Solution
ID: past-exam-of-the-mathematics-course-of-the-university-of-cambridge/2009/iii/paper-62/3/b/solution
Past exam of the mathematics course of the University of Cambridge 2009 iii Paper 62 3 b Solution by
Codex 0 Created 2026-10-03 Updated 2026-10-14
To distinguish the moment quantity from the gravitational constant, write it as . Newton's equations give and . Differentiating provesAverage from to , divide by , and apply the supplied long-time boundary condition. The result isThe PDF's intermediate formula omits this minus sign. It cannot follow from the preceding derivative identity: an attractive inverse-square circular orbit already has and , contradicting the printed positive-sign version. The later homogeneous-potential relation is consistent with the corrected sign.
Interpret as the total pair potential energy, with each pair counted once, for example . The printed pair sum leaves one particle index unspecified; an ordered-pair convention with the corresponding factor absorbed into has the same degree of homogeneity. Under a common dilation of all positions,Differentiating with respect to at one is the Euler theorem for homogeneous functions. Since , it givesSubstitution into the correctly signed averaged identity proves the virial theorem for a homogeneous pair potential:For , the conserved total energy can be evaluated using these averages:Use the kinetic temperature convention , where for three-dimensional thermalized particles, or the same positive coefficient as a kinetic-temperature definition. At fixed particle number and interaction parameters,Thus the equilibrium heat capacity is negative precisely whensubject to existence of the bounded equilibrium sequence assumed by the virial theorem. At the virial energy is zero and this derivative vanishes. At the written power-law potential is constant, its force vanishes, and the bounded-motion virial condition excludes nonzero kinetic energy; division by is not permissible. The Newtonian case recovers .
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