Friday 30 September 2011

LANGRANGE'S MEAN VALUE THEOREM


Proof of the Mean Value Theorem  (L.M.V.T)


Assume Rolle's theorem. The equation of the secant -- a straight line -- through points (a, f(a)) and (b, f(b)) is given by

g(x) = f(a) + [(f(b) - f(a)) / (b - a)](x - a).

The line is straight and, by inspection, g(a) = f(a) and g(b) = f(b). Because of this, the difference f - g satisfies the conditions of Rolle's theorem:

(f - g)(a) = f(a) - g(a) = 0 = f(b) - g(b) = (f - g)(b).

We are therefore guaranteed the existence of a point c in (a, b) such that (f - g)'(c) = 0. But

(f - g)'(x) = f '(x) - g'(x) = f '(x) - (f(b) - f(a)) / (b - a).

(f - g)'(c) = 0 is then the same as

f'(c) = (f(b) - f(a)) / (b - a).

ROLL'S THEOREM

syllabus basic electronics 1st semester


LEC. NO.                                                                                                                                           TOPICS TO BE COVERED 
1     INTRODUCTION TO P-N JUNCTION
2    V-I CHARACTERISTICS
3   DIODE EQUATION
4 TUTORIAL
5  CLIPPERS: SERIES, SHUNT, SINGLE & DOUBLE SIDE CLIPPERS 
6 CLAMPERS: POSITIVE & NEGATIVE CLAMPERS, ZENER DIODE: V-I CHARACTERISTICS
7 ZENER REGULATORS, LED
8 TUTORIAL
9 BJT: CHARACTERISTICS, CE & CB CONFIGURATION. RELATION B/W ANGLES
10 Q- POINT, TRANSISTOR BIASING, FIXED BIAS & SELF BIAS
11 H- PARAMETERS. TRNSISTOR AS AN AMPLIFIER, FREQUENCY RESPONSE
12 TUTORIAL
13 OPERATIONAL AMPLIFIER, BASIC MODEL, INVERTING AMPLIFIER
14 NON-INVERTING AMPLIFIER, INTEGRATOR, DIFFERENTIATOR
15 SUMMING AMPLIFIER, COMPARATOR
16 TUTORIAL
17 INTRODUCTION TO NUMBER SYSTEMS
18 INTRODUCTION TO NUMBER SYSTEMS
19 CODE CONVERSIONS
20 TUTORIAL
21 DIGITAL ARITHMETIC
22 BOOLEAN ALGEBRA
23 BOOLEAN ALGEBRA
24 TUTORIAL
25 LOGIC GATES: OR, NOT , AND, NOR & NAND; UNIVERSAL GATES, XOR &XNOR GATE; TRUTH TABLES
26 LOGIC FUNCTION REPRESENTATION COMBINATIONAL CIRCUITS
27 DESIGNING COMBINATIONAL CIRCUITS: SOP , POS FORM
28 TUTORIAL
29 K-MAP , FLIP- FLOPS
30 SR, JK & D FLIP- FLOPS
31 RIPPLE COUNTERS: CONFIGURATION, OPERATION;
32 TUTORIAL
33 UP/ DOWN COUNTERS ; SHIFT REGISTERS
34 MULTI VIBRATOR
35 D/A CONVERTOR A/D CONVERTOR
36 TUTORIAL
37 INTRODUCTION TO COMMUNICATION, FREQUENCY BANDS, NOISE
38 TRANSMISSION MEDIA: WIRE MEDIA, TWO WIRE, CO-AXIL CABLE,
39 OPTICAL FIBER, COMPARISON. WIRELESS COMMUNICATION
40 TUTORIAL
41 ANALOG MODULATION, AM BLOCK DIAGRAM , MODULATION EQUATION, WAVEFORMS
42 AM DETECTOR, DEFINITION & APPLICATIONS OF SSB  , DSB , VSB
43 FM BLOCK DIAGRAM, MODULATION EQUATIONS  
44 TUTORIAL
45 FDM
46 TDM
47 COMPARISON OF AM & FM
48 TUTORIAL

ABOUT CARBON NOT SHOWING SEMICUNDUCTANCE PROPERTY


              ABOUT CARBON NOT SHOWING SEMICUNDUCTANCE PROPERTY.
--- carbon can conduct electricity, but carbon does not have resistivity and                                                      much of electrical energy will be lost as heat energy when it passes through carbon and it forms diamond crystal structures so when we add impurity atom it will not  make any significant change. . . . .
---à carbon is not used as semiconductor it has 4 valence electron in its valence shell but the energy gap is very small it will conduct electricity even at room temperature , the size of carbon is very small. Whether in case of germanium and silicon it has d orbital which shows mobility.
---àor its allotropic form like graphite and carbon doesn’t allow the addition of electron , because carbon is already stable hence its stability doesn’t allow conductivity.

intereference

Interference (wave propagation)


Two point interference in a ripple tank.
In physics, interference is the phenomenon in which two waves superpose each other to form a resultant wave of greater or lower amplitude. Interference usually refers to the interaction of waves that are correlated or coherent with each other, either because they come from the same source or because they have the same or nearly the same frequency.
The term interference has a different meaning in radio communications.

