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Chapter 6. Light Source and Detectors Quantum- element units of energy Quantum optics: photoelectric effect laser emission blackbody radiation.

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Presentation on theme: "Chapter 6. Light Source and Detectors Quantum- element units of energy Quantum optics: photoelectric effect laser emission blackbody radiation."— Presentation transcript:

1 Chapter 6. Light Source and Detectors Quantum- element units of energy Quantum optics: photoelectric effect laser emission blackbody radiation

2 6.1 Light Sources 1. Light Sources An object is a source of light. A direct source produces light, e.g. the sun, light bulb, fire. An indirect source does not produce light, e.g. an illuminated object. An extended object may be regarded as a set of point sources.

3 ( a) Thermal source: sun, wax candle, kerosene lanterns, electric light bulb light--the consequence of the temperature kerosene lanterns: carbon freed by the combustion process electric light bulbs: a filament is heated. carbon filaments, metal filaments Incandescent lamps: be heated to incandescence Refractory metals: a high melting point Tungsten: 3410 C ; evaporates, Some halogens( iodine), retard the process

4 How tungsten filaments works

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6 (b) Fluorescent lamps Fluorescent lamps High-pressure mercury lamps High-pressure xenon lamps (c) Stimulated emission: laser, LED

7 2. Blackbody Radiators (a) Black body (a) Black body : is an ideal absorber, also a perfect emitter A good way of making a blackbody is to force reflected light to make lots of reflections: inside a bottle with a small opening 6.1 Light Sources The spectral distribution of that radiation is a function of temperature alone; the material as such plays no role

8 Classical theory failed Ultraviolet catastrophe

9 Quantization of Energy Planck s hypothesis: An object can only gain or lose energy by absorbing or emitting radiant energy in QUANTA. Max Planck ( ) Solved the ultraviolet catastrophe

10 All waves have: frequency and wavelength symbol: Greek letter nu ) Greek lambda ) units: cycles per sec = Hertz distance (nm) Electromagnetic Radiation Note: Long wavelength small frequency Short wavelength high frequency increasing wavelength increasing frequency

11 E = h Energy of radiation is proportional to frequency. where h = Plancks constant = x Js Light with large (small ) has a small E. Light with a short (large ) has a large E. (b) Photon: (b) Photon: the oscillators emit energy, as discrete, elemental units of energy called quanta or photons

12 Photons Light also behaves as a stream of particles, called photons. Light has wave-particle duality, meaning that it behaves as waves and as particles. This is a concept in quantum mechanics.

13 (c) Black-body radiation is electromagnetic radiation that is in thermal equilibrium at a temperature T with matter that can absorb and emit without favouring any particular wavelength d)Planks radiation law (d) Planks radiation law

14 3. Wien's Displacement Law 6.1 Light Sources plot Planck's law for different temperatures increasing temperature more energy is emitted the peak emission shifts toward the shorter wavelengths The temperature and the wavelength of maximum intensity satisfy T max =constant

15 Black-Body Radiation Hole in a cavity is a perfect absorber a perfect emitter Called a Black Body Wiens law

16 Example - Wiens Law What is the peak radiation emitted by an object at 100 o C ? This is in the far infrared. What T required for middle of visible range?

17 Blackbody Radiation: Experimental Results At 310 Kelvin (=37 o C = 98.6 o F), only get IR Intensity wavelength UV IRblue yellow red

18 Blackbody Radiation:Experimental Results At much higher temperatures, get visible look at blue/red ratio to get temperature Intensity wavelength UV IRblue yellow red

19 Temperature of the Sun When we look at the visible spectra of the sun, we see that its intensity peaks at about 500 nm (green light). From the equation: = b/T (where b = 2.9 x m*K) we get: T = b/ = (2.9 x m*K) / 500 x m 6000 K.

20 4. Stefan-Boltzmann's Law 6.1 Light Sources The total energy density inside a blackbody cavity is given by integration over all wavelengths Note that Intensity increases with T Temperature must be in Kelvin, where size of one Kelvin is same as size of one degree Celsius, but T=0K is absolute zero, and T=273K = 0 o C (freezing).

21 5. Klrchhoff's Law 6.1 Light Sources Kirchhoff's law :an object that is a good radiator at a given wavelength is also a good absorber at the same wavelength Stefan-Boltzmann's law for gray bodies factor : the emissivity of the surface Recall that a good absorber is also a good emitter, and a poor absorber is a poor emitter. We use the symbol to indicate the blackness ( =0) or the whiteness ( =1) of an object.

