| 1. | The test particles were lost exponentially with a half life of 553 Myr.
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| 2. | That way the potential is independent from the test particle properties.
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| 3. | A stationary spacetime metric, making the orbit of a nearby test particle precess.
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| 4. | The easiest case for the application of a test particle arises in Newtonian gravity.
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| 5. | The Hamiltonian for test particle motion in Kerr spacetime is separable in Boyer Lindquist coordinates.
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| 6. | It is instructive to look at the total relativistic energy of a free test particle.
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| 7. | Calculations showed that when test particles were inserted into it, they flew away from each other.
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| 8. | Where m is the mass of a test particle moving with velocity \ vec { v }.
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| 9. | In fact, test particles do not accelerate toward massive objects in 2 + 1 dimensional general relativity.
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| 10. | We might mention here that in general, the motion of test particles in pp-wave spacetimes can exhibit chaos.
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