1. Field of the Invention
The present invention relates in general to a short-pulse amplification technique which employs a laser oscillator that generates pulses with much larger chirps than in known fiber oscillators to reduce the complexity of the overall system design.
2. Description of the Background Art
The generation of femtosecond pulses with energies above 1 μJ from a practical fiber source requires one or more stages of amplification. To avoid excessive nonlinear phase accumulation in the amplifiers, large-mode-area fibers are employed along with chirped-pulse amplification (CPA). A typical fiber CPA system consists of an oscillator, a stretcher, one or more preamplifiers, a large-mode amplifier, and a pulse-picker to optimize the use of the available power and to lower the repetition rate to that appropriate for a given application. Much progress has been made in fiber CPA systems, but to date they have barely begun to supplant solid-state instruments in applications despite their major potential advantages. There is clear motivation to simplify the systems to better exploit the benefits of fiber, particularly greater integration and lower cost.
More particularly, known short-pulse fiber amplifiers employ a low energy, short-pulse, and high repetition-rate oscillator, the output of which must be substantially modified before the pulse can be amplified to a useful energy level. First, the stretcher is employed to stretch the output pulse form the oscillator to greater than 100 ps duration. This stretching is necessary to avoid deleterious nonlinear phase accumulation in the later amplification stages, and the pulse energy is kept low to avoid nonlinear phase shifts in the stretcher. The pulse picker is then used to cut the repetition rate to obtain more energy per pulse for a given average amplifier power, which is limited by available pump power. The modified pulse is then amplified and finally compressed back to close to the transform-limited duration (e.g. on the order of hundreds of femtoseconds). Several pre-amplification stages are generally needed to reach the desired overall gain, which can be as high as 107. The use of a low power oscillator, a pulse stretcher, a lossy and costly pulse picker and several stages of amplification represent costly and inefficient disadvantages to the otherwise desirable CPA based systems. A need clearly exists for a more cost efficient design of a CPA system.
The present invention addresses the foregoing need through provision of a CPA based pulse amplification system that only requires an oscillator, one or more amplifiers and a compressor. This is accomplished through use of a new mode of operation of a fiber oscillator, marked by large pulse energies, large pulse durations and giant pulse chirp. Because of the giant chirp, no stretcher external to the oscillator is needed, as the effect of nonlinear phase accumulation will be small. As a consequence, the energy of the oscillator can be high and can take the place of a stage of pre-amplification. Finally, the oscillator can be designed at very low repetition rates (e.g. less than 10 MHz), thereby erasing the need for a lossy and expensive pulse-picker.
The key to the oscillator design is that the characteristics of the oscillator components, including the length of a single mode fiber (SMF) and the bandwidth of a spectral filter in the oscillator cavity, are selected so that the oscillator has an inherently lower repetition rate and imparts more than 10 ps2 of group-velocity dispersion to the generated pulses. This results in a chirping of the pulse that is on the order of one or two magnitudes greater than the chirp normally imparted to pulses in previous fiber oscillators. Thus, the phrase “giant chirp” is employed here to describe this key characteristic of the resulting oscillator output pulses. Typically, the high energy giant chirped output pulse will have a duration of 100 ps or more, which eliminates the need for an external pulse stretcher and thus allows the use of increased power levels in the oscillator. The giant chirped pulses can readily be dechirped with any suitable compressor back down to hundreds of femtoseconds (e.g. on the order of 1 ps or less). The result is a short pulse with high energy, achieved without the use of external pulse stretchers and pickers, and with less need for multiple stages of amplification.
The features and advantages of the present invention will become apparent from the following detailed description of a preferred embodiment thereof, taken in conjunction with the accompanying drawings which are briefly described as follows.
a and 3b are graphs showing simulation of a GCO with realistic parameters with
a-4d are graphs illustrating results obtained in experiments on a GCO constructed in accordance with the preferred embodiment and operated in the long chirped pulse mode.
a-5d are graphs showing the narrow-bandwidth mode.
