In optics, **dispersion** is the phenomenon in which the phase velocity of a wave depends on its frequency.^{ [1] } Media having this common property may be termed *dispersive media*. Sometimes the term ** chromatic dispersion** is used for specificity. Although the term is used in the field of optics to describe light and other electromagnetic waves, dispersion in the same sense can apply to any sort of wave motion such as acoustic dispersion in the case of sound and seismic waves, in gravity waves (ocean waves), and for telecommunication signals along transmission lines (such as coaxial cable) or optical fiber. Physically, dispersion translates in a loss of kinetic energy through absorption.

- Examples
- Material and waveguide dispersion
- Material dispersion in optics
- Group velocity dispersion
- Dispersion control
- In waveguides
- Higher-order dispersion over broad bandwidths
- Spatial dispersion
- In gemology
- In imaging
- Pulsar emissions
- See also
- References
- External links

In optics, one important and familiar consequence of dispersion is the change in the angle of refraction of different colors of light,^{ [2] } as seen in the spectrum produced by a dispersive prism and in chromatic aberration of lenses. Design of compound achromatic lenses, in which chromatic aberration is largely cancelled, uses a quantification of a glass's dispersion given by its Abbe number *V*, where *lower* Abbe numbers correspond to *greater* dispersion over the visible spectrum. In some applications such as telecommunications, the absolute phase of a wave is often not important but only the propagation of wave packets or "pulses"; in that case one is interested only in variations of group velocity with frequency, so-called group-velocity dispersion.

The most familiar example of dispersion is probably a rainbow, in which dispersion causes the spatial separation of a white light into components of different wavelengths (different colors). However, dispersion also has an effect in many other circumstances: for example, group velocity dispersion causes pulses to spread in optical fibers, degrading signals over long distances; also, a cancellation between group-velocity dispersion and nonlinear effects leads to soliton waves.

Most often, chromatic dispersion refers to bulk material dispersion, that is, the change in refractive index with optical frequency. However, in a waveguide there is also the phenomenon of *waveguide dispersion*, in which case a wave's phase velocity in a structure depends on its frequency simply due to the structure's geometry. More generally, "waveguide" dispersion can occur for waves propagating through any inhomogeneous structure (e.g., a photonic crystal), whether or not the waves are confined to some region.^{[ dubious – discuss ]} In a waveguide, *both* types of dispersion will generally be present, although they are not strictly additive.^{[ citation needed ]} For example, in fiber optics the material and waveguide dispersion can effectively cancel each other out to produce a zero-dispersion wavelength, important for fast fiber-optic communication.

Material dispersion can be a desirable or undesirable effect in optical applications. The dispersion of light by glass prisms is used to construct spectrometers and spectroradiometers. Holographic gratings are also used, as they allow more accurate discrimination of wavelengths. However, in lenses, dispersion causes chromatic aberration, an undesired effect that may degrade images in microscopes, telescopes, and photographic objectives.

The * phase velocity *, *v*, of a wave in a given uniform medium is given by

where *c* is the speed of light in a vacuum and *n* is the refractive index of the medium.

In general, the refractive index is some function of the frequency *f* of the light, thus *n* = *n*(*f*), or alternatively, with respect to the wave's wavelength *n* = *n*(*λ*). The wavelength dependence of a material's refractive index is usually quantified by its Abbe number or its coefficients in an empirical formula such as the Cauchy or Sellmeier equations.

Because of the Kramers–Kronig relations, the wavelength dependence of the real part of the refractive index is related to the material absorption, described by the imaginary part of the refractive index (also called the extinction coefficient). In particular, for non-magnetic materials (*μ* = *μ*_{0}), the susceptibility *χ* that appears in the Kramers–Kronig relations is the electric susceptibility *χ*_{e} = *n*^{2} − 1.

The most commonly seen consequence of dispersion in optics is the separation of white light into a color spectrum by a prism. From Snell's law it can be seen that the angle of refraction of light in a prism depends on the refractive index of the prism material. Since that refractive index varies with wavelength, it follows that the angle that the light is refracted by will also vary with wavelength, causing an angular separation of the colors known as *angular dispersion*.

