Presentation on theme: "Chapter 6. Light Source and Detectors"— Presentation transcript:
1 Chapter 6. Light Source and Detectors Quantum- element units of energyQuantum optics: photoelectric effectlaser emissionblackbody radiation
2 6.1 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 light--the consequence of the temperature (a) Thermal source: sun, wax candle, kerosene lanterns, electric light bulblight--the consequence of the temperaturekerosene lanterns: carbon freed by the combustion processelectric light bulbs: a filament is heated. carbon filaments, metal filamentsIncandescent lamps: be heated to incandescence Refractory metals: a high melting point Tungsten: 3410C ; evaporates, Some halogens( iodine), retard the process
7 (a) Black body : is an ideal absorber, also a perfect emitter 6.1 Light Sources2. Blackbody Radiators(a) Black body : is an ideal absorber, also a perfect emitterA good way of making a blackbody is to force reflected light to make lots of reflections: inside a bottle with a small openingThe spectral distribution of that radiation is a function of temperature alone; the material as such plays no role
9 Quantization of Energy Max Planck ( )Solved the “ultravioletcatastrophe”Planck’s hypothesis: An object can only gain or lose energy by absorbing or emitting radiant energy in QUANTA.
10 Electromagnetic Radiation All waves have: frequency and wavelengthsymbol: n (Greek letter “nu”) l (Greek “lambda”)units: “cycles per sec” = Hertz “distance” (nm)Note: Long wavelength small frequencyShort wavelength high frequencyincreasingwavelengthfrequency
11 E = h • n Energy of radiation is proportional to frequency. where h = Planck’s constant = x J•sLight with large l (small n) has a small E.Light with a short l (large n) has a large E.(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) Plank’s radiation law
14 3. Wien's Displacement Law 6.1 Light Sources3. Wien's Displacement Lawplot Planck's law for different temperaturesincreasing temperaturemore energy is emittedthe peak emission shifts toward the shorter wavelengthsThe temperature and the wavelength of maximum intensity satisfy Tmax=constant
15 Black-Body Radiation Hole in a cavity is Called a Black Body a perfect absorbera perfect emitterCalled a Black BodyWien’s law
16 Example - Wien’s LawWhat is the peak radiation emitted by an object at 100oC ?This is in the far infrared.What T required for middle of visible range?
17 Blackbody Radiation: Experimental Results At 310 Kelvin (=37oC = 98.6oF), only get IRIntensityblue yellow redIRUVwavelength
18 Blackbody Radiation:Experimental Results At much higher temperatures, get visiblelook at blue/red ratio to get temperatureIntensityblue yellow redIRUVwavelength
19 Temperature of the SunWhen we look at the visible spectra of the sun, we see that it’s intensity peaks at about 500 nm (green light). From the equation: = b/T (where b = 2.9 x 10-3m*K)we get: T = b/ = (2.9 x 10-3m*K) / 500 x 10-9m 6000 K .
20 4. Stefan-Boltzmann's Law 6.1 Light Sources4. Stefan-Boltzmann's LawThe total energy density inside a blackbody cavity is given by integration over all wavelengthsNote that Intensity increases with TTemperature 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 = 0oC (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 wavelengthStefan-Boltzmann's law for gray bodiesfactor : the emissivity of the surfaceRecall 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 ExampleIf you eat 2,000 calories per day, that is equivalent to about 100 joules per second or about 100 Watts - which must be emitted.Let’s see how much radiation you emit when the temperature is comfortable, say 75oF=24oC=297K, and pick a surface area, say 1.5m2, that is at a temperature of 93oF=34oC=307K:Memitted = AT4 =(5.67x10-8W/m2K4)*(.97)*(1.5m2)*(307K)4 = 733 Watts emitted!
23 Example continuedBut this is not the whole story: besides emitting radiation, we receive radiation from the outside: Mabsorbed = AT4 =(5.67x10-8W/m2K4)*(.97)*(1.5m2)*(297K)4 = 642 Watts absorbed!Hence, the net power emitted by the body via radiation is: Mnet = 733 Watts Watts = 91 Watts. The peak of this radiation is at:peak = b/T = 2.9x10-3m*K / 307K = 9.5m 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 effectQuantum detectors are of particular interest, both theoretical and practical; some of them are so sensitive they respond to individual quanta.
25 1. Thermal Detectors 6.2 Detectors slow to respond 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 DetectorsThermocouplea 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.thermopilecontains several thermocouples and, therefore, is more sensitive.
27 6.2 Detectorsbolometercontains 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.
28 the wavelength of the light plays an important role 6.2 Detectors2. Quantum Detectorsthe wavelength of the light plays an important rolethere is a certain threshold above which there is no effect at all, no matter what the intensityintense light and dim light cause same of an effect
29 Photoelectric Effect Albert Einstein (1879-1955) Photoelectric effect demonstrates theparticle nature of lightNo e- observed until lightof a certain minimum E is used.Number of e- ejected does NOTdepend on frequency, rather itdepends on light intensity.
32 Photoelectric Effect (2) Classical theory said that E of ejectedelectron should increase with increasein light intensity — not observed!Experimental observations can be explained if light consists of particles called PHOTONS of discrete energy.
34 plate M(photocathode) 6.2 DetectorsVALighte-Variable powersupplyplate 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.
35 6.2 Detectorsif 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, V0.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 The electron photo-current can be stopped by a retarding potential. Increasing the light intensity do not change the retarding potential.
38 6.2 DetectorsIf 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 10-8 s, between the receipt of the irradiation and the resulting current.
39 Einstein's photoelectric-effect equation. 6.2 DetectorsThe 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, isKEmax = h - WEinstein's photoelectric-effect equation.
40 h = W + KEKE = h - WEinstein suggested that the linear behaviour is simply a Conservation of Energy.Energy of Light =Energy needed to get out +Kinetic Energy of electron.
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 DetectorsIt 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 106 /s = 6.63 x J = 4 x eVred photon: f = c/3 × 108 m/s / 7 x 10-7 m = 4.3 x 1014 Hz, red photon energy = eVblue: = 400 nm; photon energy = eV .
44 Photoelectric Properties Of Some Alkali Metals 6.2 DetectorsThe 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 MetalsAlkali Work function (eV) Threshold (nm)SodiumPotassiumRubidiumCesium
45 The Photoelectric Effect on Potassium Determine the work function WKE=(hc)(1/) － W
46 From the graph:The plot is essentially KE vs 1/, so that sinceKE=hc/－WThe intercept when (1/)=0 giveW=－KE=－(－2eV)=2eVTo obtain Planck’s constant h, we need the slope SThen h=S/c.S=(4－(－2))/(5－0) × 10-3=1.2 * 103 eV nmh = 1.2 × 103 × × 10-19×10-9 /(3 × 108) 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 - + e- hv 6.3 Practical Quantum Detectors The simplest type is probably the vacuum phototube, an example of a photoemissive detector.Light strikes photocathode (-)Photocathode emits photoelectronsPhotoelectrons accelerate toward anode (+)flow of electrons = currentcurrent 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 photoelectronsPhotoelectrons 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 photo-voltaic detectors: 6.3 Practical Quantum Detectorsphoto-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 image tube:not only detects light but also preserves the spatial characteristics of an image. 6.3 Practical Quantum Detectorscontain 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 converterthe image is formed in the IR, the UV or the X-ray range and converted into the visiblemicrochannel image intensifierthe system is built around an array of many short fibers or capillaries, fused into a wafer.