22 Example If you eat 2,000 calories per day, that is equivalent to about 100 joules per second or about 100 Watts - which must be emitted. Lets see how much radiation you emit when the temperature is comfortable, say 75 o F=24 o C=297K, and pick a surface area, say 1.5m 2, that is at a temperature of 93 o F=34 o C=307K: M emitted = AT 4 = (5.67x10 -8 W/m 2 K 4 )*(.97)*(1.5m 2 )*(307K) 4 = 733 Watts emitted!

23 Example continued But this is not the whole story: besides emitting radiation, we receive radiation from the outside: M absorbed = AT 4 = (5.67x10 -8 W/m 2 K 4 )*(.97)*(1.5m 2 )*(297K) 4 = 642 Watts absorbed! Hence, the net power emitted by the body via radiation is: M net = 733 Watts Watts = 91 Watts. The peak of this radiation is at: peak = b/T = 2.9x10 -3 m*K / 307K = 9.5 m which is in the infrared (as expected).

24 6.2 Detectors thermal detectors based on absorption and heating If the absorbing material is black, they are independent of wavelength. quantum detectors. based on photoelectric effect Quantum detectors are of particular interest, both theoretical and practical; some of them are so sensitive they respond to individual quanta.

25 6.2 Detectors 1. Thermal Detectors slow to respond Golay cell Golay cell a thin black membrane placed over a small, gas-filled chamber. Heat absorbed by the membrane causes the gas to expand, which in turn can be measured, either optically (by a movable mirror) or electrically (by a change in capacitance). used in the infrared.

26 6.2 Detectors Thermocouple Thermocouple a junction between two dissimilar metals. As the junction is heated, the potential difference changes. In practice, two junctions are used in series, a hot junction exposed to the radiation, and a cold junction shielded from it. The two voltages are opposite to each other; thus the detector, which without this precaution would show the absolute temperature, now measures the temperature differential. a junction between two dissimilar metals. As the junction is heated, the potential difference changes. In practice, two junctions are used in series, a hot junction exposed to the radiation, and a cold junction shielded from it. The two voltages are opposite to each other; thus the detector, which without this precaution would show the absolute temperature, now measures the temperature differential. thermopile thermopile contains several thermocouples and, therefore, is more sensitive. contains several thermocouples and, therefore, is more sensitive.

27 6.2 Detectors bolometer bolometer contains a metal element whose electrical resistance changes as a function of temperature; if instead of the metal a semiconductor is used, it is called a thermistor. contains a metal element whose electrical resistance changes as a function of temperature; if instead of the metal a semiconductor is used, it is called a thermistor. Unlike a thermocouple, a bolometer or thermistor does not generate a voltage; they must be connected to a voltage source. Unlike a thermocouple, a bolometer or thermistor does not generate a voltage; they must be connected to a voltage source.

28 6.2 Detectors 2. Quantum Detectors the wavelength of the light plays an important role there is a certain threshold above which there is no effect at all, no matter what the intensity intense light and dim light cause same of an effect

29 Photoelectric effect demonstrates the particle nature of light Number of e - ejected does NOT depend on frequency, rather it depends on light intensity. No e - observed until light of a certain minimum E is used. Photoelectric Effect Albert Einstein ( )

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32 Photoelectric Effect (2) Experimental observations can be explained if light consists of particles called PHOTONS of discrete energy. Classical theory said that E of ejected electron should increase with increase in light intensity not observed!

33 Discrete Packets of Energy

34 6.2 Detectors plate M(photocathode) when irradiated, releases electrons (called photoelectrons) collector plate C(anode) photoelectrons released by M are attracted by, and travel to C. As the potential V, read on an high-impedance voltmeter, is increased, the current, I, read on an ammeter, increases too, but only up to a given saturation level, because then all of the electrons emitted by M are collected by C. V A Light e- Variable power supply

35 6.2 Detectors if C is made negative, some photocurrent will still exist, provided the electrons ejected from M have enough kinetic energy to overcome the repulsive field at C. But as C is made more negative, a point is reached where no electrons reach C and the current drops to zero. This occurs at the stopping potential, V 0. In short: A significant amount of photocurrent is present only if the collector, C, is made positive

36 When the frequency of the light is increased, the stopping potential also increases.

37 The electron photo-current can be stopped by a retarding potential. Increasing the light intensity do not change the retarding potential.

38 6.2 Detectors If more intense light falls on the photocathode, it will release more electrons but their energies, and their velocities, will remain the same. The energy of the photoelectrons depends on the frequency of the light: blue light produces more energetic photo-electrons than red light. The response of a quantum detector is all but instantaneous: there is no time lag, at least not more than s, between the receipt of the irradiation and the resulting current.