As noted previously, the major new component of the fiber amplifier system is the oscillator. The details of a first preferred embodiment will first be discussed followed by a discussion of possible variations. A schematic of a fiber oscillator 10 constructed in accordance with a first preferred embodiment of the invention is shown in
Also disposed in the ring cavity 18 are first and second quarter-waveplates (QWP) 20; a half-waveplate (HWP) 22; a polarizing beam-splitter (PBS) 24; and a wavelength-division multiplexer (WDM) 25. The QWPs 20 and HWP 22 are standard optical elements used to control the state of the polarization which in turn controls nonlinear polarization evolution (NPE), which starts the solution from noise and plays a major role in pulse formation. More particularly, the wave plates 20 and 22 and polarizing beam splitter 24 function as a fast saturable absorber which controls NPE. These NPE controlling components can be replaced with several other types of suitable saturable absorbers, such as a SESAM (semiconductor saturable absorber mirror) or a CNT (carbon nanotube absorber). The PBS 24 is also a standard optical component and serves three purposes. First, it is crucial to have a polarizer for NPE to function, and second, the PBS 24 also serves as an output coupler to generate an output 26 because the beam is split at this point. The pump laser 27 is a 980 single mode pump diode, which is coupled into the gain fiber with the 980/1030 WDM 25.
The PBS 24 also serves as part of a crucial component for this mode of operation, which is a spectral filter 28. The spectral filter 28 is formed from the combination of a birefringent plate 29, an isolator 30 and the PBS 24, which both act as polarizers. The birefringent plate 29 is preferably a standard birefringent piece of quartz. It must be placed between two polarizers, in this case the isolator 30 and the PBS 24, in order to operate as a sinusoidal spectral filter. The bandwidth of the filter is proportional to the thickness of the birefringent plate 29. The birefringent plate 29 is turned at an angle (usually Brewster's angle) to minimize transmission loss. In addition to serving as a polarizer, the optical isolator 30 insures that the light can only propagate in one direction. Without the isolator 30, starting the laser can be very difficult.
Attached to the two ends of the SMF fibers 14 and 16, are first and second 1030 collimators 32 and 34, respectively, which output a beam with 1 mm diameter. This parameter can vary. Regarding the lengths of the SMF fibers 14 and 16, the SMF 16 to the right of the gain fiber 12 should be short (0-1 m) to minimize nonlinearity. The gain fiber 12 should be only long enough to absorb all of the pump power (typically 50 cm-1 m). The SMF fiber 14 to the left of the gain fiber 12 should be long for proper operation of the GCO (>10 m). This long fiber is the main differentiating ingredient for the GCO, the key difference being that it provides a large amount of normal GVD in the cavity, allowing for pulse solutions with large quadratic spectral phase (e.g. greater than 10 ps2).
The GCO 10 forms part of a CPA system 35. The giant chirped output pulses from the oscillator 10 are fed through an amplifier 36 and then through a compressor 38, which compresses the amplified pulses back down to about 1 ps or less in duration. The compressed pulses are then emitted by the CPA system 35 through an output 40. It should be noted that the amplifier 36 can actually be formed from a number of pre-amplifiers and/or amplifiers.
Analysis, realistic numerical simulations and actual experiments were conducted to confirm the behavior and performance of these fiber lasers that operate in a new regime, characterized by the generation of pulses with chirp one to two orders of magnitude larger than can be achieved with existing mode-locked lasers. The pulses, which are dissipative solitons, can be dechirped to near the transform limit. Stable chirped pulses with large energies can be generated at low repetition rates. A GCO may therefore eliminate the stretcher, pulse-picker, and one or more pre-amplifier stages from a conventional fiber CPA system. A system operating at a 3-MHz repetition rate has been experimentally demonstrated, with initial results that reach microjoule pulse energies and sub-picosecond pulse durations.
