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Journal of Radio Electronics

On the relationship between the delay time of a narrowband signal |in a dispersing medium and its attenuation

Nikolai S. Bukhman

Published May 1, 2024• 0 citations
Publisher

Abstract

The 1D problem of propagation of a narrowband signal in a homogeneous dispersing medium is considered. It is shown that there is a direct and immediate relationship between the additional (to vacuum) delay time of the signal and its attenuation during propagation in an absorbing medium. It is shown that with an additional delay time of more than several tens of coherence times of uniformly broadened spectral lines of the medium, the signal weakens by hundreds of decibels and therefore practically disappears. On the other hand, when the delay of the signal is less than the coherence time of the medium, its absorption is small. A similar situation arises in an amplifying (thermodynamically nonequilibrium) environment – of course, with the replacement of signal attenuation with its amplification and the replacement of signal delay with its advance. As an example, the propagation of a narrowband signal, the carrier frequency of which is outside the gain band of the space maser, is considered. It is shown that in this case, due to the long lifetime of the excited states of interstellar gas molecules, the signal propagates at superluminal velocity with practically no change in amplitude, which is very rare in problems of this type.

DOI
10.30898/1684-1719.2024.5.12

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The 1D problem of propagation of a narrowband signal in a homogeneous dispersing medium is considered. It is shown that there is a direct and immediate relationship between the additional (to vacuum) delay time of the signal and its attenuation during propagation in an absorbing medium. It is shown that with an additional delay time of more than several tens of coherence times of uniformly broadened spectral lines of the medium, the signal weakens by hundreds of decibels and therefore practically disappears. On the other hand, when the delay of the signal is less than the coherence time of the medium, its absorption is small. A similar situation arises in an amplifying (thermodynamically nonequilibrium) environment – of course, with the replacement of signal attenuation with its amplification and the replacement of signal delay with its advance. As an example, the propagation of a narrowband signal, the carrier frequency of which is outside the gain band of the space maser, is considered. It is shown that in this case, due to the long lifetime of the excited states of interstellar gas molecules, the signal propagates at superluminal velocity with practically no change in amplitude, which is very rare in problems of this type.
It is shown that the average group velocity over the signal spectrum (both subluminal and superluminal) describes the movement of the «center of gravity» of not all, but a wide class of narrowband signals for any length of the path, including beyond the range of applicability of the first order of the classical theory of dispersion, where the time dependence of the signal is usually significantly distorted. The absorption dispersion inevitably distorts the frequency distribution of the signal spectrum as the length of the path increases, so its group velocity changes accordingly. So, in particular, the initial superluminal group velocity may change to sublight as the length of the route increases. Moreover, for any signals with an unlimited spectrum (including for any signals of artificial origin), with a sufficient length of the route, this is inevitable. The reverse transition from sublight group velocity to superluminal velocity is impossible. It is shown that any signal with a carrier frequency located near the central frequency of the spectral absorption line travels at the initial section of the path with a superluminal group velocity, and its absorption is insignificant. Of course, as the length of the route increases, this superluminal group speed usually changes to sublight.
It is shown that the delay time of a weak signal propagating in an amplifying medium on the wings of the spectral amplification line may be shorter than the time of propagation of the signal with the velocity of light in vacuum. It is found that in this case, the time dependence of the signal is exactly 'reconstructed' at the point of detection, and the detection of the signal continues even if it is abruptly terminated at the point of transmission. It is also shown that using the complex time of group delay of the signal, it is possible to improve the accuracy of the results in the first order of dispersion theory within this approximation.
Abstract This paper considers the question of superluminal (or negative) group velocities of signals in dispersive media, as well as negative group delay times of signals passing through linear filters. It is shown that information can be transmitted only with the help of jumps in the time dependence of a function or its derivatives and, therefore, the information propagation velocity in any (including dispersive, absorbing, or amplifying) medium exactly coincides with the speed of light in vacuum. As for the group velocity of a wave packet, it is only the propagation velocity of its infinitely differentiable envelope, by means of which the transmission of information, strictly speaking, is impossible. Therefore, in regions with anomalous dispersion, the group velocity can be superluminal or negative without violating the “light limitation” of the theory of relativity or the principle of causality. Examples of situations in which superluminal or negative group velocity occurs are given.
It is shown that in a selectively absorbing medium, the propagation velocity of a linearly frequency-modulated signal differs from its group velocity and depends on its modulation index, and the "modulation" addition to the group delay time reverses its sign when the sign of the modulation index changes. As a result, the propagation velocity of a linearly frequency-modulated signal can be superluminal at its subluminal group velocity and superluminal at its subluminal group velocity. When the center of the spectral line falls within the spectrum of a linearly frequency–modulated signal, a single linearly frequency-modulated signal is divided into two signals, one of which propagates at a speed higher than the group velocity (possibly higher than the vacuum light velocity), and the second is lower than the group velocity. The difference in the propagation speed of linearly frequency-modulated signals differing in the sign of the modulation index can lead to the fact that the initially amplitude-modulated signal, when propagating in a selectively absorbing medium, can be divided into several signals propagating at different speeds, and these signals, under certain conditions, can also be purely amplitude-modulated. Obviously, these effects can occur not only when a signal propagates in a selectively absorbing medium, but also when it is reflected from a selectively absorbing surface and propagated through linear filters in circuit theory.
The transfer function for transmission through a maser medium is derived. It is valid within the dynamic range of linear maser response and under the assumption of weak dispersion. All signal distortions due to propagation in a maser medium may be canceled by subsequent propagation in a complementary absorbing medium. The signal leaves the cascaded media undistorted with a delay corresponding to propagation at the vacuum velocity of light. This possibility of recovering the speed of light makes it difficult to talk of the propagation of information in a dispersive medium as taking place at a signal velocity below that of light. A potentially useful scheme is shown in which a severely distorting low-noise maser amplifier is used. After further amplification the signal distortions are eliminated by transmission through a complementary absorbing medium. The mathematical form of the transfer functions also leads to a new integral formula involving Bessel functions.