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Weber–Fechner law

The Weber–Fechner laws are two related scientific laws in the field of psychophysics, known as Weber's law and Fechner's law. Both relate to human perception, more specifically the relation between the actual change in a physical stimulus and the perceived change. This includes stimuli to all senses: vision, hearing, taste, touch, and smell.

History and formulation of the laws
Both Weber's law and Fechner's law were formulated by Gustav Theodor Fechner (1801–1887). They were first published in 1860 in the work Elemente der Psychophysik (Elements of Psychophysics). This publication was the first work ever in this field, and where Fechner coined the term psychophysics to describe the interdisciplinary study of how humans perceive physical magnitudes. He made the claim that "...psycho-physics is an exact doctrine of the relation of function or dependence between body and soul." Weber's law Ernst Heinrich Weber (1795–1878) was one of the first persons to approach the study of the human response to a physical stimulus in a quantitative fashion. Fechner was a student of Weber and named his first law in honor of his mentor, since it was Weber who had conducted the experiments needed to formulate the law. In sensation and contrast, change is defined as "contrast over time". The senses detect the change; in Weber's law, specifically, it is relative change, not absolute change, which is detected. In Weber's law, to notice a change in stimulus (e.g. brightness or weight), the change must be constant proportion of the original stimulus. Weber's law states that just noticeable difference is proportional to the magnitude of the initial stimulus. The brain is a percentage of change detector. The differential threshold is the smallest difference needed to differentiate two stimuli for each sense has been studied by using similarly methods to signal detection. For instance, holding an object that weighs 1,2,10, and 11lbs. If one were to hold the lightest object (1lb), and then swap out that object for the 2lb object, one could easily tell that the second object is heavier than the first. There is a 100 % weight increase from the first object to the second. However, it becomes more difficult when the difference is a smaller percentage of the initial object's weight. For example, if one were to hold the 10lb object, and then swap it out and hold the 11lb object, it would be difficult for one to tell which of the two is heavier, because there is only a 10 % increase from the first to the second object. This demonstrates that bigger stimuli require a larger difference in order to be noticed. This is Weber's Law. Fechner formulated several versions of the law, all communicating the same idea. One formulation states: What this means is that the perceived change in stimuli is inversely proportional to the initial stimuli. Weber's law also incorporates the just-noticeable difference (JND). Let S be some reference stimulus, and dS_{JND} the smallest change in this stimulus that can be perceived. This means that for any dS the stimulus S\pm dS is indistinguishable from S. Weber's law states that dS_{JND} and S are proportional to one another,dS_{JND} = k S, where k> 0 is some constant of proportionality. Weber's law always fails at low intensities, near and below the absolute detection threshold, and often also at high intensities, but may be approximately true across a wide middle range of intensities. Weber contrast Although Weber's law includes a statement of the proportionality of a perceived change to initial stimuli, Weber only refers to this as a rule of thumb regarding human perception. It was Fechner who formulated this statement as a mathematical expression referred to as Weber contrast. dp = \alpha \frac{dS}{S} \,\! where dp is how much the perception changes when the stimulus, S, changes by an amount dS. \alpha>0 is another proportionality constant. Plugging in the JND, dS=dS_{JND}, we see the proportionality constant in Weber's law is related to the new constant and the smallest perceptual change, dp_{JND}=\alpha k. If dS then Weber's law states that dp=0. In Weber contrast this is not the case, so, though the mathematical relationships look similar, they differ in content. Weber contrast, when integrated, explains Fechner's law (below). Starting at some base stimulus, S_0, and changing it to S, the total change in perception is p(S)-p(S_0)=\alpha \int_{S_0}^S \frac{dS'}{S'}=\ln \left(\frac{S}{S_0}\right)^\alpha. Fechner's law Fechner noticed in his own studies that different individuals have different sensitivity to certain stimuli. For example, the ability to perceive differences in light intensity could be related to how good that individual's vision is. Since Weber's law fails at low intensity, so does Fechner's law. == Types of perception ==
Types of perception
