30.6 Positrons and Other Antiparticles 985TABLE 30.1Particle InteractionsInteraction Relative Mediating(Force) Strength a Range of Force Field ParticleStrong 1 Short (1 fm) GluonElectromagnetic 10 2 Long (1/r 2 ) PhotonWeak 10 6 Short (10 3 fm) W and Z bosonsGravitational 10 43 Long (1/r 2 ) Gravitona For two quarks separated by 3 10 17 m.particles is negligible. The gravitational force is by far the weakest of all the fundamentalforces.Modern physics often describes the forces between particles in terms of theactions of field particles or quanta. In the case of the familiar electromagneticinteraction, the field particles are photons. In the language of modern physics, theelectromagnetic force is mediated (carried) by photons, which are the quanta of theelectromagnetic field. Likewise, the strong force is mediated by field particlescalled gluons, the weak force is mediated by particles called the W and Z bosons,and the gravitational force is thought to be mediated by quanta of the gravitationalfield called gravitons. All of these field quanta have been detected except forthe graviton, which may never be found directly because of the weakness of thegravitational field. These interactions, their ranges, and their relative strengths aresummarized in Table 30.1.30.6 POSITRONS AND OTHER ANTIPARTICLESIn the 1920s, the theoretical physicist Paul Adrien Maurice Dirac (1902–1984)developed a version of quantum mechanics that incorporated special relativity.Dirac’s theory successfully explained the origin of the electron’s spin and its magneticmoment. But it had one major problem: its relativistic wave equationrequired solutions corresponding to negative energy states even for free electrons,and if negative energy states existed, we would expect a normal free electron in astate of positive energy to make a rapid transition to one of these lower states,emitting a photon in the process. Normal electrons would not exist and we wouldbe left with a universe of photons and electrons locked up in negative energystates.Dirac circumvented this difficulty by postulating that all negative energy statesare normally filled. The electrons that occupy the negative energy states are said tobe in the “Dirac sea” and are not directly observable when all negative energystates are filled. However, if one of these negative energy states is vacant, leaving ahole in the sea of filled states, the hole can react to external forces and thereforecan be observed as the electron’s positive antiparticle. The general and profoundimplication of Dirac’s theory is that for every particle, there is an antiparticle withthe same mass as the particle, but the opposite charge. For example, the electron’santiparticle, the positron, has a mass of 0.511 MeV/c 2 and a positive charge of1.6 10 19 C. As noted in Chapter 29, we usually designate an antiparticle with abar over the symbol for the particle. For example, p denotes the antiproton andthe antineutrino. In this book, the notation e is preferred for the positron.The positron was discovered by Carl Anderson in 1932, and in 1936 he wasawarded the Nobel prize for his achievement. Anderson discovered the positronwhile examining tracks created by electron-like particles of positive charge in acloud chamber. (These early experiments used cosmic rays—mostly energeticprotons passing through interstellar space—to initiate high-energy reactionson the order of several GeV.) In order to discriminate between positive andnegative charges, the cloud chamber was placed in a magnetic field, causingmoving charges to follow curved paths. Anderson noted that some of theCourtesy AIP Emilio Segre Visual ArchivesPAUL ADRIEN MAURICE DIRAC(1902 – 1984)Dirac was instrumental in the understandingof antimatter and in the unification ofquantum mechanics and relativity. Hemade numerous contributions to thedevelopment of quantum physics andcosmology, and won the Nobel Prize forphysics in 1933.
