27.8 The Uncertainty Principle 891waves change in space and time. The Schrödinger wave equation represents a keyelement in the theory of quantum mechanics. It’s as important in quantum mechanicsas Newton’s laws in classical mechanics. Schrödinger’s equation has beensuccessfully applied to the hydrogen atom and to many other microscopic systems.Solving Schrödinger’s equation (beyond the level of this course) determines aquantity called the wave function. Each particle is represented by a wave function that depends both on position and on time. Once is found, 2 gives usinformation on the probability (per unit volume) of finding the particle in anygiven region. To understand this, we return to Young’s experiment involving coherentlight passing through a double slit.First, recall from Chapter 21 that the intensity of a light beam is proportional tothe square of the electric field strength E associated with the beam: I E 2 . Accordingto the wave model of light, there are certain points on the viewing screenwhere the net electric field is zero as a result of destructive interference of wavesfrom the two slits. Because E is zero at these points, the intensity is also zero, andthe screen is dark there. Likewise, at points on the screen at which constructiveinterference occurs, E is large, as is the intensity; hence, these locations are bright.Now consider the same experiment when light is viewed as having a particle nature.The number of photons reaching a point on the screen per second increasesas the intensity (brightness) increases. Consequently, the number of photons thatstrike a unit area on the screen each second is proportional to the square of theelectric field, or N E 2 . From a probabilistic point of view, a photon has a highprobability of striking the screen at a point at which the intensity (and E 2 ) is highand a low probability of striking the screen where the intensity is low.When describing particles rather than photons, rather than E plays the roleof the amplitude. Using an analogy with the description of light, we make the followinginterpretation of for particles: If is a wave function used to describe asingle particle, the value of 2 at some location at a given time is proportional tothe probability per unit volume of finding the particle at that location at that time.Adding up all the values of 2 in a given region gives the probability of finding theparticle in that region.AIP Emilio Segré Visual ArchivesERWIN SCHRÖDINGER, AustrianTheoretical Physicist (1887–1961)Schrödinger is best known as the creator ofwave mechanics, a less cumbersome theorythan the equivalent matrix mechanicsdeveloped by Werner Heisenberg. In 1933Schrödinger left Germany and eventuallysettled at the Dublin Institute of AdvancedStudy, where he spent 17 happy, creativeyears working on problems in general relativity,cosmology, and the application ofquantum physics to biology. In 1956, he returnedhome to Austria and his belovedTirolean mountains, where he died in 1961.27.8 THE UNCERTAINTY PRINCIPLEIf you were to measure the position and speed of a particle at any instant, you wouldalways be faced with experimental uncertainties in your measurements. According toclassical mechanics, no fundamental barrier to an ultimate refinement of the apparatusor experimental procedures exists. In other words, it’s possible, in principle, tomake such measurements with arbitrarily small uncertainty. <strong>Quantum</strong> theory predicts,however, that such a barrier does exist. In 1927, Werner Heisenberg (1901–1976) introducedthis notion, which is now known as the uncertainty principle:If a measurement of the position of a particle is made with precision x and asimultaneous measurement of linear momentum is made with precision p x ,then the product of the two uncertainties can never be smaller than h/4:x p x [27.16]In other words, it is physically impossible to measure simultaneously the exactposition and exact linear momentum of a particle. If x is very small, then p x islarge, and vice versa.To understand the physical origin of the uncertainty principle, consider the followingthought experiment introduced by Heisenberg. Suppose you wish to measurethe position and linear momentum of an electron as accurately as possible. Youmight be able to do this by viewing the electron with a powerful light microscope.For you to see the electron and determine its location, at least one photon of lightmust bounce off the electron, as shown in Figure 27.18a, and pass through theh4Courtesy of the University of HamburgWERNER HEISENBERG, GermanTheoretical Physicist (1901 – 1976)Heisenberg obtained his Ph.D. in 1923 at theUniversity of Munich, where he studied underArnold Sommerfeld. While physicists such asde Broglie and Schrödinger tried to developphysical models of the atom, Heisenbergdeveloped an abstract mathematical modelcalled matrix mechanics to explain the wavelengthsof spectral lines. Heisenberg mademany other significant contributions tophysics, including his famous uncertaintyprinciple, for which he received the NobelPrize in 1932; the prediction of two forms ofmolecular hydrogen; and theoretical modelsof the nucleus of an atom.