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Interference

Animation: interference of waves from 2 point sources. Crests blue, troughs red/yellow.
For two coherent sources, the spatial separation between sources is half the wavelength times the number of nodal lines. The principle of superposition of waves states that the resultant displacement at a point is equal to the vector sum of the displacements of different waves at that point. If a crest of a wave meets a crest of another wave at the same point then the crests interfere constructively and the resultant crest wave amplitude is increased; similarly troughs make a trough of increased amplitude. If a crest of a wave meets a trough of another wave then they interfere destructively, and the overall amplitude is decreased.
This form of interference can occur whenever a wave can propagate from a source to a destination by two or more paths of different lengths. Two or more sources can only be used to produce interference when there is a fixed phase relation between them, but in this case the interference generated is the same as with a single source; see Huygens' principle.
Interference of two circular waves. Absolute value snapshots of the (real-valued, scalar) wave field. Wavelength increasing from top to bottom, distance between wave centers increasing from left to right. The dark regions indicate destructive interference.
The colors seen in a soap bubble or an oil film on water are a common example of interference. Light reflecting off the front and back surfaces of the thin soap film interferes, resulting in different colors being enhanced.
Light from any source can be used to obtain interference patterns, for example, Newton's rings can be produced with sunlight and the colours which can be seen when sunlight is reflected in a soap-bubble are white light fringes.

Constructive and destructive interference

Consider two waves that are in phase, sharing the same frequency and with amplitudes A1 and A2. Their troughs and peaks line up and the resultant wave will have amplitude A = A1 + A2. This is known as constructive interference.
If the two waves are π radians, or 180°, out of phase, then one wave's crests will coincide with another waves' troughs and so will tend to cancel itself out. The resultant amplitude is A = |A1A2|. If A1 = A2, the resultant amplitude will be zero. This is known as destructive interference.
When two sinusoidal waves superimpose, the resulting waveform depends on the frequency (or wavelength) amplitude and relative phase of the two waves. If the two waves have the same amplitude A and wavelength the resultant waveform will have an amplitude between 0 and 2A depending on whether the two waves are in phase or out of phase.
combined
waveform
Interference of two waves.svg
wave 1
wave 2

Two sinusoidal waves in phaseTwo sinusoidal waves 180° out
of phase

Examples

A conceptually simple case of interference is a small (compared to wavelength) source – say, a small array of regularly spaced small sources (see diffraction grating).
Consider the case of a flat boundary (say, between two media with different densities or simply a flat mirror), onto which the plane wave is incident at some angle. In this case of continuous distribution of sources, constructive interference will only be in specular direction – the direction at which angle with the normal is exactly the same as the angle of incidence. Thus, this results in the law of reflection which is simply the result of constructive interference of a plane wave on a plane surface.

Optical interferometry

Interference pattern produced with a Michelson interferometer.
Optical interferometry had played a major role in the advancement of physics, e.g. Young's slits interferometer and the Michelson-Morley experiment. It is also widely used in a range of physical and engineering measurement applications.

coherence

In physics, coherence is a property of waves that enables stationary (i.e. temporally and spatially constant) interference. More generally, coherence describes all properties of the correlation between physical quantities of a wave.
When interfering, two waves can add together to create a larger wave (constructive interference) or subtract from each other to create a smaller wave (destructive interference), depending on their relative phase. Two waves are said to be coherent if they have a constant relative phase. The degree of coherence is measured by the interference visibility, a measure of how perfectly the waves can cancel due to destructive interference.

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[edit]Introduction

Coherence was originally introduced in connection with Thomas Young's double-slit experiment in optics but is now used in any field that involves waves, such as acoustics, electrical engineering, neuroscience, and quantum mechanics. The property of coherence is the basis for commercial applications such as holography, the Sagnacgyroscope, radio antenna arrays, optical coherence tomography and telescope interferometers (astronomical optical interferometers and radio telescopes).

