| 1. | Also equations of motion can be formulated which connect acceleration and force.
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| 2. | The equation of motion for \ psi is the time differential equation:
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| 3. | Furthermore, the equations of motion impose that the Romans mass is constant.
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| 4. | In Newtonian mechanics, the equations of motion are given by Newton's laws.
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| 5. | Using this plane-wave displacement, the equation of motion becomes the eigenvalue equation
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| 6. | This differential equation is the classic equation of motion for charged particles.
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| 7. | The Liouville space equation of motion governs the observable averages of spin variables.
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| 8. | The equations of motion in general relativity are notoriously hard to solve analytically.
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| 9. | Furthermore, we find the equation of motion for the variable \ alpha as
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| 10. | Instead, we have a more complicated formula ( the equations of motion ).
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