For visible light, refraction indices *n* of most transparent materials (e.g., air, glasses) decrease with increasing wavelength *λ*:

or alternatively:

In this case, the medium is said to have *normal dispersion*. Whereas, if the index increases with increasing wavelength (which is typically the case in the ultraviolet^{ [4] }), the medium is said to have *anomalous dispersion*.

At the interface of such a material with air or vacuum (index of ~1), Snell's law predicts that light incident at an angle *θ* to the normal will be refracted at an angle arcsin(sin *θ*/*n*). Thus, blue light, with a higher refractive index, will be bent more strongly than red light, resulting in the well-known rainbow pattern.

Beyond simply describing a change in the phase velocity over wavelength, a more serious consequence of dispersion in many applications is termed group velocity dispersion (GVD). While phase velocity *v* is defined as *v* = *c*/*n*, this describes only one frequency component. When different frequency components are combined together, as when considering a signal or a pulse, one is often more interested in the group velocity which describes the speed at which a pulse or information superimposed on a wave (modulation) propagates. In the accompanying animation, it can be seen that the wave itself (orange-brown) travels at a phase velocity which is much faster than the speed of the *envelope* (black) which corresponds to the group velocity. This pulse might be a communications signal, for instance, and its information only travels at the group velocity rate even though it consists of wavefronts advancing at a faster rate (the phase velocity).

It is possible to calculate the group velocity from the refractive index curve *n*(*ω*) or more directly from the wavenumber *k* = *ωn*/*c* where *ω* is the radian frequency *ω*=2*πf*. Whereas one expression for the phase velocity is *v _{p}=ω/k*, the group velocity can be expressed using the derivative:

When dispersion is present, not only will the group velocity not be equal to the phase velocity, but generally will itself vary with wavelength. This is known as group velocity dispersion and causes a short pulse of light to be broadened, as the different frequency components within the pulse travel at different velocities. Group velocity dispersion is quantified as the derivative of the *reciprocal* of the group velocity with respect to radian frequency which results in *group velocity dispersion* = *d*^{2}*k*/*dω*^{2}.

If a light pulse is propagated through a material with positive group-velocity dispersion, then the shorter wavelength components travel slower than the longer wavelength components. The pulse therefore becomes *positively chirped *, or *up-chirped*, increasing in frequency with time. On the other hand, if a pulse travels through a material with negative group-velocity dispersion, shorter wavelength components travel faster than the longer ones, and the pulse becomes *negatively chirped*, or *down-chirped*, decreasing in frequency with time.

The *group velocity dispersion parameter*:

is often used to quantify GVD, that is proportional to *D* through a negative factor:

According to some authors a medium is said to have *normal dispersion*/*anomalous dispersion* for a certain vacuum wavelength *λ*_{0} if the *second* derivative of the refraction index calculated in *λ*_{0} is positive/negative or, equivalently, if *D*(*λ*_{0}) is negative/positive.^{ [5] } This definition concerns group velocity dispersion and should not be confused with the one given in previous section. The two definitions do not coincide in general, so the reader has to understand the context.

The result of GVD, whether negative or positive, is ultimately temporal spreading of the pulse. This makes dispersion management extremely important in optical communications systems based on optical fiber, since if dispersion is too high, a group of pulses representing a bit-stream will spread in time and merge, rendering the bit-stream unintelligible. This limits the length of fiber that a signal can be sent down without regeneration. One possible answer to this problem is to send signals down the optical fibre at a wavelength where the GVD is zero (e.g., around 1.3–1.5 μm in silica fibres), so pulses at this wavelength suffer minimal spreading from dispersion. In practice, however, this approach causes more problems than it solves because zero GVD unacceptably amplifies other nonlinear effects (such as four wave mixing). Another possible option is to use soliton pulses in the regime of negative dispersion, a form of optical pulse which uses a nonlinear optical effect to self-maintain its shape. Solitons have the practical problem, however, that they require a certain power level to be maintained in the pulse for the nonlinear effect to be of the correct strength. Instead, the solution that is currently used in practice is to perform dispersion compensation, typically by matching the fiber with another fiber of opposite-sign dispersion so that the dispersion effects cancel; such compensation is ultimately limited by nonlinear effects such as self-phase modulation, which interact with dispersion to make it very difficult to undo.