[edit]Coherence and correlation

The coherence of two waves follows from how well correlated the waves are as quantified by the cross-correlation function.[1][2][3][4][5] The cross-correlation quantifies the ability to predict the value of the second wave by knowing the value of the first. As an example, consider two waves perfectly correlated for all times. At any time, if the first wave changes, the second will change in the same way. If combined they can exhibit complete constructive interference/superposition at all times, then it follows that they are perfectly coherent. As will be discussed below, the second wave need not be a separate entity. It could be the first wave at a different time or position. In this case, the measure of correlation is the autocorrelation function (sometimes called self-coherence). Degree of correlation involves correlation functions.

[edit]Examples of wave-like states

These states are unified by the fact that their behavior is described by a wave equation or some generalization thereof.
In most of these systems, one can measure the wave directly. Consequently, its correlation with another wave can simply be calculated. However, in optics one cannot measure the electric field directly as it oscillates much faster than any detector’s time resolution.[6] Instead, we measure the intensity of the light. Most of the concepts involving coherence which will be introduced below were developed in the field of optics and then used in other fields. Therefore, many of the standard measurements of coherence are indirect measurements, even in fields where the wave can be measured directly.

[edit]Temporal coherence

Figure 1: The amplitude of a single frequency wave as a function of time t (red) and a copy of the same wave delayed by τ(green). The coherence time of the wave is infinite since it is perfectly correlated with itself for all delays τ.
Figure 2: The amplitude of a wave whose phase drifts significantly in time τc as a function of time t (red) and a copy of the same wave delayed by 2τc(green). At any particular time t the wave can interfere perfectly with its delayed copy. But, since half the time the red and green waves are in phase and half the time out of phase, when averaged over t any interference disappears at this delay.
Temporal coherence is the measure of the average correlation between the value of a wave and itself delayed by τ, at any pair of times. Temporal coherence tells us how monochromatic a source is. In other words, it characterizes how well a wave can interfere with itself at a different time. The delay over which the phase or amplitude wanders by a significant amount (and hence the correlation decreases by significant amount) is defined as the coherence timeτc. At τ=0 the degree of coherence is perfect whereas it drops significantly by delay τc. The coherence lengthLc is defined as the distance the wave travels in time τc.
One should be careful not to confuse the coherence time with the time duration of the signal, nor the coherence length with the coherence area (see below).

[edit]The relationship between coherence time and bandwidth

It can be shown that the faster a wave decorrelates (and hence the smaller τc is) the larger the range of frequencies Δf the wave contains. Thus there is a tradeoff:
\tau_c \Delta f \approx 1.
Formally, this follows from the convolution theorem in mathematics, which relates the Fourier transform of the power spectrum (the intensity of each frequency) to its autocorrelation.

[edit]Examples of temporal coherence

We consider four examples of temporal coherence.
  • A wave containing only a single frequency (monochromatic) is perfectly correlated at all times according to the above relation. (See Figure 1)
  • Conversely, a wave whose phase drifts quickly will have a short coherence time. (See Figure 2)
  • Similarly, pulses (wave packets) of waves, which naturally have a broad range of frequencies, also have a short coherence time since the amplitude of the wave changes quickly. (See Figure 3)
  • Finally, white light, which has a very broad range of frequencies, is a wave which varies quickly in both amplitude and phase. Since it consequently has a very short coherence time (just 10 periods or so), it is often called incoherent.
The most monochromatic sources are usually lasers; such high monochromaticity implies long coherence lengths (up to hundreds of meters). For example, a stabilized helium-neon laser can produce light with coherence lengths in excess of 5 m. Not all lasers are monochromatic, however (e.g. for a mode-locked Ti-sapphire laser, Δλ ≈ 2 nm - 70 nm). LEDs are characterized by Δλ ≈ 50 nm, and tungsten filament lights exhibit Δλ ≈ 600 nm, so these sources have shorter coherence times than the most monochromatic lasers.
Holography requires light with a long coherence time. In contrast, Optical coherence tomography uses light with a short coherence time.

[edit]Measurement of temporal coherence

Figure 3: The amplitude of a wavepacket whose amplitude changes significantly in time τc (red) and a copy of the same wave delayed by 2τc(green) plotted as a function of time t. At any particular time the red and green waves are uncorrelated; one oscillates while the other is constant and so there will be no interference at this delay. Another way of looking at this is the wavepackets are not overlapped in time and so at any particular time there is only one nonzero field so no interference can occur.
Figure 4: The time-averaged intensity (blue) detected at the output of an interferometer plotted as a function of delay τ for the example waves in Figures 2 and 3. As the delay is changed by half a period, the interference switches between constructive and destructive. The black lines indicate the interference envelope, which gives the degree of coherence. Although the waves in Figures 2 and 3 have different time durations, they have the same coherence time.
In optics, temporal coherence is measured in an interferometer such as the Michelson interferometer or Mach–Zehnder interferometer. In these devices, a wave is combined with a copy of itself that is delayed by time τ. A detector measures the time-averaged intensity of the light exiting the interferometer. The resulting interference visibility (e.g. see Figure 4) gives the temporal coherence at delay τ. Since for most natural light sources, the coherence time is much shorter than the time resolution of any detector, the detector itself does the time averaging. Consider the example shown in Figure 3. At a fixed delay, here 2τc, an infinitely fast detector would measure an intensity that fluctuates significantly over a time t equal to τc. In this case, to find the temporal coherence at 2τc, one would manually time-average the intensity.

