full bandwidth (not the full width at half maximum) is

$$\Delta \nu = \frac{{{{\left( {g\gamma /2} \right)}^{1/3}}}}{{\pi {\beta _2}^{2/3}}}{E_{\rm{p}}}^{1/3}$$

Both grow with the cubic root of the pulse energy <$E_\textrm{p}$>, so that the time–bandwidth product of the pulses grows in proportion to <$E_\textrm{p}^{2/3}$>.

In the asymptotic regime, the pulses have a very nearly linear up-chirp, i.e., a linearly rising instantaneous frequency, with a growth rate of the instantaneous frequency which is independent of the pulse energy:

$$\frac{{\partial \nu }}{{\partial t}} = \frac{g}{{6\pi {\beta _2}}}$$

Calculator for Parabolic Pulses

Dispersion:(1 fs2 = 1e-30 s2)
Pulse energy:calc
Pulse duration:calc

Enter input values with units, where appropriate. After you have modified some values, click a “calc” button to recalculate the field left of it.

The default values in this form correspond to a pulse energy of 1 nJ in the diagram below.

With increasing propagation length, the peak power rises in proportion to <$E_\textrm{p}^{2/3}$>. The chirp rate (in THz/ps) approaches a constant value, which is determined only by the fiber dispersion and gain per unit length. The spectral bandwidth rises in proportion to the pulse duration, i.e., in proportion to <$E_\textrm{p}^{1/3}$>.

evolution of pulse duration
Figure 2: Evolution of the pulse duration in a hypothetical amplifier with infinite gain bandwidth.

The solid curves show the pulse duration in the amplifier (blue) and after a compressor with optimized GDD (red). The dashed curve shows the asymptotic values, which in this case are reached after ≈ 20 dB of amplification.

case study parabolic pulse fiber amplifier

Case Studies

Case Study, Parabolic Pulses in a Fiber Amplifier

We explore the regime of parabolic pulse amplification in an Yb-doped single-mode fiber. We find suitable system parameters and investigate limiting effects.

Depending on the input pulse parameters, in particular on the pulse duration and energy, the parabolic evolution may set in only after some amount of linear amplification. Therefore, the pulse duration and bandwidth do not necessarily rise by orders of magnitude even if the pulse energy is increased by several orders of magnitude. This is shown in Figure 2, where the seed pulses had 10 pJ energy and 500 fs duration. Initially, the amplification is nearly linear, but then both the bandwidth and pulse duration begin to rise significantly. Due to the increased bandwidth, dispersive compression of the pulses after fiber propagation can lead to a pulse duration significantly below that of the initial pulses.

Note that the limited gain bandwidth of a real fiber amplifier limits the pulse energy range in which parabolic pulse amplification is possible. The parameters in Figure 2 go far beyond that limit, making the simulation somewhat unrealistic in that sense. Numerical simulations can of course take into account a finite gain bandwidth and can thus be used to test to which extent self-similar pulse propagation is practically possible.

Attractions of Parabolic Pulse Amplification

The remarkable properties of parabolic pulses lead to a number of technologically attractive features of fiber amplifiers for ultrashort pulses, when they are designed as “parabolic amplifiers”:

  • Wave breaking is safely avoided. The pulses generated have no significant side lobes in the temporal or spectral shape.
  • Such an amplifier does not require a seed source with carefully chosen pulse parameters, as these are not important provided that the amplification factor is large enough. The seed pulses may be significantly longer than the output pulses. They should not be too long, however, as otherwise the asymptotic solution is only slowly approached.
  • The fiber parameters (chromatic dispersion, nonlinearity and gain) are also not critical. (This is remarkably different to schemes based on soliton effects.)
  • As the amplified pulses have a nearly linear chirp, it is relatively easy to obtain nearly transform-limited pulses by dispersive pulse compression. However, higher-order chromatic dispersion of the compressor should not be excessive.
  • The chirp during amplification can be an important advantage because the amplification of transform-limited pulses could lead to excessive nonlinear phase shifts. The situation is therefore similar to that of chirped-pulse amplification, but with a lower amount of pulse stretching.

Limitations arise from the following effects:

  • The limited gain bandwidth effectively limits the possible pulse energy. For ytterbium-doped fibers with standard mode areas, it is of the order of some tens of nJ – far below the saturation energy. Therefore, with a parabolic pulse one can only extract a minor part of the stored energy in the fiber. This regime is thus most suitable for amplifying pulse trains with very high repetition rates but moderate pulse energies.
  • In principle, the amplified pulse could generate a high Raman gain at some longer wavelengths, so that a strong Stokes pulse would be formed, and the original pulse would be distorted. However, a high enough Raman gain for that problem is usually not reached in a parabolic pulse amplifier.
  • Higher-order chromatic dispersion of the fiber and a compressor should not be too strong.
  • Amplifier noise may also be relevant under certain circumstances.