Dispersion control is also important in lasers that produce short pulses. The overall dispersion of the optical resonator is a major factor in determining the duration of the pulses emitted by the laser. A pair of prisms can be arranged to produce net negative dispersion, which can be used to balance the usually positive dispersion of the laser medium. Diffraction gratings can also be used to produce dispersive effects; these are often used in high-power laser amplifier systems. Recently, an alternative to prisms and gratings has been developed: chirped mirrors. These dielectric mirrors are coated so that different wavelengths have different penetration lengths, and therefore different group delays. The coating layers can be tailored to achieve a net negative dispersion.

Waveguides are highly dispersive due to their geometry (rather than just to their material composition). Optical fibers are a sort of waveguide for optical frequencies (light) widely used in modern telecommunications systems. The rate at which data can be transported on a single fiber is limited by pulse broadening due to chromatic dispersion among other phenomena.

In general, for a waveguide mode with an angular frequency *ω*(*β*) at a propagation constant *β* (so that the electromagnetic fields in the propagation direction *z* oscillate proportional to *e*^{i(βz−ωt)}), the group-velocity dispersion parameter *D* is defined as:^{ [6] }

where *λ* = 2π*c*/*ω* is the vacuum wavelength and *v*_{g} = *dω*/*dβ* is the group velocity. This formula generalizes the one in the previous section for homogeneous media, and includes both waveguide dispersion and material dispersion. The reason for defining the dispersion in this way is that |*D*| is the (asymptotic) temporal pulse spreading Δ*t* per unit bandwidth Δ*λ* per unit distance travelled, commonly reported in ps/nm/km for optical fibers.

In the case of multi-mode optical fibers, so-called modal dispersion will also lead to pulse broadening. Even in single-mode fibers, pulse broadening can occur as a result of polarization mode dispersion (since there are still two polarization modes). These are *not* examples of chromatic dispersion as they are not dependent on the wavelength or bandwidth of the pulses propagated.

When a broad range of frequencies (a broad bandwidth) is present in a single wavepacket, such as in an ultrashort pulse or a chirped pulse or other forms of spread spectrum transmission, it may not be accurate to approximate the dispersion by a constant over the entire bandwidth, and more complex calculations are required to compute effects such as pulse spreading.

In particular, the dispersion parameter *D* defined above is obtained from only one derivative of the group velocity. Higher derivatives are known as *higher-order dispersion*.^{ [7] }^{ [8] } These terms are simply a Taylor series expansion of the dispersion relation *β*(*ω*) of the medium or waveguide around some particular frequency. Their effects can be computed via numerical evaluation of Fourier transforms of the waveform, via integration of higher-order slowly varying envelope approximations, by a split-step method (which can use the exact dispersion relation rather than a Taylor series), or by direct simulation of the full Maxwell's equations rather than an approximate envelope equation.

In electromagnetics and optics, the term *dispersion* generally refers to aforementioned temporal or frequency dispersion. Spatial dispersion refers to the non-local response of the medium to the space; this can be reworded as the wavevector dependence of the permittivity. For an exemplary anisotropic medium, the spatial relation between electric and electric displacement field can be expressed as a convolution:^{ [9] }

where the kernel is dielectric response (susceptibility); its indices make it in general a tensor to account for the anisotropy of the medium. Spatial dispersion is negligible in most macroscopic cases, where the scale of variation of is much larger than atomic dimensions, because the dielectric kernel dies out at macroscopic distances. Nevertheless, it can result in non-negligible macroscopic effects, particularly in conducting media such as metals, electrolytes and plasmas. Spatial dispersion also plays role in optical activity and Doppler broadening,^{ [9] } as well as in the theory of metamaterials.^{ [10] }