[edit]Spatial coherence

In some systems, such as water waves or optics, wave-like states can extend over one or two dimensions. Spatial coherence describes the ability for two points in space, x1 and x2, in the extent of a wave to interfere, when averaged over time. More precisely, the spatial coherence is the cross-correlation between two points in a wave for all times. If a wave has only 1 value of amplitude over an infinite length, it is perfectly spatially coherent. The range of separation between the two points over which there is significant interference is called the coherence area, Ac. This is the relevant type of coherence for the Young’s double-slit interferometer. It is also used in optical imaging systems and particularly in various types of astronomy telescopes. Sometimes people also use “spatial coherence” to refer to the visibility when a wave-like state is combined with a spatially shifted copy of itself.

[edit]Examples of spatial coherence

Consider a tungsten light-bulb filament. Different points in the filament emit light independently and have no fixed phase-relationship. In detail, at any point in time the profile of the emitted light is going to be distorted. The profile will change randomly over the coherence time τc. Since for a white-light source such as a light-bulb τc is small, the filament is considered a spatially incoherent source. In contrast, a radio antenna array, has large spatial coherence because antennas at opposite ends of the array emit with a fixed phase-relationship. Light waves produced by a laser often have high temporal and spatial coherence (though the degree of coherence depends strongly on the exact properties of the laser). Spatial coherence of laser beams also manifests itself as speckle patterns and diffraction fringes seen at the edges of shadow.
Holography requires temporally and spatially coherent light. Its inventor, Dennis Gabor, produced successful holograms more than ten years before lasers were invented. To produce coherent light he passed the monochromatic light from an emission line of a mercury-vapor lamp through a pinhole spatial filter.
In February 2011, Dr Andrew Truscott, leader of a research team at the ARC Centre of Excellence for Quantum-Atom Optics at Australian National University in Canberra, Australian Capital Territory, showed that helium atoms cooled to near absolute zero / Bose-Einstein condensate state, can be made to flow and behave as a coherent beam as occurs in a laser.[7][8]

[edit]Spectral coherence

Figure 10: Waves of different frequencies (i.e. colors) interfere to form a pulse if they are coherent.
Figure 11: Spectrally incoherent light interferes to form continuous light with a randomly varying phase and amplitude
Waves of different frequencies (in light these are different colours) can interfere to form a pulse if they have a fixed relative phase-relationship (see Fourier transform). Conversely, if waves of different frequencies are not coherent, then, when combined, they create a wave that is continuous in time (e.g. white light or white noise). The temporal duration of the pulse Δt is limited by the spectral bandwidth of the light Δf according to:
\Delta f\Delta t \ge 1,
which follows from the properties of the Fourier transform (for quantum particles it also results in the Heisenberg uncertainty principle).
If the phase depends linearly on the frequency (i.e. \theta (f) \propto f) then the pulse will have the minimum time duration for its bandwidth (a transform-limited pulse), otherwise it is chirped (see dispersion).

[edit]Measurement of spectral coherence

Measurement of the spectral coherence of light requires a nonlinear optical interferometer, such as an intensity optical correlator, frequency-resolved optical gating (FROG), or Spectral phase interferometry for direct electric-field reconstruction (SPIDER).

[edit]Polarization coherence

Light also has a polarization, which is the direction in which the electric field oscillates. Unpolarized light is composed of two equally intense incoherent light waves with orthogonal polarizations. The electric field of the unpolarized light wanders in every direction and changes in phase over the coherence time of the two light waves. A polarizer rotated to any angle will always transmit half the incident intensity when averaged over time.
If the electric field wanders by a smaller amount the light will be partially polarized so that at some angle, the polarizer will transmit more than half the intensity. If a wave is combined with an orthogonally polarized copy of itself delayed by less than the coherence time, partially polarized light is created.
The polarization of a light beam is represented by a vector in the Poincare sphere. For polarized light the end of the vector lies on the surface of the sphere, whereas the vector has zero length for unpolarized light. The vector for partially polarized light lies within the sphere

[edit]Applications

[edit]Holography

Coherent superpositions of optical wave fields include holography. Holographic objects are used frequently in daily life in bank notes and credit cards.