39 The light is received in the form of discrete quanta. Part of the energy contained in a quantum is needed to make the electron escape from the surface; that part is called the work function, W. Only the excess energy, beyond the work function, appears as kinetic energy of the electron. The maximum kinetic energy with which the electron can escape, therefore, is KE max = h - W Einstein's photoelectric-effect equation. 6.2 Detectors

40 Einstein suggested that the linear behaviour is simply a Conservation of Energy. Energy of Light =Energy needed to get out +Kinetic Energy of electron. h = W + KE KE = h - W

41 Example - Photoelectric Effect Given that aluminum has a work function of 4.08 eV, what are the threshold frequency and the cutoff wavelength?

42 6.2 Detectors It is often convenient to measure energies on an atomic scale not in joule but in electron volt, eV. 1 eV = (1e)(1V) = J

43 Photons and Colors Electron volts are useful size units of energy 1 eV = 1.6 x Coul × 1V = 1.6 x J. radio photon: hf = 6.63 x Js × 1 x 10 6 /s = 6.63 x J = 4 x eV red photon: f = c/ 3 × 10 8 m/s / 7 x m = 4.3 x Hz, red photon energy = 1.78 eV blue: = 400 nm; photon energy = 3.11 eV.

44 6.2 Detectors The work function determines the longest wavelength to which a detector can respond: the lower the work function, the longer the wavelength. The lowest work functions are found among the alkali metals. Photoelectric Properties Of Some Alkali Metals Alkali Work function (eV) Threshold (nm) Sodium Potassium Rubidium Cesium

45 The Photoelectric Effect on Potassium Determine the work function W KE=(hc)(1/ ) W

46 From the graph: The plot is essentially KE vs 1/, so that since KE=hc/ W The intercept when (1/ )=0 give W= KE= ( 2eV)=2eV To obtain Plancks constant h, we need the slope S Then h=S/c. S=(4 ( 2))/(5 0) × =1.2 * 10 3 eV nm h = 1.2 × 10 3 × × ×10 -9 /(3 × 10 8 ) J s = 6.4× J s cf (6.626 × J s)

47 6-3. Practical Quantum Detectors In contrast to thermal detectors, quantum detectors respond to the number of quanta, rather than to the energy contained in them.

48 The simplest type is probably the vacuum phototube, an example of a photoemissive detector. 6.3 Practical Quantum Detectors e-e-e-e- hv Light strikes photocathode (-) Photocathode emits photoelectrons Photoelectrons accelerate toward anode (+) flow of electrons = current current proportional to # photons incident on photocathode

49 quantum efficiency:the ratio of the number of photoelectrons released to the number of photons received. Ordinarily, this efficiency is no higher than a few percent. Several diodes are combined in series to form a photomultiplier, the efficiency becomes much higher. Light strikes photocathode (-) Photocathode emits photoelectrons Photoelectrons accelerate toward series of increasingly positive anodes (+) at which photoelectrons and secondary electrons are emitted (dynodes) Electrons accelerated toward collection anode

50 6.3 Practical Quantum Detectors A photocell is the solid-state equivalent of the vacuum photodiode; most often it is a semiconductor. A semiconductor conducts electricity better than an insulator but not as well as a conductor. In an insulator, the electrons are tightly bound to their respective atoms. In a metal, the electrons can move freely; hence, even a small voltage applied to the conductor will cause a current.

51 6.3 Practical Quantum Detectors photoconductive detectors : semiconductor, such as cadmium sulfide (CdS), gallium arsenide, and silicon, conduct electricity poorly only in the dark; when exposed to light, they conduct very well.

52 6.3 Practical Quantum Detectors photo-voltaic detectors: made from two semiconductors, one of them transparent to light, for instance a layer of CdS deposited on selenium. When light is incident on the junction, the electrons start moving, but only in one direction producing a current; in other words, the junction converts light energy into electrical energy. used as solar cells and as exposure meters in photographic cameras.

53 6.3 Practical Quantum Detectors image tube:not only detects light but also preserves the spatial characteristics of an image. contain an array of photoconductors, one for each pixel. When exposed to light, the elements from a latent image that can be read by an electron beam scanning across them. the photoelectrons emitted by the cathode can be focused by an electron lens and made visible on a phosphor screen mounted in the same tube.

54 6.3 Practical Quantum Detectors image intensifier: the image is merely amplified. image converter the image is formed in the IR, the UV or the X-ray range and converted into the visible microchannel image intensifier the system is built around an array of many short fibers or capillaries, fused into a wafer.


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