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Simulation of Charged Particle Orbits in Fusion
Simulation of Charged Particle Orbits in Fusion

... 90◦ , and allows us to determine |C| by adding the squares of vy and vz . If we define the perpendicular velocity to be v⊥ ≡ (vy2 + vz2 )1/2 , we get ...
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... free fall accelerates. Every second something is in free fall, it accelerates by 9.8 meters per second. So if an object free falls for two seconds, it would be traveling at 19.6 meters per second. If a piece of paper and a marble are in free fall, they will fall at the same speed, so they should hit ...
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... turn it towards its original direction. The equations of motion to be solved are now (1), (2A) and (3) and the analytical solution is even more complicated. Basically the solution is a damped (or overdamped) oscillatory approach to the equilibrium state if the kite is stable and an oscillation of in ...
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Calculation of an Atomically Modulated Friction Force in Atomic-Force Microscopy.

... on B. In that case, C is given by the elastic constants of A at the interface (7], hence cannot be changed independently. Since c is rather large in many materials, zero friction should be observed for moderate applied loads in the absence of wear and plastic deformations. For a multiatom «tip» whic ...
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... re-taking it at a later time. Tutors are available either for free through the UGA Tutoring Program at Tutors: Milledge Hall, http://tutor.uga.edu, or for pay through the Physics Department, http://www.physast.uga.edu/tutors. NOTE: In physics, learning can be frustrating and nonlinear. Often you hav ...
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Classical central-force problem



In classical mechanics, the central-force problem is to determine the motion of a particle under the influence of a single central force. A central force is a force that points from the particle directly towards (or directly away from) a fixed point in space, the center, and whose magnitude only depends on the distance of the object to the center. In many important cases, the problem can be solved analytically, i.e., in terms of well-studied functions such as trigonometric functions.The solution of this problem is important to classical physics, since many naturally occurring forces are central. Examples include gravity and electromagnetism as described by Newton's law of universal gravitation and Coulomb's law, respectively. The problem is also important because some more complicated problems in classical physics (such as the two-body problem with forces along the line connecting the two bodies) can be reduced to a central-force problem. Finally, the solution to the central-force problem often makes a good initial approximation of the true motion, as in calculating the motion of the planets in the Solar System.
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