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Coherence is ... Coherence of light waves. Temporal coherence

Consider a wave propagating in space. Coherence is a measure of the correlation between its phases, measured at various points. The coherence of a wave depends on the characteristics of its source.

Two types of coherence

Let's look at a simple example. Imagine two floats rising and falling on the surface of the water. Suppose that the source of the waves is a single stick, which is harmoniously immersed and removed from the water, disturbing the calm surface of the water surface. In this case, there is an ideal correlation between the movements of the two floats. They may not rise and fall exactly in phase, when one goes up and the other down, but the phase difference between the positions of the two floats is constant in time. A harmonically oscillating point source produces an absolutely coherent wave.

When describing the coherence of light waves, there are two types of light waves - temporal and spatial.

Coherence refers to the ability of light to produce an interference pattern. If two light waves are brought together, and they do not create areas of increased and reduced brightness, they are called incoherent. If they produce an "ideal" interference pattern (in the sense of the existence of regions of complete destructive interference), then they are completely coherent. If two waves create a "less perfect" picture, then they are considered to be partially coherent.

Michelson interferometer

Coherence is a phenomenon that is best explained by experiment.

In the Michelson interferometer, the light from the source S (which can be any: the sun, laser or stars) is directed to a semitransparent mirror M 0 that reflects 50% of the light in the direction of the mirror M 1 and passes 50% towards the mirror M 2 . The beam is reflected from each of the mirrors, returns to M 0 , and equal parts of the light reflected from M 1 and M 2 are combined and projected onto screen B. The device can be adjusted by changing the distance from mirror M 1 to the beam splitter.

The Michelson interferometer, in essence, mixes the beam with the delayed time in its own version. The light that passes along the path to the mirror M 1 must travel a distance 2d greater than the beam that moves to the mirror M 2 .

Coherence length and time

What is observed on the screen? For d = 0, we see a lot of very clear interference fringes. When d increases, the bands become less pronounced: dark areas become brighter, and light ones become dimmer. Finally, for very large d, exceeding some critical value of D, the light and dark rings disappear completely, leaving only a blurred spot.

Obviously, the light field can not interfere with the delayed version of itself, if the time delay is sufficiently large. Distance 2D is the coherence length: interference effects are noticeable only when the path difference is less than this distance. This value can be transformed at the time t c by dividing it by the speed of light c: t c = 2D / s.

The Michelson experiment measures the temporal coherence of a light wave: its ability to interfere with a delayed version of itself. In a well-stabilized laser, t c = 10 -4 s, l c = 30 km; For filtered thermal light t c = 10 -8 s, l c = 3 m.

Coherence and time

Temporal coherence is a measure of the correlation between the phases of a light wave at various points along the direction of propagation.

Suppose a source emits waves of length λ and λ ± Δλ that at some point in space will interfere at a distance l c = λ 2 / (2πΔλ). Here l c is the coherence length.

The phase of the wave propagating in the x direction is given by φ = kx - ωt. If we consider the wave pattern in space at time t at a distance l c , the phase difference between two waves with vectors k 1 and k 2 , which are in phase at x = 0, is Δφ = l c (k 1 - k 2 ). When Δφ = 1, or Δφ ~ 60 °, the light is no longer coherent. Interference and diffraction have a significant effect on contrast.

In this way:

  • 1 = l c (k 1 - k 2 ) = l c (2π / λ - 2π / (λ + Δλ));
  • L c (λ + Δλ - λ) / (λ (λ + Δλ)) ~ l c Δλ / λ 2 = 1 / 2π;
  • L c = λ 2 / (2πΔλ).

The wave passes through the space at a speed c.

The coherence time t c = l c / s. Since λf = c, then Δf / f = Δω / ω = Δλ / λ. We can write

  • L c = λ 2 / (2πΔλ) = λf / (2πΔf) = c / Δω;
  • T c = 1 / Δω.

