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Subatomic Physics

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Part III<br />

Symmetries and Conservation Laws<br />

If the laws of the subatomic world were fully known, there would no longer be a<br />

need for investigating symmetries and conservation laws. The state of any part of<br />

the world could be calculated from a master equation that would contain all symmetries<br />

and conservation laws. In classical electrodynamics, for example, the Maxwell<br />

equations already contain the symmetries and the conservation laws. In subatomic<br />

physics, however, the fundamental equations are not yet established, as we shall<br />

see in Part IV. The exploration of the various symmetries and conservation laws,<br />

and of their consequences, therefore provides essential clues for the construction of<br />

the missing equations. One particular consequence of a symmetry is of the utmost<br />

importance: Whenever a law is invariant under a certain symmetry operation there<br />

usually exists a corresponding conservation principle. Invariance under translation<br />

in time, for instance, leads to conservation of energy; invariance under spatial rotation<br />

leads to conservation of angular momentum. This profound connection is<br />

used both ways: If a symmetry is found or suspected, the corresponding conserved<br />

quantity is searched for until it is discovered. If a conserved quantity turns up, the<br />

search is on for the corresponding symmetry principle. One word of warning is in<br />

place here: Intuitive feelings can be misleading. Often a certain symmetry principle<br />

looks attractive but turns out to be partially or completely wrong. Experiment is<br />

the only judge as to whether a symmetry principle holds.<br />

Conserved quantities can be used to label states. A particle can be characterized<br />

by its mass or rest energy because energy is conserved. Or consider the electric<br />

charge, q. It is conserved and comes only in units of the elementary quantum e.<br />

The value of q/e can thus be used to distinguish particles of the same mass. Positive,<br />

neutral, and negative pions can be christened; pion is the family and positive the<br />

first name.<br />

In the next three chapters we shall discuss a number of symmetries and conservation<br />

laws. Additional symmetries exist, and we shall encounter some later on.<br />

Some of the symmetries are perfect even under closest scrutiny, and no breakdown<br />

in the corresponding conservation law has ever been found. Rotational symmetry<br />

and conservation of angular momentum are one example of this “perfect” class.

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