Name | B–G | C–F |
---|---|---|

Cinnabar (HgS) | 0.40 | — |

Synth. rutile | 0.330 | 0.190 |

Rutile (TiO_{2}) | 0.280 | 0.120–0.180 |

Anatase (TiO_{2}) | 0.213–0.259 | — |

Wulfenite | 0.203 | 0.133 |

Vanadinite | 0.202 | — |

Fabulite | 0.190 | 0.109 |

Sphalerite (ZnS) | 0.156 | 0.088 |

Sulfur (S) | 0.155 | — |

Stibiotantalite | 0.146 | — |

Goethite (FeO(OH)) | 0.14 | — |

Brookite (TiO_{2}) | 0.131 | 0.12–1.80 |

Zincite (ZnO) | 0.127 | — |

Linobate | 0.13 | 0.075 |

Synthetic moissanite (SiC) | 0.104 | — |

Cassiterite (SnO_{2}) | 0.071 | 0.035 |

Zirconia (ZrO_{2}) | 0.060 | 0.035 |

Powellite (CaMoO_{4}) | 0.058 | — |

Andradite | 0.057 | — |

Demantoid | 0.057 | 0.034 |

Cerussite | 0.055 | 0.033–0.050 |

Titanite | 0.051 | 0.019–0.038 |

Benitoite | 0.046 | 0.026 |

Anglesite | 0.044 | 0.025 |

Diamond (C) | 0.044 | 0.025 |

Flint glass | 0.041 | — |

Hyacinth | 0.039 | — |

Jargoon | 0.039 | — |

Starlite | 0.039 | — |

Zircon (ZrSiO_{4}) | 0.039 | 0.022 |

GGG | 0.038 | 0.022 |

Scheelite | 0.038 | 0.026 |

Dioptase | 0.036 | 0.021 |

Whe Vinay wellite | 0.034 | — |

Alabaster | 0.033 | — |

Gypsum | 0.033 | 0.008 |

Epidote | 0.03 | 0.012–0.027 |

Achroite | 0.017 | — |

Cordierite | 0.017 | 0.009 |

Danburite | 0.017 | 0.009 |

Dravite | 0.017 | — |

Elbaite | 0.017 | — |

Herderite | 0.017 | 0.008–0.009 |

Hiddenite | 0.017 | 0.010 |

Indicolite | 0.017 | — |

Liddicoatite | 0.017 | — |

Kunzite | 0.017 | 0.010 |

Rubellite | 0.017 | 0.008–0.009 |

Schorl | 0.017 | — |

Scapolite | 0.017 | — |

Spodumene | 0.017 | 0.010 |

Tourmaline | 0.017 | 0.009–0.011 |

Verdelite | 0.017 | — |

Andalusite | 0.016 | 0.009 |

Baryte (BaSO_{4}) | 0.016 | 0.009 |

Euclase | 0.016 | 0.009 |

Alexandrite | 0.015 | 0.011 |

Chrysoberyl | 0.015 | 0.011 |

Hambergite | 0.015 | 0.009–0.010 |

Phenakite | 0.01 | 0.009 |

Rhodochrosite | 0.015 | 0.010–0.020 |

Sillimanite | 0.015 | 0.009–0.012 |

Smithsonite | 0.014–0.031 | 0.008–0.017 |

Amblygonite | 0.014–0.015 | 0.008 |

Aquamarine | 0.014 | 0.009–0.013 |

Beryl | 0.014 | 0.009–0.013 |

Brazilianite | 0.014 | 0.008 |

Celestine | 0.014 | 0.008 |

Goshenite | 0.014 | — |

Heliodor | 0.014 | 0.009–0.013 |

Morganite | 0.014 | 0.009–0.013 |

Pyroxmangite | 0.015 | — |

Synth. scheelite | 0.015 | — |

Dolomite | 0.013 | — |

Magnesite (MgCO_{3}) | 0.012 | — |

Synth. emerald | 0.012 | — |

Synth. alexandrite | 0.011 | — |

Synth. sapphire (Al_{2}O_{3}) | 0.011 | — |

Phosphophyllite | 0.010–0.011 | — |

Enstatite | 0.010 | — |

Anorthite | 0.009–0.010 | — |

Actinolite | 0.009 | — |

Jeremejevite | 0.009 | — |

Nepheline | 0.008–0.009 | — |

Apophyllite | 0.008 | — |

Hauyne | 0.008 | — |

Natrolite | 0.008 | — |

Synth. quartz (SiO_{2}) | 0.008 | — |

Aragonite | 0.007–0.012 | — |

Augelite | 0.007 | — |

Tanzanite | 0.030 | 0.011 |

Thulite | 0.03 | 0.011 |

Zoisite | 0.03 | — |

YAG | 0.028 | 0.015 |

Almandine | 0.027 | 0.013–0.016 |

Hessonite | 0.027 | 0.013–0.015 |

Spessartine | 0.027 | 0.015 |

Uvarovite | 0.027 | 0.014–0.021 |

Willemite | 0.027 | — |

Pleonaste | 0.026 | — |

Rhodolite | 0.026 | — |

Boracite | 0.024 | 0.012 |

Cryolite | 0.024 | — |