To find an optimized design of a parabolic amplifier, it is advisable to study its behavior with numerical pulse propagation modeling, including the potentially disturbing effects mentioned above.

The principle of parabolic pulse amplification has also been applied to mode-locked fiber lasers [6] (similariton fiber lasers, Mamyshev oscillators). Here, the spectral width of the circulating pulse is strongly oscillating: it increases during amplification but is reset in every round trip by some optical filter. This approach makes it possible to reach significantly higher pulse energies with potentially cheap fiber laser sources.

More to Learn

Case studies:

Encyclopedia articles:


[1]D. Anderson et al., “Wave-breaking-free pulses in nonlinear-optical fibers”, J. Opt. Soc. Am. B 10 (7), 1185 (1993); https://doi.org/10.1364/JOSAB.10.001185
[2]K. Tamura and M. Nakazawa, “Pulse compression by nonlinear pulse evolution with reduced optical wave breaking in erbium-doped fiber amplifiers”, Opt. Lett. 21 (1), 68 (1996); https://doi.org/10.1364/OL.21.000068
[3]M. E. Fermann et al., “Self-similar propagation and amplification of parabolic pulses in optical fibers”, Phys. Rev. Lett. 84 (26), 6010 (2000); https://doi.org/10.1103/PhysRevLett.84.6010
[4]V. I. Kruglov et al., “Self-similar propagation of high-power parabolic pulses in optical fiber amplifiers”, Opt. Lett. 25 (24), 1753 (2000); https://doi.org/10.1364/OL.25.001753
[5]T. Hirooka and M. Nakazawa, “Parabolic pulse generation by use of a dispersion-decreasing fiber with normal group-velocity dispersion”, Opt. Lett. 29 (5), 498 (2004); https://doi.org/10.1364/OL.29.000498
[6]F. Ö. Ilday et al., “Self-similar evolution of parabolic pulses in a laser”, Phys. Rev. Lett. 92 (21), 213902 (2004); https://doi.org/10.1103/PhysRevLett.92.213902
[7]C. K. Nielsen et al., “Self-starting self-similar all-polarization maintaining Yb-doped fiber laser”, Opt. Express 13 (23), 9346 (2005); https://doi.org/10.1364/OPEX.13.009346
[8]V. I. Kruglov and J. D. Harvey, “Asymptotically exact parabolic solutions of the generalized nonlinear Schrödinger equation with varying parameters”, J. Opt. Soc. Am. B 23 (12), 2541 (2006); https://doi.org/10.1364/JOSAB.23.002541
[9]T. Schreiber et al., “Microjoule-level all-polarization-maintaining femtosecond fiber source”, Opt. Lett. 31 (5), 574 (2006); https://doi.org/10.1364/OL.31.000574
[10]A. Ruehl et al., “Dynamics of parabolic pulses in an ultrafast fiber laser”, Opt. Lett. 31 (18), 2734 (2006); https://doi.org/10.1364/OL.31.002734
[11]J. M. Dudley et al., “Self-similarity and scaling phenomena in nonlinear ultrafast optics”, Nature Phys. 3, 597 (2007); https://doi.org/10.1038/nphys705
[12]D. N. Papadopoulos et al., “Generation of 63 fs 4.1 MW peak power pulses from a parabolic fiber amplifier operated beyond the gain bandwidth limit”, Opt. Lett. 32 (17), 2520 (2007); https://doi.org/10.1364/OL.32.002520
[13]P. Sidorenko and F. Wise, “Generation of 1 μJ and 40 fs pulses from a large mode area gain-managed nonlinear amplifier”, Opt. Lett. 45 (14), 4084 (2020); https://doi.org/10.1364/OL.396683
[14]R. Paschotta, tutorial on "Fiber Amplifiers", part 8 on ultrafast amplifiers

(Suggest additional literature!)

Dr. R. Paschotta

This encyclopedia is authored by Dr. Rüdiger Paschotta, the founder and executive of RP Photonics AG. How about a tailored training course from this distinguished expert at your location? Contact RP Photonics to find out how his technical consulting services (e.g. product designs, problem solving, independent evaluations, training) and software could become very valuable for your business!

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