By the end of this section, you will be able to:
Conservation laws are critical to an understanding of particle physics. Strong evidence exists that energy, momentum, and angular momentum are all conserved in all particle interactions. The annihilation of an electron and positron at rest, for example, cannot produce just one photon because this violates the conservation of linear momentum. As discussed in Relativity, the special theory of relativity modifies definitions of momentum, energy, and other familiar quantities. In particular, the relativistic momentum of a particle differs from its classical momentum by a factor that varies from 1 to depending on the speed of the particle.
In previous chapters, we encountered other conservation laws as well. For example, charge is conserved in all electrostatic phenomena. Charge lost in one place is gained in another because charge is carried by particles. No known physical processes violate charge conservation. In the next section, we describe three less-familiar conservation laws: baryon number, lepton number, and strangeness. These are by no means the only conservation laws in particle physics.
No conservation law considered thus far prevents a neutron from decaying via a reaction such as
This process conserves charge, energy, and momentum. However, it does not occur because it violates the law of baryon number conservation. This law requires that the total baryon number of a reaction is the same before and after the reaction occurs. To determine the total baryon number, every elementary particle is assigned a baryon number B. The baryon number has the value for baryons, –1 for antibaryons, and 0 for all other particles. Returning to the above case (the decay of the neutron into an electron-positron pair), the neutron has a value whereas the electron and the positron each has a value of 0. Thus, the decay does not occur because the total baryon number changes from 1 to 0. However, the proton-antiproton collision process
does satisfy the law of conservation of baryon number because the baryon number is zero before and after the interaction. The baryon number for several common particles is given in Table 11.2.
| Particle name | Symbol | Lepton number | Lepton number | Lepton number | Baryon number (B) | Strange-ness number |
|---|---|---|---|---|---|---|
| Electron | 1 | 0 | 0 | 0 | 0 | |
| Electron neutrino | 1 | 0 | 0 | 0 | 0 | |
| Muon | 0 | 1 | 0 | 0 | 0 | |
| Muon neutrino | 0 | 1 | 0 | 0 | 0 | |
| Tau | 0 | 0 | 1 | 0 | 0 | |
| Tau neutrino | 0 | 0 | 1 | 0 | 0 | |
| Pion | 0 | 0 | 0 | 0 | 0 | |
| Positive kaon | 0 | 0 | 0 | 0 | 1 | |
| Negative kaon | 0 | 0 | 0 | 0 | –1 | |
| Proton | p | 0 | 0 | 0 | 1 | 0 |
| Neutron | n | 0 | 0 | 0 | 1 | 0 |
| Lambda zero | 0 | 0 | 0 | 1 | –1 | |
| Positive sigma | 0 | 0 | 0 | 1 | –1 | |
| Negative sigma | 0 | 0 | 0 | 1 | –1 | |
| Xi zero | 0 | 0 | 0 | 1 | –2 | |
| Negative xi | 0 | 0 | 0 | 1 | –2 | |
| Omega | 0 | 0 | 0 | 1 | –3 |
For reaction (a), the net baryon number of the two reactants is and the net baryon number of the four products is Since the net baryon numbers of the reactants and products are equal, this reaction is allowed on the basis of the baryon number conservation law.
For reaction (b), the net baryon number of the reactants is and the net baryon number of the proposed products is Since the net baryon numbers of the reactants and proposed products are not equal, this reaction cannot occur.
What is the baryon number of a hydrogen nucleus?
Lepton number conservation states that the sum of lepton numbers before and after the interaction must be the same. There are three different lepton numbers: the electron-lepton number the muon-lepton number and the tau-lepton number In any interaction, each of these quantities must be conserved separately. For electrons and electron neutrinos, for their antiparticles, all other particles have Similarly, for muons and muon neutrinos, for their antiparticles, and for all other particles. Finally, , or 0, depending on whether we have a tau or tau neutrino, their antiparticles, or any other particle, respectively. Lepton number conservation guarantees that the number of electrons and positrons in the universe stays relatively constant. (Note: The total lepton number is, as far as we know, conserved in nature. However, observations have shown variations of family lepton number (for example, in a phenomenon called neutrino oscillations.)
To illustrate the lepton number conservation law, consider the following known two-step decay process:
In the first decay, all of the lepton numbers for are 0. For the products of this decay, for and for Therefore, muon-lepton number is conserved. Neither electrons nor tau are involved in this decay, so and for the initial particle and all decay products. Thus, electron-lepton and tau-lepton numbers are also conserved. In the second decay, has a muon-lepton number whereas the net muon-lepton number of the decay products is . Thus, the muon-lepton number is conserved. Electron-lepton number is also conserved, as for , whereas the net electron-lepton number of the decay products is . Finally, since no taus or tau-neutrinos are involved in this decay, the tau-lepton number is also conserved.
For decay (b), the muon-lepton number of the is 0, and the net muon-lepton number of the proposed decay products is . Thus, on the basis of the law of conservation of muon-lepton number, this decay cannot occur.
What is the lepton number of an electron-positron pair?
In the late 1940s and early 1950s, cosmic-ray experiments revealed the existence of particles that had never been observed on Earth. These particles were produced in collisions of pions with protons or neutrons in the atmosphere. Their production and decay were unusual. They were produced in the strong nuclear interactions of pions and nucleons, and were therefore inferred to be hadrons; however, their decay was mediated by the much more slowly acting weak nuclear interaction. Their lifetimes were on the order of to whereas a typical lifetime for a particle that decays via the strong nuclear reaction is These particles were also unusual because they were always produced in pairs in the pion-nucleon collisions. For these reasons, these newly discovered particles were described as strange. The production and subsequent decay of a pair of strange particles is illustrated in Figure 11.4 and follows the reaction
The lambda particle then decays through the weak nuclear interaction according to
and the kaon decays via the weak interaction
To rationalize the behavior of these strange particles, particle physicists invented a particle property conserved in strong interactions but not in weak interactions. This property is called strangeness and, as the name suggests, is associated with the presence of a strange quark. The strangeness of a particle is equal to the number of strange quarks of the particle. Strangeness conservation requires the total strangeness of a reaction or decay (summing the strangeness of all the particles) is the same before and after the interaction. Strangeness conservation is not absolute: It is conserved in strong interactions and electromagnetic interactions but not in weak interactions. The strangeness number for several common particles is given in Table 11.2.
(b) The following decay is mediated by the weak nuclear force:
Does the decay conserve strangeness? If not, can the decay occur?
What is the strangeness number of a muon?