Paper 4, Section I, B

Cosmology | Part II, 2021

A collection of NN particles, with masses mim_{i} and positions xi\mathbf{x}_{i}, interact through a gravitational potential

V=i<jVij=i<jGmimjxixj.V=\sum_{i<j} V_{i j}=-\sum_{i<j} \frac{G m_{i} m_{j}}{\left|\mathbf{x}_{i}-\mathbf{x}_{j}\right|} .

Assume that the system is gravitationally bound, and that the positions xi\mathbf{x}_{i} and velocities x˙i\dot{\mathbf{x}}_{i} are bounded for all time. Further, define the time average of a quantity XX by

Xˉ=limt1t0tX(t)dt\bar{X}=\lim _{t \rightarrow \infty} \frac{1}{t} \int_{0}^{t} X\left(t^{\prime}\right) \mathrm{d} t^{\prime}

(a) Assuming that the time average of the kinetic energy TT and potential energy VV are well defined, show that

Tˉ=12Vˉ\bar{T}=-\frac{1}{2} \bar{V}

[You should consider the quantity I=12i=1NmixixiI=\frac{1}{2} \sum_{i=1}^{N} m_{i} \mathbf{x}_{i} \cdot \mathbf{x}_{i}, with all xi\mathbf{x}_{i} measured relative to the centre of mass.]

(b) Explain how part (a) can be used, together with observations, to provide evidence in favour of dark matter. [You may assume that time averaging may be replaced by an average over particles.]

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