Staurolite | 0.023 | 0.012–0.013 |

Pyrope | 0.022 | 0.013–0.016 |

Diaspore | 0.02 | — |

Grossular | 0.020 | 0.012 |

Hemimorphite | 0.020 | 0.013 |

Kyanite | 0.020 | 0.011 |

Peridot | 0.020 | 0.012–0.013 |

Spinel | 0.020 | 0.011 |

Vesuvianite | 0.019–0.025 | 0.014 |

Clinozoisite | 0.019 | 0.011–0.014 |

Labradorite | 0.019 | 0.010 |

Axinite | 0.018–0.020 | 0.011 |

Ekanite | 0.018 | 0.012 |

Kornerupine | 0.018 | 0.010 |

Corundum (Al_{2}O_{3}) | 0.018 | 0.011 |

Rhodizite | 0.018 | — |

Ruby (Al_{2}O_{3}) | 0.018 | 0.011 |

Sapphire (Al_{2}O_{3}) | 0.018 | 0.011 |

Sinhalite | 0.018 | 0.010 |

Sodalite | 0.018 | 0.009 |

Synth. corundum | 0.018 | 0.011 |

Diopside | 0.018–0.020 | 0.01 |

Emerald | 0.014 | 0.009–0.013 |

Topaz | 0.014 | 0.008 |

Amethyst (SiO_{2}) | 0.013 | 0.008 |

Anhydrite | 0.013 | — |

Apatite | 0.013 | 0.010 |

Apatite | 0.013 | 0.008 |

Aventurine | 0.013 | 0.008 |

Citrine | 0.013 | 0.008 |

Morion | 0.013 | — |

Prasiolite | 0.013 | 0.008 |

Quartz (SiO_{2}) | 0.013 | 0.008 |

Smoky quartz (SiO_{2}) | 0.013 | 0.008 |

Rose quartz (SiO_{2}) | 0.013 | 0.008 |

Albite | 0.012 | — |

Bytownite | 0.012 | — |

Feldspar | 0.012 | 0.008 |

Moonstone | 0.012 | 0.008 |

Orthoclase | 0.012 | 0.008 |

Pollucite | 0.012 | 0.007 |

Sanidine | 0.012 | — |

Sunstone | 0.012 | — |

Beryllonite | 0.010 | 0.007 |

Cancrinite | 0.010 | 0.008–0.009 |

Leucite | 0.010 | 0.008 |

Obsidian | 0.010 | — |

Strontianite | 0.008–0.028 | — |

Calcite (CaCO_{3}) | 0.008–0.017 | 0.013–0.014 |

Fluorite (CaF_{2}) | 0.007 | 0.004 |

Hematite | 0.500 | — |

Synthetic cassiterite (SnO_{2}) | 0.041 | — |

Gahnite | 0.019–0.021 | — |

Datolite | 0.016 | — |

Tremolite | 0.006–0.007 | — |

In the technical terminology of gemology, *dispersion* is the difference in the refractive index of a material at the B and G (686.7 nm and 430.8 nm) or C and F (656.3 nm and 486.1 nm) Fraunhofer wavelengths, and is meant to express the degree to which a prism cut from the gemstone demonstrates "fire". Fire is a colloquial term used by gemologists to describe a gemstone's dispersive nature or lack thereof. Dispersion is a material property. The amount of fire demonstrated by a given gemstone is a function of the gemstone's facet angles, the polish quality, the lighting environment, the material's refractive index, the saturation of color, and the orientation of the viewer relative to the gemstone.^{ [11] }^{ [12] }

In photographic and microscopic lenses, dispersion causes chromatic aberration, which causes the different colors in the image not to overlap properly. Various techniques have been developed to counteract this, such as the use of achromats, multielement lenses with glasses of different dispersion. They are constructed in such a way that the chromatic aberrations of the different parts cancel out.

It has been suggested that this section be split out into another articletitled Dispersion measure . (Discuss) (November 2015) |

