| 1. | For a free non-relativistic particle it follows that
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| 2. | Relativistic particles do not stand still-they just last longer before they decay.
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| 3. | The second approach to the problem of accelerating relativistic particles is the isochronous cyclotron.
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| 4. | :: The Dirac Equation expresses the wave function for a general relativistic particle.
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| 5. | This is the mathematically precise form of the relativistic particle propagator, free of any ambiguities.
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| 6. | Such relativistic particles are generated in particle accelerators, as well as naturally occurring in cosmic radiation.
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| 7. | A charged relativistic particle crossing the interface of two media with different dielectric constants emits transition radiation.
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| 8. | It arises from the observation that accelerating non-relativistic particles with associated magnetic moment emit radiation.
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| 9. | Spin of a relativistic particle moving in a circular orbit precesses similar to the swing plane of Foucault pendulum.
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| 10. | This is why anyone who does any nontrivial relativistic particle modeling uses a computer to do the number-crunching.
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