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| A '''frequency comb''' is a [[light]] source whose spectrum consists of a series of discrete, equally spaced elements. Frequency combs can be generated by a number of mechanisms, including [[amplitude modulation]] of a continuous wave laser or stabilization of the pulse train generated by a [[modelocking|mode locked laser]]. Much work has been devoted to the latter mechanism, which was developed around the turn of the twenty first century and ultimately lead to one half of the [[Nobel Prize in Physics]] being shared by [[John L. Hall]] and [[Theodor W. Hänsch]] in 2005.
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| The [[frequency domain]] representation of a perfect frequency comb is a series of delta functions spaced according to | |
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| <math>
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| f(n) = f_0 + n\,f_r
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| </math>
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| where <math>n</math> is an integer, <math>f_r</math> is the comb tooth spacing (equal to the mode locked laser's repetition rate or, alternatively, the AM frequency) <math>f_0</math> is the carrier offset frequency, which is less than <math>f_r</math>.
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| Combs spanning an octave in frequency (i.e., a factor of two) can be used to directly measure (and correct for drifts in) <math>f_0</math>. Thus, octave spanning combs can be used to steer a [[Mirror mount|piezoelectric mirror]] within a carrier envelope phase correcting feedback loop. Any mechanism by which the combs' two degrees of freedom (<math>f_r</math> and <math>f_0</math>) are stabilized generate a comb that is useful for mapping optical frequencies into the radio frequency for the direct measurement of optical frequency.
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| [[File:Ultrashort_pulse.svg|thumb|400px|right|An [[ultrashort pulse]] of light in the time domain. The electric field is a sinusoid with a Gaussian envelope.]]
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| [[File:Dirac comb.svg|thumb|300px|A Dirac comb is an infinite series of [[Dirac delta function]]s spaced at intervals of ''T''.]]
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| == Frequency comb generation ==
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| [[modelocking|Modelock]]ed lasers produce a series of optical pulses separated in time by the round-trip time of the laser cavity. The spectrum of such a pulse train approximates a series of [[Dirac delta function]]s separated by the repetition rate (the inverse of the round trip time) of the laser.
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| This series of sharp spectral lines is called a frequency comb or a frequency [[Dirac comb]].
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| A purely electronic device, which generates a series of pulses, also generates a frequency comb. These are produced for electronic sampling [[oscilloscopes]], but also used for frequency comparison of microwaves, because they reach up to 1 THz. Since they include 0 Hz they do not need the tricks which make up the rest of this article.
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| ==Frequency comb widening to one octave==
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| To be usable, the comb must be widened to at least an [[Octave (electronics)|octave]]: that is, the highest-frequency must be at least double the lowest frequency. One of three techniques may be used:
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| * [[supercontinuum]] generation by strong self-phase modulation in nonlinear [[photonic crystal fiber]]
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| *a Ti:sapphire laser using intracavity [[self-phase modulation]]
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| *the second harmonic can be generated in a long crystal so that by consecutive sum frequency generation and difference frequency generation the spectrum of first and second harmonic widens until they overlap.
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| == Carrier-envelope offset measurement ==
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| Each line is displaced from a harmonic of the repetition rate by the carrier-envelope offset frequency. The carrier-envelope offset frequency is the rate at which the peak of the carrier frequency slips from the peak of the pulse envelope on a pulse-to-pulse basis.
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| Measurement of the carrier-envelope offset frequency is usually done with a self-referencing technique, in which the phase of one part of the spectrum is compared to its harmonic.
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| In the 'frequency − 2 × frequency' technique, light at the lower energy side of the broadened spectrum is doubled using [[second harmonic generation]] in a nonlinear crystal and a [[heterodyne]] beat is generated between that and light at the same wavelength on the upper energy side of the spectrum. This beat frequency, detectable with a [[photodiode]], is the carrier-envelope offset frequency.
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| Alternatively, from light at the higher energy side of the broadened spectrum the frequency at the peak of the spectrum is subtracted in a nonlinear crystal and a [[heterodyne]] beat is generated between that and light at the same wavelength on the lower energy side of the spectrum. This beat frequency, detectable with a [[photodiode]], is the carrier-envelope offset frequency.
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| Because the [[Phase detector|phase is measured directly]] and not the frequency, it is possible to set the frequency to zero and additionally lock the phase, but because the intensity of the laser and this detector is not very stable, and because the whole spectrum beats in phase
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| [http://www.attoworld.de/publications/Doctoral_Theses/Rauschenberger_thesis_2007.pdf source],
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| one has to lock the phase on a fraction of the repetition rate.
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| == Carrier-envelope offset control ==
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| In the absence of active stabilization, the repetition rate and carrier-envelope offset frequency would be free to drift. They vary with changes in the cavity length, refractive index of laser optics, and nonlinear effects such as the [[Kerr effect]]. The repetition rate can be stabilized using a [[piezoelectric]] transducer, which moves a mirror to change the cavity length.
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| In Ti:sapphire lasers using [[prism (optics)|prism]]s for dispersion control, the carrier-envelope offset frequency can be controlled by tilting the high reflector mirror at the end of the prism pair. This can be done using piezoelectric transducers.
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| In high repetition rate Ti:sapphire ring lasers, which often use double-chirped mirrors to control dispersion, modulation of the pump power using an [[acousto-optic modulator]] is often used to control the offset frequency. The phase slip depends strongly on the Kerr effect, and by changing the pump power one changes the peak intensity of the laser pulse and thus the size of the Kerr phase shift. This shift is far smaller than 6 rad, so an additional device for coarse adjustment is needed.
