30.9 Conservation Laws 989LeptonsLeptons (from the Greek leptos, meaning “small” or “light”) are a group of particlesthat participate in the weak interaction. All leptons have a spin of 1/2.Included in this group are electrons, muons, and neutrinos, which are less massivethan the lightest hadron. Although hadrons have size and structure, leptonsappear to be truly elementary, with no structure down to the limit of resolution ofexperiment (about 10 19 m).Unlike hadrons, the number of known leptons is small. Currently, scientistsbelieve there are only six leptons (each having an antiparticle): the electron, themuon, the tau, and a neutrino associated with each: e e The tau lepton, discovered in 1975, has a mass about twice that of the proton.Although neutrinos have masses of about zero, there is strong indirect evidencethat the electron neutrino has a nonzero mass of about 3 eV/c 2 , or 1/180 000 ofthe electron mass. A firm knowledge of the neutrino’s mass could have great significancein cosmological models and in our understanding of the future of theUniverse.30.9 CONSERVATION LAWSA number of conservation laws are important in the study of elementary particles.Although the two described here have no theoretical foundation, they are supportedby abundant empirical evidence. Baryon NumberThe law of conservation of baryon number tells us that whenever a baryon is createdin a reaction or decay, an antibaryon is also created. This information can bequantified by assigning a baryon number: B 1 for all baryons, B 1 for allantibaryons, and B 0 for all other particles. Thus, the law of conservation ofbaryon number states that whenever a nuclear reaction or decay occurs, the sumof the baryon numbers before the process equals the sum of the baryon numbersafter the process.Note that if the baryon number is absolutely conserved, the proton must beabsolutely stable: if it were not for the law of conservation of baryon number, theproton could decay into a positron and a neutral pion. However, such a decay hasnever been observed. At present, we can only say that the proton has a half-life ofat least 10 31 years. (The estimated age of the Universe is about 10 10 years.) In onerecent version of a so-called grand unified theory (GUT), physicists have predictedthat the proton is actually unstable. According to this theory, the baryon number(sometimes called the baryonic charge) is not absolutely conserved, whereas electriccharge is always conserved. Conservation of baryon numberEXAMPLE 30.4 Checking Baryon NumbersGoal Use conservation of baryon number to determine whether a given reaction can occur.ProblemDetermine whether the following reaction can occur based on the law of conservation of baryon number.p n: p p n pStrategy Count the baryons on both sides of the reaction, recalling that that B 1 for baryons and B 1 forantibaryons.SolutionCount the baryons on the left: The neutron and proton are both baryons; hence, 1 1 2.
990 Chapter 30 Nuclear Energy and Elementary ParticlesCount the baryons on the right:There are three baryons and one antibaryon, so1 1 1 (1) 2.Remarkenergy.Baryon number is conserved in this reaction, so it can occur, provided the incoming proton has sufficientExercise 30.4Can the following reaction occur, based on the law of conservation of baryon number?p n : p p pAnswerNo. (Show this by computing the baryon number on both sides and finding that they’re not equal.)Conservation of lepton number Neutron decay Lepton NumberThere are three conservation laws involving lepton numbers, one for each varietyof lepton. The law of conservation of electron-lepton number states that the sumof the electron-lepton numbers before a reaction or decay must equal the sum ofthe electron-lepton numbers after the reaction or decay. The electron and theelectron neutrino are assigned a positive electron-lepton number L e 1, theantileptons e and e are assigned the electron-lepton number L e 1, and allother particles have L e 0. For example, consider neutron decay:Before the decay, the electron-lepton number is L e 0; after the decay, it is0 1 (1) 0, so the electron-lepton number is conserved. It’s important to recognizethat the baryon number must also be conserved. This can easily be seen by notingthat before the decay B 1, whereas after the decay B 1 0 0 1.Similarly, when a decay involves muons, the muon-lepton number L is conserved.The and the are assigned L 1, the antimuons and are assignedL 1, and all other particles have L 0. Finally, the tau-lepton number L isconserved, and similar assignments can be made for the lepton and its neutrino.n : p e e EXAMPLE 30.5 Checking Lepton NumbersGoal Use conservation of lepton number to determine whether a given process is possible.ProblemStrategyDetermine which of the following decay schemes can occur on the basis of conservation of lepton number.: e : e Count the leptons on either side and see if the numbers are equal. e(1)(2)SolutionBecause decay 1 involves both a muon and an electron, L and L e must both be conserved. Before the decay, L 1and L e 0. After the decay, L 0 0 1 1 and L e 1 1 0 0. Both lepton numbers are conserved,and on this basis, the decay mode is possible.Before decay 2 occurs, L 0 and L e 0. After the decay, L 1 1 0 0, but L e 1. This decay isn’tpossible because the electron-lepton number is not conserved.Exercise 30.5Determine whether the decay : e ecan occur.AnswerNo. (Show this by computing muon-lepton numbers on both sides and showing they’re not equal.)
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Color-enhanced scanning electronmic
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876 Chapter 27 Quantum PhysicsSolve
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27.3 X-Rays 881even when black card
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28.3 Th Bohr Theory of Hydrogen 909
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IndexPage numbers followed by “f
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Current, 568-573, 586direction of,
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Index I.5Fissionnuclear, 973-976, 9
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Polarizer, 805-806, 805f, 806-807Po
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South poleEarth’s geographic, 626
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CreditsPhotographsThis page constit
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PEDAGOGICAL USE OF COLORDisplacemen
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PHYSICAL CONSTANTSQuantity Symbol V