986 Chapter 30 Nuclear Energy and Elementary ParticlesTIP 30.1 AntiparticlesAn antiparticle is not identified solelyon the basis of opposite charge: evenneutral particles have antiparticles.APPLICATIONPositron EmissionTomographyHIDEKI YUKAWA, JapanesePhysicist (1907 – 1981)Yukawa was awarded the Nobel Prize in1949 for predicting the existence ofmesons. This photograph of Yukawa atwork was taken in 1950 in his office atColumbia University.TIP 30.2 The Nuclear Forceand the Strong ForceThe nuclear force discussed inChapter 29 was originally called thestrong force. Once the quark theory wasestablished, however, the phrase strongforce was reserved for the force betweenquarks. We will follow this convention:the strong force is between quarks andthe nuclear force is between nucleons.UPI/Corbis-Bettmanelectronlike tracks deflected in a direction corresponding to a positively chargedparticle.Since Anderson’s initial discovery, the positron has been observed in a numberof experiments. Perhaps the most common process for producing positrons is pairproduction, introduced in Chapter 26. In this process, a gamma ray with sufficientlyhigh energy collides with a nucleus, creating an electron–positron pair.Because the total rest energy of the pair is 2m e c 2 1.02 MeV, the gamma ray musthave at least this much energy to create such a pair.Practically every known elementary particle has a distinct antiparticle. Amongthe exceptions are the photon and the neutral pion ( 0 ), which are their own antiparticles.Following the construction of high-energy accelerators in the 1950s,many of these antiparticles were discovered. They included the antiproton p, discoveredby Emilio Segrè and Owen Chamberlain in 1955, and the antineutron n,discovered shortly thereafter.The process of electron–positron annihilation is used in the medical diagnostictechnique of positron emission tomography (PET). The patient is injected with aglucose solution containing a radioactive substance that decays by positron emission.Examples of such substances are oxygen-15, nitrogen-13, carbon-11, andfluorine-18. The radioactive material is carried to the brain. When a decay occurs,the emitted positron annihilates with an electron in the brain tissue, resulting intwo gamma ray photons. With the assistance of a computer, an image can be createdof the sites in the brain at which the glucose accumulates.The images from a PET scan can point to a wide variety of disorders in thebrain, including Alzheimer’s disease. In addition, because glucose metabolizesmore rapidly in active areas of the brain, the PET scan can indicate which areas ofthe brain are involved in various processes such as language, music, and vision.30.7 MESONS AND THE BEGINNINGOF PARTICLE PHYSICSPhysicists in the mid-1930s had a fairly simple view of the structure of matter. Thebuilding blocks were the proton, the electron, and the neutron. Three other particleswere known or postulated at the time: the photon, the neutrino, and thepositron. These six particles were considered the fundamental constituents of matter.Although the accepted picture of the world was marvelously simple, no onewas able to provide an answer to the following important question: Because themany protons in proximity in any nucleus should strongly repel each other due totheir like charges, what is the nature of the force that holds the nucleus together?Scientists recognized that this mysterious nuclear force must be much strongerthan anything encountered up to that time.The first theory to explain the nature of the nuclear force was proposed in 1935by the Japanese physicist Hideki Yukawa (1907–1981), an effort that later earnedhim the Nobel prize. In order to understand Yukawa’s theory, it is useful to firstnote that two atoms can form a covalent chemical bond by the exchange ofelectrons. Similarly, in the modern view of electromagnetic interactions, chargedparticles interact by exchanging a photon. Yukawa used this same idea to explainthe nuclear force by proposing a new particle that is exchanged by nucleons in thenucleus to produce the strong force. Further, he demonstrated that the range ofthe force is inversely proportional to the mass of this particle, and predicted thatthe mass would be about 200 times the mass of the electron. Because the new particlewould have a mass between that of the electron and the proton, it was called ameson (from the Greek meso, meaning “middle”).In an effort to substantiate Yukawa’s predictions, physicists began looking forthe meson by studying cosmic rays that enter the Earth’s atmosphere. In 1937,Carl Anderson and his collaborators discovered a particle with mass 106 MeV/c 2 ,about 207 times the mass of the electron. However, subsequent experimentsshowed that the particle interacted very weakly with matter and hence could not bethe carrier of the nuclear force. This puzzling situation inspired several theoreticians
- 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 18 and 19:
27.8 The Uncertainty Principle 891w
- 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 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