If the wavelength or propagation frequency of a light source is known, l c and t c can be calculated. It is not possible to observe an interference pattern obtained by dividing an amplitude, such as thin-film interference, if the optical path difference significantly exceeds l c .

The temporal coherence speaks of the monochrome nature of the source.

Coherence and space

Spatial coherence is a measure of the correlation between the phases of a light wave at various points transversely with respect to the direction of propagation.

At a distance L from a thermal monochromatic (linear) source, whose linear dimensions are of the order of δ, two slits located at a distance greater than d c = 0.16λL / δ no longer produce a recognizable interference pattern. Πd c 2/4 is the source coherence area.

If you look at a source of width δ at a time t located perpendicular to the distance L from the screen, you can see on the screen two points (P1 and P2) separated by a distance d. The electric field in P1 and P2 is a superposition of the electric fields of the waves emitted by all points of the source, the radiation of which is not related to each other. In order for the electromagnetic waves leaving P1 and P2 to create a recognizable interference pattern, the superpositions in P1 and P2 must be in phase.

Coherence condition

The light waves emitted by the two edges of the source at some instant of time t have a certain phase difference right at the center between two points. A ray going from the left edge δ to the point P2 must pass d (sinθ) / 2 further than the ray directed to the center. The trajectory of the ray going from the right edge δ to the point P2 passes the path to d (sinθ) / 2 less. The path difference for two beams is d · sinθ and represents the phase difference Δφ '= 2πd · sinθ / λ. For a distance from P1 to P2 along the wave front, we obtain Δφ = 2Δφ '= 4πd · sinθ / λ. The waves emitted by the two edges of the source are in phase with P1 at time t and do not coincide in phase at a distance of 4πdsinθ / λ in P2. Since sinθ ~ δ / (2L), then Δφ = 2πdδ / (Lλ). When Δφ = 1 or Δφ ~ 60 °, the light is no longer considered coherent.

Δφ = 1 -> d = Lλ / (2πδ) = 0.16 Lλ / δ.

Spatial coherence indicates the homogeneity of the phase of the wave front.

The incandescent lamp is an example of an incoherent light source.

Coherent light can be obtained from a source of incoherent radiation if the majority of the radiation is discarded. First of all, spatial filtration is performed to increase the spatial coherence, and then spectral filtration to increase temporal coherence.

Fourier series

A sinusoidal plane wave is absolutely coherent in space and time, and its length, time and area of coherence are infinite. All real waves are wave impulses that last for a finite time interval and have a finite perpendicular to their propagation direction. Mathematically, they are described by nonperiodic functions. To find the frequencies present in the wave pulses for determining Δω and the coherence length, it is necessary to analyze the nonperiodic functions.

According to Fourier analysis, an arbitrary periodic wave can be regarded as a superposition of sinusoidal waves. The Fourier synthesis means that the superposition of a plurality of sinusoidal waves makes it possible to obtain an arbitrary periodic waveform.

Communication with statistics

The theory of coherence can be considered as a link between physics and other sciences, since it is the result of the fusion of electromagnetic theory and statistics, as well as statistical mechanics is the union of mechanics with statistics. The theory is used to quantify and characterize the effects of random fluctuations on the behavior of light fields.

It is usually impossible to measure the fluctuations of the wave field directly. Individual "ups and downs" of visible light can not be detected directly or even with complex instruments: its frequency is of the order of 10 15 oscillations per second. Only average values can be measured.

Application of coherence

The connection of physics with other sciences using the example of coherence can be traced in a number of applications. Partially coherent fields are less susceptible to atmospheric turbulence, which makes them useful for laser communications. They are also used in the study of laser-induced reactions of thermonuclear fusion: a decrease in the interference effect leads to a "smooth" action of the beam on the thermonuclear target. Coherence is used, in particular, to determine the size of stars and the separation of binary stellar systems.

The coherence of light waves plays an important role in the study of quantum and also classical fields. In 2005, Roy Glauber became one of the Nobel Prize winners in physics for his contribution to the development of the quantum theory of optical coherence.

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