The fiber laser of
where D is the GVD, g is the net gain and loss, Ω is the filter bandwidth squared, α is a cubic saturable absorber term, δ is a quintic saturable absorber term, γ refers to the cubic refractive nonlinearity of the medium, U is the product of the electric field envelope and √{square root over (γ)}, z is the propagation coordinate and t is the product of the local time and √{square root over (Ω)}, admits the following exact solution:
The variation of Eq. 2 with GVD (see the graph of
To verify and refine the analytical results, numerical simulations of the oscillator were also performed. The simulations include the appropriate terms of the CQGLE with saturating gain, g=go/(1+Epulse/Esat), where go corresponds to 30 dB of small-signal gain,
where A is the electric field envelope, TR is the cavity round trip time and Esat=10 nJ. A 62-m segment of SMF precedes 40 cm of Yb-doped gain fiber, and a 50-cm segment follows it, with β2=230 fs2/cm and γ=0.0047 (Wm)−1. The fiber is followed by a monotonic saturable absorber given by T=1−lo/[1+P(τ)/Psat] where lo=0.7 is the unsaturated loss, P(τ) is the instantaneous pulse power and Psat=0.5 kW is the saturation power. The gain is assumed to have a gaussian spectral profile with a 60 nm bandwidth, the output coupling is 88%, and a gaussian filter with 10 nm bandwidth is placed after the saturable absorber. The 30 nJ output pulse is 70 ps long (
A laser was constructed with all-normal-dispersion elements but with a much longer segment of SMF, as in the simulation of
To assess the utility of the laser for seeding amplifiers, a setup was employed with an SMF preamplifier pumped in-core by a single-mode diode, a large-mode-area (≈1000 μm2) photonic crystal fiber (PCF) main amplifier pumped with as much as 25 W, and a grating compressor. In CPA it is generally desirable to stretch the pulse to the longest duration that can be recompressed, and fiber versions commonly stretch the seed pulse to hundreds of picoseconds. The longest pulses generated by this GCO are shown in
CPA becomes more difficult to implement as the pulse duration increases, owing to the increased dispersion needed to stretch narrow-bandwidth pulses. The pulse spectrum shown in
A number of alternative versions of the invention are possible. The invention applies to any repetition rate with appropriate filter bandwidth. Any wavelength where the cavity has large net normal dispersion (e.g. 1550 nm with added normal dispersion fiber). Any saturable absorber can replace the three waveplate/polarizer combination. For example, a saturable absorbing mirror (SESAM) or a carbon nanotube absorber (CNT) can be employed. In these cases it would be much preferable to use polarization maintaining fiber because one can then avoid solution drift. Any filter implementation is possible, such as for example, an interference filter. It is even possible to use no filter, but with loss of performance. The cavity can be in ring, linear or sigma configurations. Any pumping configuration is also possible including single clad, double clad, etc.
Useful criteria in designing a GCO include the following. First, the giant chirped output pulses from the GCO 10 require greater than 10 ps2 of anomalous GVD to be dechirped in the compressor. As far as the saturable absorber, any suitable type including an NPE, SESAM or CNT should work. The type of oscillator cavity is also not limited to a ring and can include linear or sigma. Regardless of what types of components are selected, the GCO design process is the same. First, the desired repetition rate is selected. The repetition rate determines the required fiber length and the fiber length determines net GVD. Given this GVD, determine the appropriate filter to achieve the required chirp. If the chirp is too high, decrease the filter bandwidth. If the chirp is too low, increase the filter bandwidth. Less GVD requires larger filters for the same chirp. For example, a 3 MHz repetition rate requires ˜60 m of fiber which provides a total GVD of 1.4 ps2. Using a 10 nm filter results in 11 ps2 of spectral phase as in the discussion above.
In summary, the subject invention defines a new operating regime of dissipative soliton lasers, which features long and highly-chirped pulses. In addition to their scientific importance as solutions of a mode-locked laser, these pulses are attractive for femtosecond and picosecond fiber amplifiers. The combination of long pulse duration, low repetition rate, and relatively high pulse energy is unique, and allows the removal of the stretcher, pulse-picker, and one or more pre-amplifiers from previous CPA designs. It is expected that these lasers will enable practical fiber amplifiers with performance well beyond the microjoule level attained in initial experiments.
Although the invention has been disclosed in terms of a preferred embodiment and variations thereon, it will be understood that numerous other modifications and variations could be made without departing from the scope of the invention as defined in the following claims.
The work on this invention was supported by the National Science Foundation under Grant No. ECS-0701680 and the National Institutes of Health under Grant No. EB002019. The Government has certain rights in the invention.
Filing Document | Filing Date | Country | Kind | 371c Date |
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PCT/US2009/064277 | 11/12/2009 | WO | 00 | 9/23/2011 |
Publishing Document | Publishing Date | Country | Kind |
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WO2010/056920 | 5/20/2010 | WO | A |
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20120033690 A1 | Feb 2012 | US |
Number | Date | Country | |
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61113696 | Nov 2008 | US |