892 Chapter 27 <strong>Quantum</strong> <strong>Physics</strong>Figure 27.18 A thought experimentfor viewing an electron with apowerful microscope. (a) The electronis viewed before colliding with thephoton. (b) The electron recoils(is disturbed) as the result of thecollision with the photon.IncidentphotonBeforecollisionScatteredphotonAftercollisionElectronRecoilingelectron(a)(b)microscope into your eye, as shown in Figure 27.18b. When it strikes the electron,however, the photon transfers some unknown amount of its momentum to the electron.Thus, in the process of locating the electron very accurately (that is, by makingx very small), the light that enables you to succeed in your measurement changesthe electron’s momentum to some undeterminable extent (making p x very large).The incoming photon has momentum h/. As a result of the collision, the photontransfers part or all of its momentum along the x-axis to the electron. Therefore,the uncertainty in the electron’s momentum after the collision is as great asthe momentum of the incoming photon: p x h/. Further, because the photonalso has wave properties, we expect to be able to determine the electron’s positionto within one wavelength of the light being used to view it, so x . Multiplyingthese two uncertainties givesx p x hThe value h represents the minimum in the product of the uncertainties. Becausethe uncertainty can always be greater than this minimum, we havex p x hApart from the numerical factor 1/4 introduced by Heisenberg’s more preciseanalysis, this inequality agrees with Equation 27.16.Another form of the uncertainty relationship sets a limit on the accuracy withwhich the energy E of a system can be measured in a finite time interval t :E t h[27.17]It can be inferred from this relationship that the energy of a particle cannot bemeasured with complete precision in a very short interval of time. Thus, when anelectron is viewed as a particle, the uncertainty principle tells us that (a) its positionand velocity cannot both be known precisely at the same time and (b) itsenergy can be uncertain for a period given by t h/(4 E ).h4Applying <strong>Physics</strong> 27.4A common, but erroneous, description of the absolutezero of temperature is “that temperature at which allmolecular motion ceases.” How can the uncertaintyprinciple be used to argue against this description?Motion at Absolute ZeroExplanation Imagine a particular molecule in a piece ofmaterial. The molecule is confined within the material,so there is a fixed uncertainty x in its position alongone axis, corresponding to the size of that piece of material.If all molecular motion ceased at absolute zero, thegiven molecule’s velocity, in particular, would be exactlyzero, so its uncertainty in velocity would be v 0,meaning its uncertainty in momentum would also bezero, since p mv. The product of zero uncertainty inmomentum and a nonzero uncertainty in position iszero, violating the uncertainty principle. So according tothe uncertainty principle, there must be some molecularmotion even at absolute zero.
- Page 1 and 2: Color-enhanced scanning electronmic
- Page 3: 876 Chapter 27 Quantum PhysicsSolve
- Page 6 and 7: 27.2 The Photoelectric Effect and t
- Page 8 and 9: 27.3 X-Rays 881even when black card
- Page 10 and 11: 27.4 Diffraction of X-Rays by Cryst
- Page 12 and 13: 27.5 The Compton Effect 885Exercise
- Page 14 and 15: 27.6 The Dual Nature of Light and M
- Page 16 and 17: 27.6 The Dual Nature of Light and M
- Page 20 and 21: 27.8 The Uncertainty Principle 893E
- Page 22 and 23: 27.9 The Scanning Tunneling Microsc
- Page 24 and 25: Problems 897The probability per uni
- Page 26 and 27: Problems 89917. When light of wavel
- Page 28 and 29: Problems 90151.time of 5.00 ms. Fin
- Page 30 and 31: “Neon lights,” commonly used in
- Page 32 and 33: 28.2 Atomic Spectra 905l(nm) 400 50
- Page 34 and 35: 28.3 The Bohr Theory of Hydrogen 90
- Page 36 and 37: 28.3 Th Bohr Theory of Hydrogen 909
- Page 38 and 39: 28.4 Modification of the Bohr Theor
- Page 40 and 41: 28.6 Quantum Mechanics and the Hydr
- Page 42 and 43: 28.7 The Spin Magnetic Quantum Numb
- Page 44 and 45: 28.9 The Exclusion Principle and th
- Page 46 and 47: 28.9 The Exclusion Principle and th
- Page 48 and 49: 28.11 Atomic Transitions 921electro
- Page 50 and 51: 28.12 Lasers and Holography 923is u
- Page 52 and 53: 28.13 Energy Bands in Solids 925Ene
- Page 54 and 55: 28.13 Energy Bands in Solids 927Ene
- Page 56 and 57: 28.14 Semiconductor Devices 929I (m
- Page 58 and 59: Summary 931(a)Figure 28.32 (a) Jack
- Page 60 and 61: Problems 9335. Is it possible for a
- Page 62 and 63: Problems 935tum number n. (e) Shoul
- Page 64 and 65: Problems 93748. A dimensionless num
- Page 66 and 67: Aerial view of a nuclear power plan
- Page 68 and 69:
29.1 Some Properties of Nuclei 941T
- Page 70 and 71:
29.2 Binding Energy 943130120110100
- Page 72 and 73:
29.3 Radioactivity 94529.3 RADIOACT
- Page 74 and 75:
29.3 Radioactivity 947INTERACTIVE E
- Page 76 and 77:
29.4 The Decay Processes 949Alpha D
- Page 78 and 79:
29.4 The Decay Processes 951Strateg
- Page 80 and 81:
29.4 The Decay Processes 953they we
- Page 82 and 83:
29.6 Nuclear Reactions 955wounds on
- Page 84 and 85:
29.6 Nuclear Reactions 957EXAMPLE 2
- Page 86 and 87:
29.7 Medical Applications of Radiat
- Page 88 and 89:
29.7 Medical Applications of Radiat
- Page 90 and 91:
29.8 Radiation Detectors 963Figure
- Page 92 and 93:
Summary 965Photo Researchers, Inc./
- Page 94 and 95:
Problems 967CONCEPTUAL QUESTIONS1.