Weber and Fechner conducted research on differences in light intensity and the perceived difference in weight. Following the work of S. S. Stevens, many researchers came to believe in the 1960s that the Stevens's power law was a more general psychophysical principle than Fechner's logarithmic law. Sound Weber's law does not quite hold for loudness. It is a fair approximation for higher intensities, but not for lower amplitudes. Limitation of Weber's law in the auditory system Weber's law does not hold at perception of higher intensities. Intensity discrimination improves at higher intensities. The first demonstration of the phenomena was presented by Riesz in 1928, in Physical Review. This deviation of the Weber's law is known as the "near miss" of the Weber's law. This term was coined by McGill and Goldberg in their paper of 1968 in Perception & Psychophysics. Their study consisted of intensity discrimination in pure tones. Further studies have shown that the near miss is observed in noise stimuli as well. Jesteadt et al. (1977) demonstrated that the near miss holds across all the frequencies, and that the intensity discrimination is not a function of frequency, and that the change in discrimination with level can be represented by a single function across all frequencies: \Delta I / I = 0.463 {(I/I_0)}^{-0.072}. This magnitude scale was invented by the ancient Greek astronomer Hipparchus in about 150 B.C. He ranked the stars he could see in terms of their brightness, with 1 representing the brightest down to 6 representing the faintest, though now the scale has been extended beyond these limits; an increase in 5 magnitudes corresponds to a decrease in brightness by a factor of 100. Limitations of Weber's law in visual regularity perception Perception of Glass patterns and mirror symmetries in the presence of noise follows Weber's law in the middle range of regularity-to-noise ratios (S), but in both outer ranges, sensitivity to variations is disproportionally lower. As Maloney, Mitchison, & Barlow (1987) showed for Glass patterns, and as van der Helm (2010) showed for mirror symmetries, perception of these visual regularities in the whole range of regularity-to-noise ratios follows the law p = g/(2+1/S) with parameter g to be estimated using experimental data. Limitation of Weber's law at low light levels For vision, Weber's law implies constancy of luminance contrast. Suppose a target object is set against a background luminance B. In order to be just visible, the target must be brighter or fainter than the background by some small amount \Delta B. The Weber contrast is defined as C=\Delta B / B, and Weber's law says that C should be constant for all B. Human vision follows Weber's law closely at normal daylight levels (i.e. in the photopic range) but begins to break down at twilight levels (the mesopic range) and is completely inapplicable at low light levels (scotopic vision). This can be seen in data collected by Blackwell and plotted by Crumey, showing threshold increment \Delta B versus background luminance B for various targets sizes. At daylight levels, the curves are approximately straight with slope 1, i.e. \Delta B = B + const., implying C=\Delta B / B is constant. At the very darkest background levels (B ≲ 10− 5 cd m−2, approximately 25 mag arcsec−2) the curves are flat - this is where the only visual perception is the observer's own neural noise ('dark light'). In the intermediate range, a portion can be approximated by the De Vries - Rose law, related to Ricco's law. == Logarithmic coding schemes for neurons ==
Logarithmic coding schemes for neurons
Lognormal distributions Activation of neurons by sensory stimuli in many parts of the brain is by a proportional law: neurons change their spike rate by about 10–30%, when a stimulus (e.g. a natural scene for vision) has been applied. However, as Scheler (2017) showed, the population distribution of the intrinsic excitability or gain of a neuron is a heavy tail distribution, more precisely a lognormal shape, which is equivalent to a logarithmic coding scheme. Neurons may therefore spike with 5–10 fold different mean rates. Obviously, this increases the dynamic range of a neuronal population, while stimulus-derived changes remain small and linear proportional. == Other applications ==
Other applications
The Weber–Fechner law has been applied in other fields of research than just the human senses. Numerical cognition Psychological studies show that it becomes increasingly difficult to discriminate between two numbers as the difference between them decreases. This is called the distance effect. This is important in areas of magnitude estimation, such as dealing with large scales and estimating distances. It may also play a role in explaining why consumers neglect to shop around to save a small percentage on a large purchase, but will shop around to save a large percentage on a small purchase which represents a much smaller absolute dollar amount. Pharmacology It has been hypothesized that dose-response relationships can follow Weber's Law which suggests this law – which is often applied at the sensory level – originates from underlying chemoreceptor responses to cellular signaling dose relationships within the body. Dose response can be related to the Hill equation, which is closer to a power law. Public finance There is a new branch of the literature on public finance hypothesizing that the Weber–Fechner law can explain the increasing levels of public expenditures in mature democracies. Election after election, voters demand more public goods to be effectively impressed; therefore, politicians try to increase the magnitude of this "signal" of competence – the size and composition of public expenditures – in order to collect more votes. Communication An analysis of the length of comments in internet discussion boards across several languages shows that comment lengths obey the lognormal distribution with great precision. The authors explain the distribution as a manifestation of the Weber–Fechner law. == See also ==
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