| Virial Theorem |
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: where r''i'' and '''F'''''i'' are the Position and Force Vector s on the ''i'' th particle respectively. The bar over top of an expression represents time-averaging of the overlined quantity for the entire system. If the force is derivable from a Potential , the theorem becomes :. If ''V'' is a power-law function of ''r'', : or if ''V'' is the sum of terms ''V''''ij''(''r''''ij'') of this form, then the virial theorem can be written as :. In particular, for the further special case of inverse square law forces (i.e. ''n'' = -2), the virial theorem states:
Equivalently:
Since the gravitational force obeys an inverse square law relation, the virial theorem is a remarkably useful simplifying result for otherwise very complex physical systems such as Solar System s or Galaxies , and is also applicable to a number of other similar scenarios. The theorem is also very useful in the theory of gases and can be used to derive Boyle's Law for perfect gases. The virial theorem takes its name from the quantity known as the virial (rooted in the Latin vires, "forces"), defined as: : where r''i'' and '''p'''''i'' are the Position and Momentum Vector s of the ''i''th particle respectively. The virial theorem can be derived by considering the properties of the virial in the limit over a long period of time. In quantum mechanics, the Virial theorem can be written as : UNBOUND CASE Without assuming boundedness we have the following more general properties for gravitational systems:
For two simple cases:
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