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| {{See also|phase-locked loop}}
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| The breakthrough which led to a practical frequency comb was the development of technology for stabilizing the carrier-envelope offset frequency.
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| ==Applications==
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| [[File:The laser frequency comb in action.jpg|thumb|The laser frequency comb tested with the [[High Accuracy Radial Velocity Planet Searcher|HARPS]] planet-finder on the [[ESO]] 3.6-metre telescope at the [[La Silla Observatory]].<ref>{{cite news|title=Nobel Prize-Winning Laser Technology to Help Find Earth-like Planets|url=http://www.eso.org/public/announcements/ann12037/|accessdate=31 May 2012|newspaper=ESO Announcement}}</ref> ]]
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| A '''frequency comb''' allows a direct link from [[radio frequency]] standards to optical frequencies. Current frequency standards such as [[atomic clocks]] operate in the [[microwave]] region of the spectrum, and the frequency comb brings the accuracy of such clocks into the optical part of the electromagnetic spectrum. A simple electronic feedback loop can lock the repetition rate to a frequency standard.
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| There are two distinct applications of this technique. One is the '''optical clock''' where an optical frequency is overlapped with a single tooth of the comb on a photodiode and a radio frequency is compared to the beat signal, the repetition rate, and the CEO-frequency. Applications for the frequency comb technique include optical [[metrology]], frequency chain generation, optical [[atomic clocks]], high precision spectroscopy, and more precise [[GPS]] technology.<ref>[http://archive.nrc-cnrc.gc.ca/eng/projects/inms/optical-comb.html Optical frequency comb for dimensional metrology, atomic and molecular spectroscopy, and precise time keeping]</ref>
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| The other is doing experiments with [[Ultrashort pulse|few cycle pulses]], like [[above threshold ionization]], [[Attophysics|attosecond pulse]]s, highly efficient [[nonlinear optics]] or [[Harmonic generation|high harmonics generation]]. This can be single pulses so that no comb exists and therefore it is not possible to define a carrier envelope offset frequency, rather the carrier envelope offset phase is important. A second photodiode can be added to the setup to gather phase and amplitude in a single shot, or difference frequency generation can be used to even lock the offset on a single shot basis albeit with low power efficiency.
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| Without an actual comb one can look at the phase vs frequency. Without a carrier envelope offset all frequencies are cosines. That means all frequencies have the phase zero. The time origin is arbitrary. If a pulse comes at later times, the phase increases linearly with frequency, but still the zero frequency phase is zero. This phase at zero frequency is the carrier envelope offset. The second harmonic not only has twice the frequency but also twice the phase. That means for a pulse with zero offset the second harmonic of the low frequency tail is in phase with the fundamental of the high frequency tail and otherwise it is not. [[Spectral phase interferometry for direct electric-field reconstruction]] (SPIDER) measures how the phase increases with frequency, but it cannot determine the offset, so the name “electric field reconstruction” is a bit misleading.
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| == History ==
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| [[Theodor W. Hänsch]] and [[John L. Hall]] shared half of the 2005 [[Nobel Prize]] in Physics for contributions to the development of laser-based precision spectroscopy, including the optical frequency comb technique. The other half of the prize was awarded to [[Roy Glauber]].
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| In 2006 the femtosecond comb technique was extended to the extreme ultraviolet range, enabling frequency metrology in that region of the spectrum.<ref>[http://www.aip.org/pnu/2005/split/735-2.html Ultraviolet Frequency Comb]
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| </ref>
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| ==See also==
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| *[[Atomic clock]]
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| *[[Magneto-optical trap]]
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| ==References==
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| {{reflist|2}}
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| ==Further reading==
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| *{{cite book |title=Femtosecond optical frequency comb |author=John L Hall & Theodor W Hänsch |editor=Jun Ye, Steven T. Cundiff |url=http://jila.colorado.edu/~junye/yelabs/pubs/scienceArticles/2005/sArticle_2005_YeCundiff_CombBook.pdf |chapter=History of optical comb development |isbn=0-387-23790-9 |year=2004 |publisher=Springer}}
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| *{{cite book |title=Ultrafast Optics |author=Andrew M. Weiner |url=http://www.wiley.com/WileyCDA/WileyTitle/productCd-0471415391.html |isbn=978-0-471-41539-8 |year=2009 |publisher=Wiley}}
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| ==External links==
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| *[http://www.nist.gov/public_affairs/images/frequency_comb_animation.htm Frequency Comb Spectroscopy Animation]
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| *[http://www.iop.org/EJ/article/1367-2630/7/1/116/njp5_1_116.html Attosecond control of optical waveforms]
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| *[http://tf.nist.gov/general/pdf/1396.pdf Femtosecond laser comb]
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| *[http://www.nrc-cnrc.gc.ca/eng/projects/inms/optical-comb.html Optical frequency comb for dimensional metrology, atomic and molecular spectroscopy, and precise time keeping]
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| *[http://www.scientificamerican.com/article.cfm?id=measuring-with-lasers&print=true Rulers of Light: Using Lasers to Measure Distance and Time] by Steven Cundiff in Scientific American
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| *[http://www.frequencycomb.com/ World-wide installations of Frequency Combs]
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| [[Category:Nonlinear optics]]
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| [[Category:Laser science]]
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| [[Category:Spectroscopy]]
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