Pulsars are spinning neutron stars that emit pulses at very regular intervals ranging from milliseconds to seconds. Astronomers believe that the pulses are emitted simultaneously over a wide range of frequencies. However, as observed on Earth, the components of each pulse emitted at higher radio frequencies arrive before those emitted at lower frequencies. This dispersion occurs because of the ionized component of the interstellar medium, mainly the free electrons, which make the group velocity frequency dependent. The extra delay added at a frequency ν is

where the dispersion constant *k*_{DM} is given by

^{ [13] }

and the **dispersion measure** (DM) is the column density of free electrons (total electron content) — i.e. the number density of electrons *n*_{e} (electrons/cm^{3}) integrated along the path traveled by the photon from the pulsar to the Earth — and is given by

with units of parsecs per cubic centimetre (1 pc/cm^{3} = 30.857 × 10^{21} m^{−2}).^{ [14] }

Typically for astronomical observations, this delay cannot be measured directly, since the emission time is unknown. What *can* be measured is the difference in arrival times at two different frequencies. The delay Δ*t* between a high frequency ν_{hi} and a low frequency ν_{lo} component of a pulse will be

Rewriting the above equation in terms of Δ*t* allows one to determine the DM by measuring pulse arrival times at multiple frequencies. This in turn can be used to study the interstellar medium, as well as allow for observations of pulsars at different frequencies to be combined.

- Abbe number
- Calculation of glass properties incl. dispersion
- Cauchy's equation
- Dispersion relation
- Fast radio burst (astronomy)
- Fluctuation theorem
- Green–Kubo relations
- Group delay
- Intramodal dispersion
- Kramers–Kronig relations
- Linear response function
- Multiple-prism dispersion theory
- Sellmeier equation
- Ultrashort pulse
- Virtually imaged phased array

The **group velocity** of a wave is the velocity with which the overall envelope shape of the wave's amplitudes—known as the *modulation* or *envelope* of the wave—propagates through space.

The **phase velocity** of a wave is the rate at which the wave propagates in some medium. This is the velocity at which the phase of any one frequency component of the wave travels. For such a component, any given phase of the wave will appear to travel at the phase velocity. The phase velocity is given in terms of the wavelength λ (lambda) and time period T as

In optics, the **refractive index** of a material is a dimensionless number that describes how fast light travels through the material. It is defined as

In physics, the **wavelength** is the **spatial period** of a periodic wave—the distance over which the wave's shape repeats. It is the distance between consecutive corresponding points of the same phase on the wave, such as two adjacent crests, troughs, or zero crossings, and is a characteristic of both traveling waves and standing waves, as well as other spatial wave patterns. The inverse of the wavelength is called the spatial frequency. Wavelength is commonly designated by the Greek letter *lambda* (λ). The term *wavelength* is also sometimes applied to modulated waves, and to the sinusoidal envelopes of modulated waves or waves formed by interference of several sinusoids.