- Page 96 and 97:
Problems 96924. A building has beco
- Page 98 and 99:
Problems 97157. A by-product of som
- Page 100 and 101:
This photo shows scientist MelissaD
- Page 102 and 103:
30.1 Nuclear Fission 975Applying Ph
- Page 104 and 105:
30.2 Nuclear Reactors 977Courtesy o
- Page 106 and 107:
30.2 Nuclear Reactors 979events in
- Page 108 and 109:
30.3 Nuclear Fusion 981followed by
- Page 110 and 111:
30.3 Nuclear Fusion 983VacuumCurren
- Page 112 and 113:
30.6 Positrons and Other Antipartic
- Page 114 and 115:
30.7 Mesons and the Beginning of Pa
- Page 116 and 117:
30.9 Conservation Laws 989LeptonsLe
- Page 118 and 119:
30.10 Strange Particles and Strange
- Page 120 and 121:
30.12 Quarks 993n pΣ _ Σ 0 Σ + S
- Page 122 and 123:
30.12 Quarks 995charm C 1, its anti
- Page 124 and 125:
30.14 Electroweak Theory and the St
- Page 126 and 127:
30.15 The Cosmic Connection 999prot
- Page 128 and 129:
30.16 Problems and Perspectives 100
- Page 130 and 131:
Problems 100330.12 Quarks &30.13 Co
- Page 132 and 133:
Problems 1005particles fuse to prod
- Page 134 and 135:
Problems 100740. Assume binding ene
- Page 136 and 137:
A.1 MATHEMATICAL NOTATIONMany mathe
- Page 138 and 139:
A.3 Algebra A.3by 8, we have8x8 32
- Page 140 and 141:
A.3 Algebra A.5EXERCISESSolve the f
- Page 142 and 143:
A.5 Trigonometry A.7When natural lo
- Page 144 and 145:
APPENDIX BAn Abbreviated Table of I
- Page 146 and 147:
An Abbreviated Table of Isotopes A.
- Page 148 and 149:
An Abbreviated Table of Isotopes A.
- Page 150 and 151:
Some Useful Tables A.15TABLE C.3The
- Page 152 and 153:
Answers to Quick Quizzes,Odd-Number
- Page 154 and 155:
Answers to Quick Quizzes, Odd-Numbe
- Page 156 and 157:
Answers to Quick Quizzes, Odd-Numbe
- Page 158 and 159:
Answers to Quick Quizzes, Odd-Numbe
- Page 160 and 161:
Answers to Quick Quizzes, Odd-Numbe
- Page 162 and 163:
Answers to Quick Quizzes, Odd-Numbe
- Page 164 and 165:
Answers to Quick Quizzes, Odd-Numbe
- Page 166 and 167:
Answers to Quick Quizzes, Odd-Numbe
- Page 168 and 169:
IndexPage numbers followed by “f
- Page 170 and 171:
Current, 568-573, 586direction of,
- Page 172 and 173:
Index I.5Fissionnuclear, 973-976, 9
- Page 174 and 175:
Index I.7Magnetic field(s) (Continu
- Page 176 and 177:
Polarizer, 805-806, 805f, 806-807Po
- Page 178 and 179:
South poleEarth’s geographic, 626
- Page 180 and 181:
CreditsPhotographsThis page constit
- Page 182 and 183:
PEDAGOGICAL USE OF COLORDisplacemen
- Page 184 and 185:
PHYSICAL CONSTANTSQuantity Symbol V