# Phase Noise

Definition: noise of the optical phase of a beam or of an electric signal

German: Phasenrauschen

The output of a single-frequency laser is not perfectly monochromatic but rather exhibits some phase noise, i.e., fluctuations of the optical phase. This leads to a finite linewidth of the laser output. The same applies to the frequency components of the output of a mode-locked laser, i.e. to the lines of the emitted frequency comb.

The fundamental origin of phase noise is quantum noise, in particular spontaneous emission of the gain medium into the resonator modes, but also quantum noise associated with optical losses. In addition, there can be technical noise influences, e.g. due to vibrations of the cavity mirrors or to temperature fluctuations. In many cases, there is also a coupling of intensity noise to phase noise, e.g. via nonlinearities (see, e.g., the article on the linewidth enhancement factor).

Phase noise may occur in the form of a continuous frequency drift, or as sudden phase jumps, or as a combination of both.

## Quantification of Phase Noise

Phase noise can be quantified by the power spectral density *S*_{φ}(*f*) of the phase deviations, having units of rad^{2}/Hz (or simply Hz^{−1}, as radians are dimensionless).
This power spectral density often diverges for zero frequency, so that an r.m.s. value with integration down to zero frequency can not be specified.
For simple random-walk processes, the specification of a coherence time or coherence length or of a linewidth value can be appropriate.
See the article on noise specifications for more details.

Phase noise is directly related to frequency noise, as the instantaneous frequency is essentially the temporal derivative of the phase.
For example, white (frequency-independent) frequency noise corresponds to phase noise with *S*_{φ}(*f*) ≈ 1 / *f*^{2}.

## Measurement of Optical Phase Noise

Phase noise measurements are often based on a recorded beat note between two lasers on a fast photodiode.
Alternatively, it is possible to record a beat note of the laser output with a different portion of the same laser output, which is subject to a long delay, e.g. by propagation through a long span of optical fiber (→ *self-heterodyne linewidth measurement*).
For more details on possible measurements, see the article on the term linewidth.

## Optical Phase Noise Versus Timing Jitter

Sometimes there is a confusion between optical phase noise (as discussed above) and timing jitter of a mode-locked laser, because timing jitter can also be seen as a kind of phase noise: a timing change by one pulse period (i.e. the inverse pulse repetition rate) can be interpreted as a phase change of 2π.
Such a phase can be called *timing phase*.
The corresponding phase noise may be denoted as “timing phase noise” in order to avoid confusion.
Of course, mode-locked lasers also exhibit optical phase noise in all lines of the emitted frequency combs.

## Comparison of Normalized Phase Noise

When comparing the level of phase noise of different oscillators, it is often appropriate to normalize it to the corresponding oscillator frequencies. In frequency metrology, it is common to use the quantity

which is the magnitude of phase fluctuations divided by the mean angular frequency.
The quantity of *x*(*t*) does not change e.g. when digital oscillating signal is sent through a frequency divider, which reduces the phase fluctuations in proportion to the mean frequency.
A comparison of optimized low-noise lasers, which are stabilized to some optical frequency standard, with high-quality microwave oscillators in terms of phase noise, shows that lasers normally have a higher level of phase noise δφ(*t*) but a lower level of normalized phase noise *x*(*t*), which means that they are superior e.g. when used as clocks.
Even without any stabilization, a laser can have a very low phase noise level at high noise frequencies, making it very suitable as a *fly-wheel oscillator*.

## Suppliers

The **RP Photonics Buyer's Guide** contains 4 suppliers for equipment for phase noise measurements. Among them:

### OEwaves

OEwaves’ HI-Q™ Optical Test Measurement System OE4000 utilizes a homodyne methodology for automated measurement capable of testing ultra-low phase noise laser sources. The user-friendly test system is capable of rapidly measuring <10 Hz of Lorentzian linewidth of a laser source without the complicated setup typically required to make such a narrow linewidth measurement.

This homodyne-based system is unique in wideband measurement without requiring another low noise reference laser source. The complete system operates with ease, speed and precision, and a simple graphic user interface via a PC, without requiring any additional test equipment. The unmatched ultra-low phase/frequency noise analyzer system is scalable to various input wavelengths and capable of low relative intensity noise (RIN) measurement.

### Bibliography

[1] | A. L. Schawlow and C. H. Townes, “Infrared and optical masers”, Phys. Rev. 112 (6), 1940 (1958) (contains the famous Schawlow–Townes equation) |

[2] | R. Paschotta et al., “Optical phase noise and carrier–envelope offset noise of mode-locked lasers”, Appl. Phys. B 82 (2), 265 (2006) |

[3] | R. Paschotta, "Noise in Laser Technology – Part 1: Intensity and Phase Noise" |

See also: coherence, coherence time, linewidth, optical phase, Schawlow–Townes linewidth, self-heterodyne linewidth measurement, optical heterodyne detection, noise specifications, power spectral density, frequency noise, intensity noise, frequency metrology, timing jitter, laser noise

and other articles in the category fluctuations and noise

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