A phase-locked, self-referenced frequency comb generated by a mode-locked fiber soliton laser with a tunable repetition rate is presented. The spacing of the frequency comb is set by the laser’s repetition rate, which can be scanned from 49.3 MHz to 50.1 MHz while one tooth of the comb is held phase-locked to a stable RF source. This variable repetition-rate frequency comb should be useful for wavelength and length metrology, synchronization of different fiber laser-based frequency combs, and the generation of precise swept wavelength sources.
© 2004 Optical Society of America
Phase-locked self-referenced fiber-laser-based frequency comb sources have been developed for precision infrared frequency metrology using a figure-eight fiber laser , a pulse-compression mode-locked fiber laser , and several different designs of fiber ring lasers [3–5]. The basic designs of the fiber-laser frequency combs duplicate that used for Ti:Sapphire laser-based frequency combs [6, 7]; an octave-spanning supercontinuum  is generated and used to detect the carrier envelope offset (CEO) frequency [9, 10]. Unlike their Ti:sapphire laser-based counterparts, fiber laser-based frequency combs can be relatively compact and operate in the telecommunications band. As a result, they are of particular importance for telecommunications and optical sensing applications.
Here we describe a frequency comb based on a passively mode-locked soliton laser  with a tunable repetition rate. The high gain of the fiber laser allows us to change its repetition rate by 800 kHz, or ~1.6 %, using a fiber-coupled free-space delay line with a ~1 dB insertion loss. By injecting amplified pulses from the soliton laser into highly nonlinear fiber, we can generate the octave of supercontinuum bandwidth needed to self-reference the frequency comb using the standard f-to-2f interferometer . In a closely related work, a passively mode-locked fiber laser with a variable repetition rate was recently demonstrated ; here we demonstrate that the repetition rate can be significantly changed while the laser remains mode-locked and the comb offset frequency remains phase-locked to a microwave reference.
The optical frequency of the n th tooth of a self-referenced comb is given by the simple expression f n = nf r + f 0, where f r is the repetition rate and f 0 is the comb offset frequency, set by the CEO frequency. The CEO frequency is given by f 0 = (ω0/2π)(1-v g/v p), where ω0 is the carrier frequency of the laser pulse, and v g (v p) is the appropriately averaged group (phase) velocity around the fiber laser cavity. For the fiber laser, f 0 ~ 2.5 THz. However, in metrology experiments using a self-referenced comb, the offset frequency is typically defined modulo f r to a range -f r/2 < f 0 < +f r/2, so that it represents the frequency of the lowest comb line if the optical comb were to be extended to zero frequency. Using this definition, here we phase-locked the up-shifted offset frequency at 2f r + f 0. (This frequency was convenient given the available electronics.) With this comb tooth fixed, a change in the repetition rate leads to an elastic-tape or accordion-like expansion of the entire frequency comb about this fixed point . In other words, a change in the laser’s repetition rate of 800 kHz corresponds to a 3 THz (25 nm) change of a comb tooth in the 1550 nm region. There are many attractive features of a frequency comb with a tunable repetition rate. First, it can be used for precision metrology without a wavelength meter . Second, it can be used to match the repetition rate of a second frequency comb, which can be useful, for example, for tests of the stability of the frequency comb . Third, a frequency comb with a tunable repetition rate can be used to scan precisely the frequency of a continuous wave laser locked to the comb.
2. The fiber-laser-based infrared supercontinuum source
The supercontinuum source (Fig. 1) consists of an additive pulse mode-locked (APM) erbium fiber ring laser , an erbium-doped fiber amplifier (EDFA), and a length of UV-exposed dispersion-flattened, highly nonlinear, dispersion-shifted fiber (HNLF) . The APM fiber laser has a net negative cavity dispersion and produces solitonic pulses with a spectral bandwidth of 20 nm (Fig. 2(a)) and a chirped output of 210 fs duration. The cavity has 1 m of normal dispersion erbium-doped fiber, 0.3 m of single-mode fiber (SMF) at 1060 nm, and 2.7 m of SMF at 1550 nm. The net cavity dispersion was -0.04 ps2 neglecting the dispersion of any components. The pulse spectrum exhibits Kelly sidebands that are typically found in the output of a soliton laser . A commercial fiber-coupled free-space, motor driven delay line in the fiber laser cavity allows the repetition rate to be changed from 49.34 MHz to 50.12 MHz (i.e., a total delay of 310 ps). The insertion loss of the delay line ranges from ~0.75 dB to 1 dB. The delay can be scanned quickly (128 ps/s) without any loss of mode-locking. Longer delays may be possible provided that the variation of insertion loss over a scan is minimized.
To produce the supercontinuum needed to self-reference the frequency comb output of the laser, pulses from the laser are amplified to an average power of 60 mW, and temporally compressed to less than 90 fs in the EDFA (Fig. 2(b)) before being injected into UV-exposed HNLF. The HNLF uses a combination of Ge and F dopants to produce a nonlinear coefficient of γ ~ 10.6 W-1 km-1, a dispersion of 1.74 ps/(nm km), and a dispersion slope of 0.009 ps/(nm2 km) at 1550 nm. In order to enhance the supercontinuum generation, this HNLF was exposed to UV radiation , which increased the refractive index of the Ge-doped core, enhancing the short wavelength (<1100 nm) portion of the supercontinuum. To generate a supercontinuum, a 40 cm length of HNLF with a 15 cm UV-exposed portion was used. As seen in Fig. 3(a), the generated supercontinuum spanned from 1000 nm to 2100 nm (~157 THz wide).