In physics, mathematics, and related fields, a **wave** is a propagating dynamic disturbance of one or more quantities, sometimes as described by a wave equation. In physical waves, at least two field quantities in the wave medium are involved. Waves can be periodic, in which case those quantities oscillate repeatedly about an equilibrium (resting) value at some frequency. When the entire waveform moves in one direction it is said to be a **traveling wave**; by contrast, a pair of superimposed periodic waves traveling in opposite directions makes a standing wave. In a standing wave, the amplitude of vibration has nulls at some positions where the wave amplitude appears smaller or even zero.

In physics and electrical engineering, a **cutoff frequency**, **corner frequency**, or **break frequency** is a boundary in a system's frequency response at which energy flowing through the system begins to be reduced rather than passing through.

The **reflectance** of the surface of a material is its effectiveness in reflecting radiant energy. It is the fraction of incident electromagnetic power that is reflected at the boundary. Reflectance is a component of the response of the electronic structure of the material to the electromagnetic field of light, and is in general a function of the frequency, or wavelength, of the light, its polarization, and the angle of incidence. The dependence of reflectance on the wavelength is called a *reflectance spectrum* or *spectral reflectance curve*.

In the physical sciences, the **wavenumber** is the spatial frequency of a wave, measured in cycles per unit distance or radians per unit distance. Whereas temporal frequency can be thought of as the number of waves per unit time, wavenumber is the number of waves per unit distance.

The **Kerr effect**, also called the **quadratic electro-optic** (**QEO**) **effect**, is a change in the refractive index of a material in response to an applied electric field. The Kerr effect is distinct from the Pockels effect in that the induced index change is directly proportional to the *square* of the electric field instead of varying linearly with it. All materials show a Kerr effect, but certain liquids display it more strongly than others. The Kerr effect was discovered in 1875 by John Kerr, a Scottish physicist.

In optics, **group velocity dispersion** (GVD) is a characteristic of a dispersive medium, used most often to determine how the medium will affect the duration of an optical pulse traveling through it. Formally, GVD is defined as the derivative of the inverse of group velocity of light in a material with respect to angular frequency,

In the physical sciences and electrical engineering, **dispersion relations** describe the effect of dispersion on the properties of waves in a medium. A dispersion relation relates the wavelength or wavenumber of a wave to its frequency. Given the dispersion relation, one can calculate the phase velocity and group velocity of waves in the medium, as a function of frequency. In addition to the geometry-dependent and material-dependent dispersion relations, the overarching Kramers–Kronig relations describe the frequency dependence of wave propagation and attenuation.

An **optical ring resonator** is a set of waveguides in which at least one is a closed loop coupled to some sort of light input and output. The concepts behind optical ring resonators are the same as those behind whispering galleries except that they use light and obey the properties behind constructive interference and total internal reflection. When light of the resonant wavelength is passed through the loop from input waveguide, it builds up in intensity over multiple round-trips due to constructive interference and is output to the output bus waveguide which serves as a detector waveguide. Because only a select few wavelengths will be at resonance within the loop, the optical ring resonator functions as a filter. Additionally, as implied earlier, two or more ring waveguides can be coupled to each other to form an add/drop optical filter.

In fluid dynamics, **dispersion** of water waves generally refers to frequency dispersion, which means that waves of different wavelengths travel at different phase speeds. Water waves, in this context, are waves propagating on the water surface, with gravity and surface tension as the restoring forces. As a result, water with a free surface is generally considered to be a dispersive medium.

**Self-phase modulation** (SPM) is a nonlinear optical effect of light-matter interaction. An ultrashort pulse of light, when travelling in a medium, will induce a varying refractive index of the medium due to the optical Kerr effect. This variation in refractive index will produce a phase shift in the pulse, leading to a change of the pulse's frequency spectrum.

A **fiber Bragg grating** (**FBG**) is a type of distributed Bragg reflector constructed in a short segment of optical fiber that reflects particular wavelengths of light and transmits all others. This is achieved by creating a periodic variation in the refractive index of the fiber core, which generates a wavelength-specific dielectric mirror. Hence a fiber Bragg grating can be used as an inline optical fiber to block certain wavelengths or it can be used as wavelength-specific reflector.

