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High-electric-field limit for the Vlasov–Maxwell–Fokker
High-electric-field limit for the Vlasov–Maxwell–Fokker

... High-field asymptotics have been first analyzed in the kinetic theory of semiconductors in [37], see also [17]. Then, further extensions and mathematical results for different physical models have been obtained in [1], with a discussion based on numerical simulations, [5] for a derivation of so-call ...
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3 Newton`s First Law of Motion—Inertia

Dt © 2013 The McGraw-Hill Companies, Inc. All rights reserved
Dt © 2013 The McGraw-Hill Companies, Inc. All rights reserved

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Problem 16.1 The 20-kg crate is stationary at time t = 0. It is

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3 Newton`s First Law of Motion—Inertia

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< 1 2 3 4 5 6 7 8 9 ... 82 >

N-body problem

In physics, the n-body problem is the problem of predicting the individual motions of a group of celestial objects interacting with each other gravitationally. Solving this problem has been motivated by the desire to understand the motions of the Sun, Moon, planets and the visible stars. In the 20th century, understanding the dynamics of globular cluster star systems became an important n-body problem. The n-body problem in general relativity is considerably more difficult to solve.The classical physical problem can be informally stated as: given the quasi-steady orbital properties (instantaneous position, velocity and time) of a group of celestial bodies, predict their interactive forces; and consequently, predict their true orbital motions for all future times.To this purpose the two-body problem has been completely solved and is discussed below; as is the famous restricted 3-Body Problem.
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