The CEO frequency is measured by mixing 1030 nm light with frequency-doubled 2060 nm light in an f-to-2f interferometer . A dichroic mirror at the HNLF fiber output transmits the supercontinuum above 1800 nm. The 2060 nm light is frequency doubled by second-harmonic generation in a 1 mm thick KNbO3 crystal. This light is then combined on a beamsplitter with the fundamental light at 1030 nm, filtered by a 15 nm bandpass filter (BPF), and launched into a single-mode fiber to ensure spatial overlap. The interference between the fundamental 1030 nm light and the doubled 2060 nm light is detected with a 125 MHz InGaAs photoreceiver, producing the RF spectrum shown in Fig. 3(b). The FWHM of the CEO beat signal is ~1 MHz, which is slightly larger than observed in previous work [1, 2, 9], and may be due to greater amplification of intrinsic laser noise because of the longer initial pulse .
3. Scanning the repetition rate
To demonstrate the variable repetition-rate frequency comb, the CEO frequency was locked and the repetition rate of the laser was scanned by moving the in-cavity delay line. The repetition rate was free-running for these data, although it could be phase-locked at a given repetition rate by feeding back to the intracavity PZT stretcher . The CEO frequency was locked as shown in Fig. 4. The phase-locked CEO frequency had a standard deviation of ~25 mHz for a fixed (i.e. phase-locked) repetition rate. Because of the choice of bandpass filter at 120 MHz the frequency that was actually fixed during a scan (i.e. phase-locked to the RF oscillator) was the up-shifted CEO frequency 2f r + f 0, rather than simply f 0. As a result, the offset frequency does change during the scan by -2δf r where δf r is the change in repetition rate. (The sign of f 0 ~+20 MHz was verified by measuring a heterodyne signal with a fixed laser while varying both f 0 and f r.) During a repetition rate scan, pump power changes of a few mW were required to maintain the CEO frequency phase-lock.
5Figure 5 shows the divided-down CEO frequency for repetition rate scans over 47 kHz (Fig. 5(a)) and the full range of 800 kHz Figs. 5(b)–(c)). Occasional cycle slips occurred due to the relatively low signal-to-noise ratio (SNR) of the CEO beat note. Figures 5(b)–(c) demonstrate different scan speeds from 0.62 kHz/s to 19.91 kHz/s; due to mechanical vibrations the phase-locking of the CEO frequency became more difficult as the scan velocity was increased. Higher SNR of this signal should further improve the stability of the phase-lock at high scan speeds. Nevertheless, excluding the cycle slips, the CEO frequency in a 1 s gate is phase-locked to better than a few hertz even for the worst-case example of Fig. 5(c). The corresponding contribution to the instability of the optical comb frequencies is 10-14 or less, which is negligible for most applications.
4. Applications for frequency metrology: the “accordion” frequency comb
A phase-locked frequency comb with a variable comb tooth separation has many potential uses for infrared frequency metrology. For example, the ability to sweep the comb tooth separation over a large range allows one to unambiguously identify an unknown laser frequency in a heterodyne measurement without using a wavelength meter to distinguish the mode number of the nearest comb tooth  (even for a relatively noisy unknown laser frequency). The ability is particularly attractive for the fiber-laser frequency comb since otherwise the ambiguity of 50 MHz in the mode number must be removed by using the highest-accuracy wavelength meter commercially available. Also, as noted in Ref. , the tunable repetition rate will allow synchronization between two optical frequency combs for tests of comb stability . Note that the alternative approach of building two fiber lasers with the identical repetition rates by cutting the fiber to the appropriate length is virtually impossible to achieve. A final important application of the variable repetition rate laser is to scan a CW laser precisely in frequency by locking it to a single comb tooth of the supercontinuum. Figure 6 depicts a CW laser locked to the n~4 millionth tooth of a frequency comb with a fixed CEO frequency. If f 0 is phase-locked while the repetition rate is changed from f r to f r+δf r then each n th comb tooth moves in frequency by nδf r. The frequency comb expands likes the bellows of an accordion, with the higher-frequency components experiencing a larger absolute frequency change. If the CW laser remains locked to the n th comb tooth, then the CW laser frequency will also change by nδf r. For our soliton laser, a change in its repetition rate by 800 kHz would correspond to a 3 THz change in the optical frequency of a comb tooth around 1550 nm. A CW laser locked to this comb tooth would then experience continuous tuning over 3 THz (25 nm) or over much of the C-band. A CW laser can also be scanned using a fixed frequency comb , but this is technically challenging because of the multiple RF beat signals present in the full heterodyne signal and the difficult hand-over of the phase-lock from one tooth of the comb to the next. The method proposed here of locking the CW laser to the same swept comb tooth has the significant advantage that no hand-over is required and that the heterodyne signal between the CW laser and the n th tooth is at a fixed RF frequency.
We have demonstrated the ability to phase-lock the CEO frequency of an all-fiber frequency comb while scanning its repetition rate, thus altering the comb spacing while one tooth of the comb is phase-locked to a stable RF source. A phase-locked frequency comb with a variable comb tooth separation has many potential benefits for near-infrared frequency metrology.
We thank S. Diddams, S. Gilbert, and D. J. Jones for helpful discussions and L. Hollberg for assistance with the locking electronics.
References and links
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