**Penetration depth** is a measure of how deep light or any electromagnetic radiation can penetrate into a material. It is defined as the depth at which the intensity of the radiation inside the material falls to 1/e of its original value at the surface.

**Acousto-optics** is a branch of physics that studies the interactions between sound waves and light waves, especially the diffraction of laser light by ultrasound through an ultrasonic grating.

In optics, the term **soliton** is used to refer to any optical field that does not change during propagation because of a delicate balance between nonlinear and linear effects in the medium. There are two main kinds of solitons:

When an electromagnetic wave travels through a medium in which it gets attenuated, it undergoes exponential decay as described by the Beer–Lambert law. However, there are many possible ways to characterize the wave and how quickly it is attenuated. This article describes the mathematical relationships among:

In physics and engineering, the **envelope** of an oscillating signal is a smooth curve outlining its extremes. The envelope thus generalizes the concept of a constant amplitude into an *instantaneous amplitude*. The figure illustrates a modulated sine wave varying between an *upper envelope* and a *lower envelope*. The envelope function may be a function of time, space, angle, or indeed of any variable.

- ↑ Born, Max; Wolf, Emil (October 1999).
*Principles of Optics*. Cambridge: Cambridge University Press. pp. 14–24. ISBN 0-521-64222-1. - ↑ Dispersion Compensation Retrieved 25-08-2015.
- ↑ Calculation of the Mean Dispersion of Glasses
- ↑ Born, M. and Wolf, E. (1980) "Principles of Optics, 6th ed." pg. 93. Pergamon Press.
- ↑ Saleh, B.E.A. and Teich, M.C.
*Fundamentals of Photonics (2nd Edition)*Wiley, 2007. - ↑ Ramaswami, Rajiv and Sivarajan, Kumar N. (1998)
*Optical Networks: A Practical Perspective*. Academic Press: London. - ↑ Chromatic Dispersion,
*Encyclopedia of Laser Physics and Technology*(Wiley, 2008). - ↑ Mai, Wending; Campbell, Sawyer D.; Whiting, Eric B.; Kang, Lei; Werner, Pingjuan L.; Chen, Yifan; Werner, Douglas H. (2020-10-01). "Prismatic discontinuous Galerkin time domain method with an integrated generalized dispersion model for efficient optical metasurface analysis".
*Optical Materials Express*.**10**(10): 2542–2559. doi: 10.1364/OME.399414 . ISSN 2159-3930. - 1 2 Landau, L. D.; Lifshitz, E. M.; Pitaevskii, L. P. (1984).
*Electrodynamics of Continuous Media*.**8**(2nd ed.). Butterworth-Heinemann. ISBN 978-0-7506-2634-7. - ↑ Demetriadou, A.; Pendry, J. B. (1 July 2008). "Taming spatial dispersion in wire metamaterial".
*Journal of Physics: Condensed Matter*.**20**(29): 295222. Bibcode:2008JPCM...20C5222D. doi:10.1088/0953-8984/20/29/295222. - 1 2 Schumann, Walter (2009).
*Gemstones of the World: Newly Revised & Expanded Fourth Edition*. Sterling Publishing Company, Inc. pp. 41–2. ISBN 978-1-4027-6829-3 . Retrieved 31 December 2011. - ↑ "What is Gemstone Dispersion?".
*GemSociety.org*. International Gem Society. Retrieved 2015-03-09. - ↑ Single-Dish Radio Astronomy: Techniques and Applications, ASP Conference Proceedings, Vol. 278. Edited by Snezana Stanimirovic, Daniel Altschuler, Paul Goldsmith, and Chris Salter. ISBN 1-58381-120-6. San Francisco: Astronomical Society of the Pacific, 2002, p. 251-269
- ↑ Lorimer, D.R., and Kramer, M.,
*Handbook of Pulsar Astronomy*, vol. 4 of Cambridge Observing Handbooks for Research Astronomers, (Cambridge University Press, Cambridge, U.K.; New York, U.S.A, 2005), 1st edition.

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